Satellite mission
Organisation (country)
Mission description
Orbit altitude
Civil protection applications
Sentinel-2
European Union
Comprises two polar-orbiting satellites placed in the same orbit, phased at 180° to each other. It provides high-resolution optical data that monitor land surface changes
786 km (sun-synchronous – revisit period five days at the Equator)
Hazards monitoring, risk assessments, impact assessments, damage assessments
TerraSAR-X
DLR/Airbus (Germany)
Provides high-resolution SAR (synthetic-aperture radar) imagery, used in hydrology, geology, climatology, oceanography, cartography and environmental monitoring
514 km (sun-synchronous – revisit period 11 days)
Aeolus
European Space Agency
Carries the atmospheric laser doppler instrument (ALADIN), which collects data on wind profiles at the lowermost 30 km of the atmosphere, to improve weather forecasts and climate models
320 km (sun-synchronous – revisit period seven days)
Early warning systems
Source: Based on Marsellach Pujolràs (2020[5]), .
Figure 2.2 shows that there were some 4 500 operational satellites in orbit in September 2021 (Union of Concerned Scientists, 2021[6]) . Most can be found in LEO and have mainly commercial operators. In terms of applications, communication satellites dominate followed by earth observation and navigation satellites.
1. Refers to academic and other “amateur” operators (e.g. of amateur radio satellites).
Notes: Satellites operational on 1 September 2021. All categories include a small number of dual-use missions (e.g. government-military).
Source: Union of Concerned Scientists (2021[6]) , “UCS Satellite Database: September 2021 update”, https://www.ucsusa.org/nuclear-weapons/space-weapons/satellite-database .
Global commercial revenues reached an estimated USD 271 billion in 2020 and the space sector is increasingly seen as a driver of innovation and growth in the wider economy (OECD, 2019[2] ; Bryce Tech, 2021[7]) . The same year, the US space economy accounted for some 0.5% of national gross domestic product (Highfill, Jouard and Franks, 2020[8]) . The communications industry has historically dominated the space sector in terms of commercial revenues, and expectations of continued high returns in this industry segment are driving private investments and activities. More than ten broadband satellite constellations are in various stages of development, with two companies (SpaceX and OneWeb) having already launched multiple satellites (see Table 2.2). The Starlink constellation had reached more than 1 700 operational satellites by the end of 2021 and offered beta services to a score of countries in Europe, North and South America as well as Australia. Other operators, in North America and the People’s Republic of China (hereafter “China”) in particular, also have projects in the pipeline. In 2021, the Chinese government announced that it would develop a 13 000-satellite Guo Wang (“national network”) broadband constellation. The same year, the Korean defence company Hanwha Systems published plans to develop a 2 000-satellite constellation, to be finalised by 2030. In addition to these planned communications constellations, numerous other projects are underway, often involving much smaller satellites in other applications, such as the Internet of Things or earth observation.
Selected planned communications constellations | |||
---|---|---|---|
Constellation name | Company (country) | Expected number of satellites | Status |
Astra Constellation | Astra Space (United States) | 13 620 | Project announced in 2021 |
Boeing | Boeing (United States) | 132 + 15 (HEO) | Received Federal Communications Commission approval in 2021 |
Guo Wang | China Satellite Network Group (China, People’s Republic of) | 12 992 | Project announced in 2021 |
Hanwha | Hanwha Systems (Korea) | 2 000 | Project announced in 2021, trial services planned to begin in 2023 |
Lightspeed | Telesat (Canada) | 298 | First demonstration launch in 2018 |
Mangata Networks | Mangata Networks (United States) | 791 (HEO) | Prototype development |
OneWeb | OneWeb (United Kingdom) | 648 (6 372) | 358 satellites launched in November 2021 |
Project Kuiper | Amazon (United States) | 3 236 | First satellites scheduled for launch in 2023 |
Sfera | Roscosmos and private contributions (Russia) | 640 | Project announced in 2021, building on previous Efir project |
Starlink | SpaceX (United States) | 11 943 | 1 700+ satellites launched. In 2021 started providing beta services in certain regions |
Yinhe | Galaxy Space (China, People’s Republic of) | 144 | First demonstration launch in 2020 |
Note: HEO refers to high earth orbit (entirely above the geostationary orbit at about 36 000 km), all other projects are in the low-earth orbit. | |||
Source: Adapted from OECD (2019[2]), , . |
Figure 2.3 shows the number of launches and payloads (e.g. satellites, space probes) inserted into orbit since the launch of the first satellite Sputnik in 1957.
Despite a slump in the number of satellites launched after the burst of the dotcom bubble in the late 1990s, the launch rate remained stable over the decades leading to 2019. Since 2019, however, the number of satellites launched has dramatically increased. This is mainly due to SpaceX’s deployment of the Starlink constellation, which in 2021 alone launched 1 000 communications satellites. The number of satellites (or payloads) per launch has increased over time due to smaller satellite size, standardisation of satellite design and improved deployment systems. As an illustration, Starlink and OneWeb satellites are launched in batches of several dozens of satellites – SpaceX can stack more than 50 of its 260 kg Starlink satellites in one launch. But launch frequency would still need to rise quite significantly if multiple mega constellations of several thousand satellites are to be launched and maintained.
The sheer size of these planned mega constellations, leading to an accelerated launch frequency and substantial growth in the number of satellites in orbit, raises new concerns about the environmental sustainability of space activities (Boley and Byers, 2021[9]) . This includes concerns about pollution associated with manufacturing and launch; light pollution from on-orbit satellites disrupting astronomic observations; and, most prominently, space debris’ impact on the stability of the orbital environment. Furthermore, as society’s reliance on space assets grows, so does the vulnerability to space-based hazards, both natural and man-made.
Note: Payloads refer to space objects (e.g. satellites, space probes) designed to perform a specific function in space, excluding launch functionality.
Source: US Space Force (2021[10]) , Space-Track.Org website , https://www.space-track.org .
Space-based infrastructure is exposed to several threats, both natural and man-made. Considering the limited possibility to service and repair satellites once on orbit, even minor events can have severe consequences.
Space weather is closely associated with developments on the Sun and refers to changes in the levels and types of radiation and charged particles and plasma that may affect space-based and terrestrial infrastructure. In its 2015 Space Weather Strategy, the US federal government identified space weather as one of the grand challenges for disaster risk reduction (US National Science and Technology Council, 2015[11]) .
While the Sun constantly emits radiation in the optical and near-infrared range, solar weather events see an increase in the radiation of extreme ultraviolet, X-ray and radio wavelengths (solar flares), as well as the emission of ionised energy particles and plasma (e.g. coronal mass ejections) (Royal Academy of Engineering, 2013[12]) . These events can cause radiation or geomagnetic storms, both of which can seriously affect space-based (and ground-based) activities and infrastructure, producing electrical failure, blocking radio communications, modifying Global Navigation Satellite System (GNSS) signals, etc.
One of the largest geomagnetic storms on record occurred in 1859, disabling telegraph systems in North America and Europe and producing auroras visible in Hawaii and Queensland, Australia. A coronal mass ejection of similar magnitude, potentially with catastrophic consequences, missed the Earth by a week in 2012 (NASA, 2014[13]) . The most recent severe space weather incident took place in Quebec in 1989, when Hydro Québec’s electrical grid was disabled, leaving 6 million people without electricity for nine hours (Canadian Space Agency, 2017[14]) . While minor events are quite common, very little is known about the statistical occurrence of “superstorms,” such as the 1859 Carrington event, named after British astronomer Richard Carrington, who observed it. Various studies indicate a return period of 1 in 100 to 200 years, but these estimates remain highly uncertain because of the lack of historic data (Royal Academy of Engineering, 2013[12]) .
A selection of recent events is listed in Table 2.3.
Selected space weather events since the beginning of the Space Age | |||
---|---|---|---|
Year | Event | Description | Selected reported damages to satellites |
1972 | Solar storm of August 1972, solar particle event | Coronal mass ejection with the fastest transit time to Earth recorded (14.6 hours) that created severe technological disruptions and caused the accidental detonation of numerous naval mines. | |
1989 | March 1989 geomagnetic storm | Caused a nine-hour power outage in the province of Quebec and led to the loss of positional knowledge of space objects for nearly a week. | Multiple satellite anomalies, loss of altitude, signal disruptions |
1991 | Geomagnetic storm, November 1991 | An intense solar storm with about half the energy output of the March 1989 storm. Auroras were visible in the United States as far south as Texas. | |
Bastille Day solar storm, 14 July | Involved a solar flare, solar particle event and a coronal mass ejection, creating a severe geomagnetic storm. Caused minor damage to power transformers and satellites. Strong enough to be observed by Voyager 1 and 2 spacecraft. | Astro-D (ASCA), Japan/United States, scientific satellite in low-earth orbit, loss of altitude | |
2001 | Geomagnetic storm of November 2001 | A fast-moving coronal mass ejection with auroras visible as far south as Texas, California and Florida. | |
2003 | Halloween solar storms, mid-October to early November | Series of solar flares and coronal mass ejections. Auroras visible as far south as Texas and the Mediterranean region. Caused rerouted aircraft and power outages in southern Sweden. | Reportedly some 10% of the total satellite fleet suffered anomalies, including MIDORI 2 (ADEOS), Japan/United States, France scientific satellite in low-earth orbit, anomaly |
2006 | Solar flare, 5 December 2006 | Disrupted satellite-to-ground communications and GPS signals for about ten minutes. | Damaged solar X-ray imager on the GOES-13 weather satellite |
2010 | Coronal mass ejection, 3 April 2010 | Caused a critical failure on the Galaxy-15 communications satellite | |
2022 | Coronal mass ejection, 4 February 2022 | First recorded mass satellite failure caused by an increase in atmospheric density. | 40 out of 49 recently launched Starlink satellites (SpaceX, United States) destroyed on premature re-entry into the atmosphere |
Radiation and geomagnetic disturbances from space weather events can affect space-based infrastructure in several ways. They may cause various satellite malfunctions; degraded or interrupted signals to or from the satellite; loss of altitude (for LEO satellites) due to increased atmospheric drag as it warms and expands; and accelerated aging of components (Abt Associates, 2017[15]) . In recent decades, several events have damaged satellites and disrupted terrestrial electrical and communication networks. In 2006, a solar storm caused a ten-minute disruption to GPS navigation signals (OECD, 2019[2]) . In February 2022, SpaceX reported that a geomagnetic storm caused the loss of up to 40 recently launched Starlink satellites, which lost altitude during orbit-raising and re-entered the atmosphere prematurely (SpaceX, 2022[16]) . However, information on the full impact of space weather on space-based infrastructure is not available, as it may be difficult to distinguish between failures related to space weather events and other malfunctions. Furthermore, operators may sometimes choose not to disclose incidents. According to some academic studies that have compared operator anomaly reports with solar activity, up to 60% of reported anomalies were strongly related to lower energy electron fluxes and to associated magnetic perturbations (Ahmad et al., 2018[17]) .
The World Meteorological Organization co-ordinates the observation of space weather, which currently counts six space-based missions – four US missions and two joint missions between NASA and the European Space Agency – in addition to terrestrial observations (WMO, 2019[18]) . Yet, space weather research and forecasting are still in their infancy and precise forecast horizons (if available) remain short. Coronal mass ejections transit relatively slowly through space and arrival times can be forecast with six to eight hours of accuracy (Royal Academy of Engineering, 2013[12]) . However, definitive forecasts, determining the orientation of the coronal mass ejection magnetic field, are in the 15-30-minute range. In contrast, solar flares and solar energetic particle ejections travel with the speed of light and cannot be forecasted at all. This gives little time to operators of terrestrial and space-based infrastructure to prepare. Satellite operators may mitigate against damage through different types of shielding and satellite design, integrate multiple redundancies and foresee spare satellites (Abt Associates, 2017[15]) . They may also use a higher orbit, but all these measures raise the costs of the mission. It has been argued that the increasingly widespread use of off-the-shelf components (which are cheaper and more easily accessible but not radiation-hardened) can make satellites more exposed to damage (Horne et al., 2013[19]) .
As the Sun progresses in its 25th solar cycle, more intense solar activity is expected in the 2023-26 time frame (NOAA Space Weather Prediction Center, 2022[20]) .
Issues related to the allocation and use of electromagnetic spectrum frequencies is another growing concern for the long-term sustainability of space activities, due to the intensification of space operations and terrestrial competition (OECD, 2019[2]) .
Radio frequencies, used by spacecraft to communicate with other spacecraft and terrestrial ground stations, are often defined as a limited (albeit reusable) natural resource (ITU, 2015[21]) . The International Telecommunications Union ensures equitable access to this resource by allocating frequency bands to individual countries, and mitigates interference issues by reserving specific bands for specific uses (e.g. fixed satellite service uplinks and downlinks).
There are growing concerns of interference from both terrestrial and space networks (e.g. deployment of 5G, the growth of mobile communications worldwide). Concerning the space networks, the sheer size of many planned constellations in LEO raises concerns about orbital interference. Some satellite operators in the geostationary and medium-earth orbits worry that the increasing crowding of the LEO could eventually jam the link between higher flying satellites and terrestrial satellite dishes (OECD, 2019[2]) . Efforts to improve international co-ordination were most recently discussed at the World Radiocommunication Conference in 2019.
Satellites and other types of infrastructure are subject to the risk of collisions with other operational spacecraft, with space debris, and with near-earth objects, such as meteoroids. Of these hazards, collisions with space debris are by far the most pressing and will be further elaborated on in the following sections.
As indicated in the previous sections, the use of Earth’s orbits, and in particular the LEOs, has significantly increased in recent years, as shown in Figure 2.3. This growing number of operational satellites and other spacecraft is accompanied by a growth in orbital debris population (Box 2.2). As a result, not only are the risks of collision between satellites and debris growing, but so are the potential socio-economic impacts of such collisions. There has been a notable increase in the orbital debris population in the last 15 years, associated with three specific events, as shown in Figure 2.4. The figure shows the evolution of space objects catalogued by the US Space Force, including operational and defunct spacecraft, fragmentation debris from collisions and on-orbit explosions (e.g. rocket fuel tanks), mission-related debris such as objects intentionally released during deployment and operations, and various stages of rocket bodies.
The current tracked debris object population is mainly composed of fragmentations from satellites and rockets, followed by defunct spacecraft, rocket bodies and mission-related debris such as lens caps and solid rocket firings. Rocket bodies account for only around 10% of tracked objects, but almost 40% of mass (ESA, 2019[22]) .
Debris belts are located in the low-earth orbit, mainly between 800 and 1 000 km but also at an altitude of almost 1 400 km. There are additional concentrations of space debris close to the orbits of the existing navigation satellite constellations (19 000-23 000 km), and the geostationary orbit, the home of many large telecommunications and weather satellites, at 36 000 km.
Lower altitude orbital debris objects are eventually pulled closer to Earth by atmospheric drag and other natural processes and are in most cases destroyed when entering the atmosphere. Decay timelines can be counted in days (orbits closest to Earth), in years (in orbits less than 600 km), or in centuries (more than 1 000 km). There is no atmospheric drag in higher altitude orbits such as the geostationary orbit and debris remain in orbit unless moved to dedicated “graveyard” orbits.
In November 2021, the US Space Force tracked 19 100 identifiable debris objects mainly with a 10 cm diameter or bigger (US Space Force, 2021[10]) . The total untracked number of debris probably counts in the hundreds of millions (ESA, 2021[23]) .
Source: Based on Undseth, Jolly and Olivari (2020[24]) , “Space sustainability: The economics of space debris in perspective”, https://doi.org/10.1787/a339de43-en .
The first noticeable jump in the debris population followed the intentional destruction of the Chinese weather satellite FengYun-1C in an anti-satellite weapons test in 2007. The second occurred after the first documented collision between two satellites, Iridium-33 and Kosmos-2251 in 2009, and the third jump in 2021 is associated with a Russian anti-satellite weapons test and ensuing break-up of the 2.2 metric tonnes satellite Kosmos-1408. Each of these events created debris clouds of more than 1 000 pieces. Other countries have also conducted anti-satellite tests (e.g. the United States in 1985 and 2008, India in 2019), albeit in lower orbits where debris normally decay within days or weeks.
Concerns about space debris accumulation have been rising over the last four decades. Debris objects and fragments constitute a considerable collision hazard for other spacecraft that are on orbit or travelling through debris belts during orbit-raising. Even tiny debris fragments can cause damage because of their high velocity. Furthermore, debris objects constitute an even higher collision risk for each other because they are not manoeuvrable, generate more debris if they collide and thereby compound the number of collisions (Swiss Re Corporate Solutions, 2018[25]) . Modelling exercises suggest that the likelihood of a collision between an operational geostationary orbit (GEO) satellite and a 1 cm debris object is once every 4 years and once every 50 years for a collision with a 20 cm debris object (Oltrogge et al., 2018[26]) .
Several studies show a significant projected increase in collision risk in the coming decades. A study conducted by Swiss Re in 2018 estimated an eightfold increase (from 11% to 90%) of the risk of collision over the next 20 years between a 200 kg broadband satellite and a 1 cm to 10 cm object in a 1 000-satellite constellation at an altitude of 1 200 kilometres (Swiss Re Corporate Solutions, 2018[25]) . Modelling conducted by the Inter-Agency Space Debris Coordination Committee (IADC) in the 2009-12 time frame predicted an average 30% increase in the amount of LEO debris in the next 200 years, with catastrophic collisions occurring every five to nine years, factoring in a 95% compliance rate to mitigation rules (IADC, 2013[27]) . A 2017 study at the University of Southampton found that adding one mega-constellation of several thousand satellites to low-earth orbit would increase the number of catastrophic collisions by 50% over the next 200 years (University of Southampton, 2017[28]) .
Notes: The three upward jumps in fragmentation debris correspond to: 1) the anti-satellite test conducted by the People’s Republic of China in 2007; 2) the accidental collision between Iridium 33 and Cosmos 2251 in 2009; and 3) the anti-satellite test conducted by the Russian Federation in November 2021. More Cosmos 1408 fragments are expected to be added to the catalogue in the coming weeks and months of 2022.
Source: NASA (2022[29]) , “Orbital Debris Quarterly News 26:1”, https://orbitaldebris.jsc.nasa.gov/quarterly-news/pdfs/ODQNv26i1.pdf .
While collisions with debris could harm individual satellites, the overwhelming concern is that debris density reaches such levels that it triggers an irreversible chain reaction of on-orbit collisions, the so-called Kessler Syndrome (Kessler and Cour-Palais, 1978[30]) . This tipping point may ultimately render certain orbits of high socio-economic value unusable. If or when this could happen remains unknown, but there is a theoretical possibility that it could occur within the next few decades (National Research Council, 2011[31]) .
The impacts of accumulating space debris are distributed across different types of users and are likely to change over time. Current and short-term impacts are relatively limited and affect mainly operators, whereas longer term effects could be much higher in magnitude and will affect broader society.
Currently, public and private operators of satellites and other spacecraft bear the negative consequences of space debris, carrying the costs of avoiding debris and mitigating further debris creation. There are limited data on some of the specific figures relating to these costs, but they vary according to the orbit and type of spacecraft. Table 2.4 provides an overview of the types of costs, typically including damage-related costs, operations and satellite shielding.
Spacecraft replacement costs and related delays and data loss are the most direct consequence of a fatal collision with space debris. However, many other costs can negatively affect a spacecraft’s mass and fuel consumption and hence launch costs and the length of the operational mission life. Actions to address such costs include impact avoidance or reduction measures (e.g. shielding, debris avoidance manoeuvres), as well as debris mitigation measures (e.g. orbit clearance, venting of residual fuel) and other considerations that alter the spacecraft’s design (National Research Council, 2011[31]) .
Overview of current impacts and related costs of space debris | |
---|---|
Type of cost/impact | Description |
Debris-related damage | Loss of functionality or loss of entire satellites. Many incidents go unreported. |
Satellite and constellation design | Costs associated with satellite shielding, collision avoidance capabilities, safehold modes and redundancies (i.e. launch extra satellites as spares). Satellite constellations increasingly include spares for system resilience, but this solution often becomes part of the problem. |
Operations costs | Costs of space situational awareness activities, services and software. Data blackouts when conducting avoidance manoeuvres. |
Orbit clearance costs | In the geostationary orbit: Relatively low, equivalent to about three months of station-keeping. In the low-earth orbit at an altitude above 650 km: Very high and requiring specific satellite subsystems (on-board computer). |
Insurance costs | Overall, limited use of in-orbit insurance by operators for space debris. Space debris collisions have historically been considered low probability and not affecting insurance premiums. |
Source: Based on Undseth, Jolly and Olivari (2020[24]), “Space sustainability: The economics of space debris in perspective”, . |
There are also all the costs associated with debris surveillance, tracking and reporting. Based on research by Oltrogge et al. (2021[32]) , monthly one-kilometre conjunctions (i.e. close encounters with other space vehicles or debris) in LEO may have increased fourfold between 2017 and 2021, from 1 400-2 400 (depending on the data source) average monthly conjunctions to more than 6 000. This puts severe additional stress on individual operators as well as government agencies managing debris and space traffic.
While data are limited, some estimates indicate that costs associated with protective shielding and avoidance manoeuvres may amount to some 5-10% of total mission costs (National Research Council, 2011[31]) . Orbit clearance costs, which depend on the orbit of the satellite, are not included in this estimate. It is presumed that the relative costs of debris mitigation measures are an important determinant of an operator’s compliance with government regulations and guidelines.
As for costs associated with debris-related damage, also here little is known, as only a limited number of operators share information about such events (Table 2.5). This may contribute to creating a false sense of security among operators.
Selected possible debris impact events in LEO | ||||
---|---|---|---|---|
Satellite/event | Country of operator | Altitude | Anomaly date | Details |
SUNSAT | South Africa | 400-838 km | 19/01/2001 | Irreversible multi-point physical failure |
JASON-1 | United States/ France | 1 336 km | 03/2002 | Impulse of 0.365 mm/s from GPS residuals; hit left solar array from behind; lost 10% of array struck; orbit change of 30 cm |
Cosmos 539 | Russia | 1 340-1 380 km | 21/04/2002 | Decrease in period of 1 sec. with a 20 cm x 50 cm object created |
JASON-1 | United States/ France | 1 336 km | 09/2005 | Impulse of 0.182 mm/s from GPS residuals; orbit change of 10 cm |
EOS-Terra | United States | 705 km | 13/10/2009 | One battery cell in hexbay unit and heater failed simultaneously with attitude disturbance; 3 mm impactor suggested |
Aura | United States | 685 km | 12/03/2010 | Solar panel #11 lost 50% of power |
Pegaso | Ecuador | 650-654 km | 22/05/2013 | Close pass to rocket body but no hit |
Iridium-47 | United States | 785-795 km | 07/06/2014 | Ten high velocity (80 m/s) debris produced hinting at impact |
Iridum-91 | United States | 785-795 km | 30/11/2014 | Four low-velocity debris produced insinuating an on-board anomalous event |
WorldView-2 | United States | 770 km | 19/07/2016 | Nine pieces detected, but WorldView says satellite is still working |
Sentinel-1A | Europe | 693 km | 23/08/2016 | Six to eight pieces produced (6 catalogued) and visual verification of solar array damage; impactor of 1 cm and 0.2 gr at 11 km/s |
YunHai 1-02 | China (People’s Republic of) | 780 km | 18/03/2021 | Collision with debris from a Russian Zenit-2 rocket; 37 debris objects detected; satellite remains operational |
Source: Based on Swiss Re Corporate Solutions (2018[25]), “New space, new dimensions, new challenges: How satellite constellations impact space risk”, cited in Undseth, Jolly and Olivari (2020[24]), “Space sustainability: The economics of space debris in perspective”, . |
The longer term costs of space debris could be of a quite different order of magnitude than current costs. In a worst-case scenario, the Kessler Syndrome, as described above, could render certain orbits unusable. This would have considerable negative impacts on the provision of several important government services and would most probably also curb economic growth and further development in the space sector. The societal costs would be unequally distributed, with some rural regions harder hit, given their growing dependence on satellite communications in particular. Regions that have limited surface observations for, e.g. weather forecasting, would also be disadvantaged. These tend to be lower income countries.
Table 2.6 presents a non-exhaustive selection of possible future costs and other impacts of space debris that are discussed in this section.
Selected potential longer term costs of space debris | |
---|---|
Type of cost/impact | Description |
Loss of unique applications and functionalities | Space observations from some of the orbits most vulnerable to space debris are often the best or the only source of data and signals in their domain. This applies in particular to polar-orbiting weather and earth observation satellites. The loss of polar-orbiting weather satellite observations would heavily affect the southern hemisphere, where there are fewer terrestrial observations. |
Growing risks to lives | The International Space Station and the Chinese Space Station are inhabited and located at an altitude of about 400 km. More space stations are under consideration. Although debris at that altitude decays naturally, it still poses a real collision threat. |
Interrupted time series for earth science and climate research | Uninterrupted time series are crucial for the accuracy and reliability of weather prediction and climate models. |
Curbed economic growth and slowdown in investments in the sector | Satellite broadband is widely considered to be a key driver of space activities and revenues in the coming decades. More than ten broadband satellite constellations are in various stages of development. Practically all low-earth orbit communication services would be affected, on orbit and/or during orbit-raising, as most constellations are located near or above the thickest low-earth orbit debris belts. Reduced access to venture finance, with investors preferring more affordable and less risky terrestrial alternatives. |
Distributional effects | The loss or perturbation of certain low-earth orbits could be felt more heavily in rural low-density residential areas and low-income countries. |
Source: Undseth, Jolly and Olivari (2020[24]), “Space sustainability: The economics of space debris in perspective”, . |
Disruption to or loss of certain LEOs would in some cases have severe impacts on terrestrial applications, especially those for which space observations from these orbits are either the best or the only source of data and signals. This applies in particular to polar-orbiting weather and earth observation satellites, which make unique contributions to weather forecasting and climate change observations and research. The orbits most likely to be disrupted by the Kessler Syndrome are found at 650-1 000 km and at an altitude of almost 1 400 km in the low-earth orbit, where the thickest debris belts are also located (Table 2.7).
Affected orbits and space applications | ||
---|---|---|
Application | Altitude | Examples of current missions |
Human spaceflight | 400 km | International Space Station |
Weather forecasting | 800-830 km | All polar-orbiting satellites in the World Meteorological Organization’s Global Observing System, belonging to the People’s Republic of China, Europe, Russia, the United States (e.g. Metop, JPSS) |
Earth observation | 780-900 km | Several earth observation missions, e.g. Sentinel-2/3/5P (Europe), Megha-Tropiques and Saral (France/India), Resourcesat-2 (India). The majority of earth observation missions are in lower orbits (600-700 km). |
Communications (telephony, broadband [future]) | 700-800 km and 1 200-1 400 km | Current low-earth orbit satcom providers include Iridium and Globalstar (United States). Multiple 100+ constellations are planned in the coming years. |
Source: Undseth, Jolly and Olivari (2020[24]), “Space sustainability: The economics of space debris in perspective”, . |
Several services and applications would be considerably affected:
Current human spaceflight activities: The International Space Station and the Chinese Space Station are both located at an altitude of about 400 km. Although debris at that altitude decays naturally, on re-entry into the atmosphere, it still poses a real collision threat. The International Space Station has seen a substantial increase in debris avoidance manoeuvres, with 17 manoeuvres taking place between 2009 and 2017, compared to 8 in the period 1999-2008 (Peters et al., 2013[33] ; Liou, 2018[34]) . In 2020 alone, three manoeuvres were conducted (NASA, 2021[35]) . After the destruction of the Russian satellite Kosmos-1408, the seven-member International Space Station crew had to take shelter in the docked return capsules, to allow for a potential emergency evacuation of the station.
Earth and weather observations: Placing satellites in sun-synchronous orbits (an altitude of about 600-800 km) makes it possible to pass over any given point on Earth at the same time every day, or to place the satellite’s solar panels in constant sunlight. Sun-synchronous orbits are particularly useful for the Earth, weather and climate observation, and military intelligence.
In terms of value and societal benefits, UK estimates of benefits from satellite-based meteorological observations to the UK economy range between GBP 670-1 000 million annually (Innovate UK, 2018[36]) . Polar-orbiting weather satellites provide essential inputs to numerical weather prediction models, reducing errors and improving forecast accuracy (EUMETSAT, 2014[37]) . The loss of polar-orbiting weather satellite observations could particularly affect the southern hemisphere, where there are fewer terrestrial observations. Several weather and earth observation satellites in potentially affected orbits also make unique measurements for climate observations, such as variations in sea surface height, the speed and direction of ocean currents, and heat stored in the ocean. There is also a growing number of commercial earth observation satellites in these orbits (Figure 2.5).
LEO constellations for satellite communications: Practically all current and future LEO communication services could be affected by space debris, on orbit and/or during orbit-raising, as most constellations are located near or above the thickest LEO debris belts. There are currently two commercial communications constellations in the low-earth orbit offering satellite telephony services: Globalstar (at 1 400 km) and Iridium (780 km). So far, the value of commercial operations in LEO is significantly lower than that of telecommunications activities in geostationary orbit. However, as previously noted in this chapter, satellite broadband is widely considered to be a key driver of space activities and revenues in the coming decades, although the profitability and viability of business models remain unproven.
Unequal distribution of effects: The loss or perturbation of certain LEO could be felt more heavily by some groups and geographic regions than others. In some low-income countries, satellite systems may compensate for or complement surface observations or socio-economic survey data. They may furthermore provide connectivity. Indeed, one of the big advantages of space broadband is its ability to connect remotely located areas, including rural regions in both developed and developing countries.
Note: All categories include a small number of dual-use missions (e.g. government-military).
Furthermore, the potential onset of the Kessler Syndrome would most likely curb space sector growth. Investment would probably be diverted to other sectors, with investors preferring more affordable and less risky terrestrial alternatives. Also, demand for existing services and segments, such as manufacturing and launch, would slow down. Chapters 3 and 4 provide theoretical frameworks for identifying and quantifying the different costs of space debris.
In the last 20 years, numerous measures have been taken at both the international level and in individual countries to improve the capacity to track debris and manage space traffic as well as incentivise operators to create less debris in the first place. A fairly recent addition to this policy portfolio is debris remediation, such as active debris removal or attempts to “nudge” debris out of orbital pathways.
Avoiding collisions.
To protect operating satellites and avoid collisions that generate further debris, governments and private actors keep track of their assets and those of other actors, to their best ability. Space situational awareness can be defined as the “knowledge and characterisation of space objects and their operational environment to support safe, stable, and sustainable space activities” (The White House, 2018[38]) . Effective space situational awareness and space traffic management rely on the co-ordinated efforts of military, civilian and commercial operators and space object trackers, all of which hold essential, but incomplete, data and information about the position of their own and others’ space assets. Considering the size of the space environment, this is a daunting task.
The US Space Force has the largest government surveillance and tracking system in place, relying on terrestrial and space-based observatories, and providing conjunction warnings to more than 100 private and government operators worldwide through data-sharing agreements. Other countries (e.g. China, France and the Russian Federation) also have space tracking radars and telescopes. The Indian Space Research Organisation inaugurated a new dedicated control centre for space situational awareness in 2020, underlining the need to enhance national capabilities.
Several regional organisations have countries working together to pool national resources. The International Scientific Optical Network, co-ordinated by the Keldysh Institute of Applied Mathematics in the Russian Federation, is a global network of telescopes for monitoring space debris and other objects, with sensors in more than a dozen countries. In Europe, the European Union supports a Consortium for European Space Surveillance and Tracking (EUSST), with Consortium members providing surveillance and tracking services to all EU countries, institutions, and public and private operators. The China-led Asia Pacific Space Cooperation Organisation, including Bangladesh, Iran, Mongolia, Pakistan, Peru, Thailand and the Republic of Türkiye, is sharing data and developing a network of sensors, the Asia Pacific Optical Space Observation System.
In both GEO and LEO, private capabilities in space situational awareness have also considerably improved over the last decade, with growing deployment of both terrestrial and space sensors and improved software solutions. Other initiatives, such as the Space Data Association, allow commercial satellite operators to share flight dynamics information, which is combined with other space object information and used to provide conjunction assessment and warning services.
Still, current space tracking capabilities have several shortcomings.
Government conjunction assessment services, which are free of charge and commonly used by operators, remain inaccurate and do not provide essential data, such as, for example, debris and satellite object dimensions and mass or spacecraft altitude (Oltrogge and Alfano, 2019[39]) . As a result, operators still need to make their own assessment of the collision risk, and, due to a high and growing frequency of conjunction warnings and notable costs associated with moving the satellite, may choose to ignore some of them. Operators’ interpretation of collision risk is highly subjective.
The United States Air Force currently catalogues and tracks more than 20 000 of the biggest debris objects (10 cm and above). This is deemed to represent less than 0.02% of the total estimated debris population. New sensors, like the recently deployed “Space Fence” observatory, make it possible to detect objects as small as 5 cm in LEO, doubling the space object catalogue (Hejduk, 2019[40]) , but the large majority of potentially harmful debris will remain undetected.
Space tracking organisations rely entirely on the co-operation of space operators to identify space objects. The trend to deploy multiple spacecraft per launch makes this more difficult, as does the increasing number and diversity of operators.
A further complication is the shortcomings in space traffic management. Space traffic management can be defined as “the planning, coordination, and on-orbit synchronisation of activities […]” (The White House, 2018[38]) , managing for instance close encounters between two operational satellites or between an operational satellite and debris. Unlike comparable sectors such as air or maritime traffic, there is a lack of international standardised approaches for space traffic (ESPI, 2020[41]) , as there are:
no protocols handling close conjunctions
arbitrary best practices for collision alerts
ad hoc co-ordination procedures between operators.
National practices vary, but government agencies in Europe and the United States report that current collision avoidance processes are often manual and ad hoc (ESA, 2019[42]) , and that practices for “right of way” are negotiated on a bilateral basis (Foust, 2021[43]) .
Two recent episodes, both incidentally involving SpaceX’ Starlink satellites, illustrate this disquieting situation, where operators rely on e-mails and telephone calls for communication and assess collision risk very differently. In 2019, ESA had to conduct an avoidance manoeuvre for its Aeolus satellite in low-earth orbit, as a Starlink satellite was temporarily lowered to the region already occupied by the Aeolus satellite and came within a distance that surpassed the collision risk probability threshold of 1 in 1 000 (ESA, 2019[42]) . Operators for both satellites were in contact before and after the manoeuvre, but SpaceX later communicated that a communications bug prevented the Starlink operator from seeing the correspondence announcing the increased collision risk probability. In 2021, the UK communications operator OneWeb moved one of its satellites after receiving a close conjunction warning from the US Space Force, and later claimed that SpaceX was either unable or unwilling to move its satellite. SpaceX later reported that the incident was below its probability threshold for executing an avoidance manoeuvre (Foust, 2021[43]) .
Governments across the world are taking steps to address the current situation, but progress is slow, with high stakes involved. Space traffic management has a strong military dimension, which creates its own set of challenges, and, more practically, systems need to be created for data sharing and fusion between agencies and different types of public and private actors. Beyond the aspects of safer space operations, there are also considerable first-mover advantages involved in the regulation of space traffic, favouring national standards and industry practices, as well as ensuring national or regional sovereignty of systems. Consequently, industry associations are mobilising to call for government action (see, for instance, Eurospace (2021[44]) ).
The United States has been working on the reorganisation of space traffic management for several years. It aims to move commercial traffic management from the Department of Defense to the Department of Commerce, as set out in the US Space Policy Directives 2 and 3. The initiative also foresees the creation of an open-architecture data-sharing platform, combining different data from both government and private data sources. The Office for Space Commerce is also tasked with co-ordinating activities across US agencies to create and update standards, practices and guidelines related to debris mitigation and space traffic management, which will be integrated into respective licensing processes. The process was still ongoing in December 2021. In Europe, the European Commission is supporting the SPACEWAYS project that will inform and shape future space traffic management activities in the region.
The strict application of space debris mitigation measures is inevitably needed to preserve the Earth’s orbital environment. But some studies have shown that this in and of itself would not be enough to stabilise the debris population and that debris would need to be actively removed from orbit (Liou and Johnson, 2006[45] ; Liou, Johnson and Hill, 2010[46]) .
Active debris removal faces several technological, geopolitical and economic challenges. It is technologically challenging, as it involves far- and close-proximity operations with (non co-operating) space platforms moving at speeds of several kilometres per second. Success is not guaranteed, and there is a notable risk of further debris creation. It is also very costly, involving the manufacturing and launch of dedicated, disposable, debris removal vehicles. Furthermore, the retrieval of debris could involve sharing potentially sensitive data about the debris object’s design that could involve national security, foreign policy, intellectual property, etc. (National Research Council, 2011[31]) . Therefore, countries would realistically be limited to removing their own satellites or those of close military allies.
A global consortium has put together a “top 50” list of candidates for active debris removal in low-earth orbit, combining several risk factors of high mass, orbit, inclination, etc. (McKnight et al., 2021[47]) . This mainly includes rocket bodies (39 out of the 50, as illustrated in Figure 2.6), several of which weigh several metric tonnes. Launch activity from the former USSR/Russian Federation accounts for 43 out of the 50 objects and 90% of the total mass. The vast majority of objects were launched before 2000.
Source: Based on McKnight et al. (2021[47]) , “Identifying the 50 statistically-most-concerning derelict objects in LEO”, https://doi.org/10.1016/j.actaastro.2021.01.021 .
Despite these underlying challenges, both public and private initiatives are underway, after years of technology development. Several technology demonstration missions are scheduled for the early 2020s, e.g. the ESA’s ClearSpace-1 and the Japanese Commercial Removal of Debris Demonstration (CRD2) mission. Chapter 7 provides a detailed account of the emergence of an active debris removal market.
Alternative solutions that are being explored include “just-in-time” collision avoidance approaches, which could be employed in the case of an imminent collision between derelict objects. The use of space- or ground-based lasers could potentially “nudge” one of the objects out of harm’s way (but it would remain in orbit). Alternative solutions envisage the insertion of an artificial atmosphere in front of one of the colliding debris objects to induce a drag and modify its orbital parameters (Bonnal et al., 2019[48]) . All legal, technological and economic hurdles aside, these approaches depend on a much more accurate capability of space situational awareness and space tracking than exists today.
Considering the current levels of launch activity, operators’ actions to mitigate debris creation are key to stabilising the orbital environment. Voluntary guidelines and recommendations are the main tools for incentivising operators to minimise debris. The first international guidelines were drafted by the IADC in 2001 (Box 2.3). The IADC regroups 13 of the most active space agencies in the world and co-ordinates space debris research and mitigation activities.
One of the most important recommendations is post-mission orbit clearance, i.e. moving post-mission GEO satellites to a graveyard orbit and deorbiting post-mission LEO satellites (or manoeuvring them to an orbit from which natural decay occurs within a maximum of 25 years) (IADC, 2007[49]) . The IADC stipulates that some 90% of future launches would need to comply with orbit clearance guidelines over the next 100 years to stabilise the LEO environment (IADC, 2013[27]) . These efforts have been followed by other international guidelines, recommendations and standards, such as recommendation ITU-R S.1003-2 (2010) for the GEO orbit, or the engineering standards ISO 24113:2019 from the International Organisation for Standardisation.
The Inter-Agency Debris Coordination Committee issued Space Debris Mitigation Guidelines in 2001 and updated them in 2007 (IADC, 2007[49]) . These and similar space agency guidelines aim to:
Limit space debris released during normal operations: Payloads and rocket bodies should be designed to not release debris during normal operations. Where this is not feasible, any release of debris should be minimised in number, area and orbital lifetime. If a spacecraft or orbital stage is to be disposed of by re-entry into the atmosphere, debris that survives to reach the surface of the Earth should not pose an undue risk to people or property.
Minimise the potential for in-orbit break-ups: In all operational regimes, the potential for break-ups during operational phases should be minimised, e.g. increase (sub)system reliability, minimise the potential for post-mission break-ups resulting from stored energy (stored in tanks, batteries, etc.).
Avoid intentional destruction and other harmful activities.
Post-mission disposal in low-earth orbit (LEO) and geostationary orbit (GEO): Permanent or (quasi-) periodic non-functional man-made objects should be cleared from orbit. For payloads in LEO, this involves active or passive deorbiting within 25 years of mission completion. GEO payloads should be moved to a graveyard orbit.
Prevention of in-orbit collisions: Mission projects should estimate and limit the probability of accidental collisions with known objects during the payload or rocket body’s orbital lifetime.
In 2018, the 92 members of the United Nations’ Committee on the Peaceful Uses of Outer Space approved a much wider set of 21 long-term sustainability guidelines (UN COPUOS, 2018[50]) . The guidelines address a range of issues related to space sustainability (e.g. debris, radio frequency spectrum use, space weather) and call for improved registration and supervision of space objects and activities. They also underline the importance of data collection, sharing and modelling for both space debris and space weather incidents.
The first national provisions appeared in the 1990s, and a growing number of countries have integrated the international framework or parts thereof into laws, technical standards, guidelines, etc. (at least 19 countries by the end of 2019 (Undseth, Jolly and Olivari, 2020[24]) ) or are adding new provisions. For instance, in 2019, the United States updated its Orbital Debris Mitigation Standard Practices for the first time since 2001, introducing, among other things, new quantitative limits on debris-producing events and addressing more recent issues such as the operation of cubesats (miniaturised satellites consisting of one or several stacked 10 cm cubes), large constellations and satellite servicing. New Zealand has launched the pilot “Space Regulatory and Sustainability Platform” to track space objects launched from the country and monitor compliance with permit conditions (MBIE, 2019[51]) . France and the United Kingdom require satellite operators to have in-orbit third-party liability insurance. The UK provision includes a risk-based sliding scale (UK Space Agency, 2018[52]) . France, furthermore, introduced legally binding debris mitigation requirements in 2011.
The private sector and society are also taking steps unilaterally. The Space Safety Coalition was formed in 2019 to promote space safety through the voluntary adoption of international standards, guidelines and practices. The coalition, which includes more than 20 space operators, space industry associations and space industry stakeholders, has published a set of “Best Practices for the Sustainability of Space Operations”, building on international guidelines (SSC, 2019[53]) . At the 2021 edition of the Paris Peace Forum, the global governance equivalent to the World Economic Forum in Davos, the Net Zero Space initiative was launched, in which public and private actors pledged to take concrete actions to reduce orbital debris by 2030 (Paris Peace Forum, 2021[54]) . A third initiative is the Sustainable Space Rating, jointly developed by the World Economic Forum, the European Space Agency and the Massachusetts Institute of Technology, together with the BryceTech consultancy group and the University of Texas at Austin and now led by the Swiss Federal Institute of Technology Lausanne in Switzerland. It has specifically been developed to “help reduce space debris and help ensure […] space missions are managed safely and sustainably” (eSpace, 2021[55]) . The rating aims to score space missions based on, for example, “evidence-based debris mitigation and alignment with international guidelines.”
Due to the sometimes considerable time lag between a satellite’s launch and its orbit clearance, it will take time to assess the overall effects of these efforts. Some 20% of French-licensed satellites in LEO with an end-of-life in the 2000-15 range and with a de/re-orbit capacity have so far performed a deorbit manoeuvre, after France made it compulsory in 2011 (Cazaux, 2017[56]) . In Italy, researchers have observed an increased compliance with debris remediation measures after Italy adopted international guidelines in the early 2000s (Anselmo and Pardini, 2015[57]) . Indeed, a positive trend in compliance with orbit clearance guidelines can be observed after 2000, but compliance remains highly dependent on the orbits considered and is generally too low to stop further debris accumulation:
In GEO, satellite clearance surpasses 80% of satellites with an end-of-life in 2019, especially for more recent satellites with an end-of-life after 2000.
In LEO, almost 75% of payloads with an end-of-life in 2019 cleared their orbits. However, for payloads that are not naturally compliant, the share decreased to less than 20% (ESA, 2021[58]) , as shown in Figure 2.7. It has also been argued that the positive signs observed in recent years may be skewed by SpaceX’s good performance in orbit clearance (Boley and Byers, 2021[10]) .
Overall, many commercial LEO operators lack economic incentives to adhere to voluntary guidelines:
As already noted above, actively deorbiting a spacecraft in LEO can be expensive for operators. As a ratio of total mission costs, more fuel is needed for deorbiting or moving a spacecraft in LEO to a lower orbit than to move a spacecraft in GEO to a graveyard orbit. It also requires specific equipment, such as an on-board computer and fuel systems.
Satellites in LEO are becoming increasingly “expendable.” Satellites are becoming relatively affordable to manufacture and launch, often have short mission lives, and are launched in constellations that are more resilient to in-orbit failures and other incidents.
Compliance with guidelines is difficult to control by regulators, who rely on data from satellite operators to identify and name space objects. In addition, non-compliance often bears few or no consequences, especially considering the long time lags between the launch and orbit clearance.
Operators do not have sufficient knowledge to fully calculate and address technical and commercial risks involved in orbital space activities. Although observations and modelling are improving in different parts of the world, the number and nature of objects recorded in existing debris catalogues do not accurately reflect reality.
This stands in contrast to GEO operators, which have a common interest in keeping the orbit as debris-free as possible to avoid collisions, and for which the mitigation measures remain relatively affordable.
Notes: Payloads refer to space objects designed to perform a specific function in space, excluding launch functionality (e.g. satellites, space probes). Payload clearance in the low-earth orbit compliant with debris mitigation guidelines involves deorbiting within 25 years of mission completion. Objects may be naturally compliant (cleared from orbit by atmospheric drag), but clearance above 650 km altitude requires a disposal action for it to occur within the recommended time frame. See also Box 2.2 and Box 2.3.
Source: ESA (2022[59]) , ESA's Annual Space Environment Report 2022 , https://www.esa.int/Safety_Security/Space_Debris/ESA_s_Space_Environment_Report_2022 .
It is important to note that space remains a technologically challenging and failure-prone environment. The share of “insufficient” orbit clearance attempts in LEO varies significantly between years, but can be important. In the last five years, insufficient clearance attempts as a share of total end-of-life payloads fluctuated between some 20% in 2015 and less than 5% in 2020 (ESA, 2022[59]) .
Governments are currently exploring several ways to improve compliance rates, for example through regulations or more market-based approaches, but they lack the evidence to evaluate the effects of different policy options, for instance in terms of socio-economic impacts or levels of popular acceptance. The following chapters address some of these knowledge gaps. Chapters 3 and 4 provide theoretical frameworks for identifying and quantifying the different costs of space debris. Chapter 5 looks at the benefits that space-based earth observation infrastructure brings to specific industry segments in Italy. Chapters 6 and 8 model the effects of different mitigation strategies. Chapter 7 reviews the conditions for creating a market for active space debris removal. Finally, Chapter 9 takes a different approach altogether, looking at how space debris may be reduced through more efficient use of space-based infrastructure.
It follows from the above that for OECD countries and the world as a whole, it is becoming increasingly urgent to better account for and protect space-based infrastructure, as well as the orbital environment.
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[24] Undseth, M., C. Jolly and M. Olivari (2020), “Space sustainability: The economics of space debris in perspective” , OECD Science, Technology and Industry Policy Papers , No. 87, OECD Publishing, Paris, https://doi.org/10.1787/a339de43-en .
[6] Union of Concerned Scientists (2021), “UCS Satellite Database: September 2021 update”, webpage, data as of 1 September 2021, https://www.ucsusa.org/nuclear-weapons/space-weapons/satellite-database (accessed on 20 March 2019).
[28] University of Southampton (2017), “Biggest ever space debris study highlights risk posed by satellite ‘mega-constellations’”, news release, 19 April, https://www.southampton.ac.uk/news/2017/04/space-debris-mega-constellations.page (accessed on 14 March 2019).
[11] US National Science and Technology Council (2015), National Space Weather Strategy , The White House, Washington, DC, https://www.sworm.gov/publications/2015/nsws_final_20151028.pdf (accessed on 24 January 2022).
[10] US Space Force (2021), Space-Track.Org website , 18th Space Control Squadron, update 23 November 2021, https://www.space-track.org (accessed on 23 November 2021).
[18] WMO (2019), “Satellite status” , WMO Space programme website , World Meteorological Organization, https://community.wmo.int/activity-areas/wmo-space-programme-wsp (accessed on 4 June 2018).
This work is published under the responsibility of the Secretary-General of the OECD. The opinions expressed and arguments employed herein do not necessarily reflect the official views of the Member countries of the OECD.
This document, as well as any data and map included herein, are without prejudice to the status of or sovereignty over any territory, to the delimitation of international frontiers and boundaries and to the name of any territory, city or area.
The statistical data for Israel are supplied by and under the responsibility of the relevant Israeli authorities. The use of such data by the OECD is without prejudice to the status of the Golan Heights, East Jerusalem and Israeli settlements in the West Bank under the terms of international law.
Revised version, January 2023
Details of revisions available at: https://www.oecd.org/about/publishing/Corrigendum_Earth-s-orbits-at-risk.pdf
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In the context of increasing space activities, addressing space debris is becoming more important. In April 2020, the OECD Space Forum provided an economic analysis of the issue of space debris by reviewing the most relevant socio-economic impacts and identifying and discussing key sustainability challenges for current and future space activities.
The use of Earth’s orbits has increased significantly in the last decade (e.g. the deployment of mega-constellations among others), and with it, the terrestrial reliance on space-based infrastructure. As a result, vulnerability to space hazards is growing at a fast pace.
At the same time, an orbital environmental crisis is looming, as the space debris population in Earth’s orbits continues to grow. The risk is that collisions between debris ultimately spin out of control, become self-generating and render orbits unusable (i.e. the Kessler Syndrome). This would have severe economic and societal impacts.
Therefore, debris mitigation measures are crucial to ensure orbital environmental stability. National and international measures already exist, however various factors affect levels of compliance with current frameworks and hence their effectiveness (e.g. lack of monitoring capacity and enforcement authority, multiple legal and technological challenges).
To address this issue, OECD is looking into practices in other policy domains for options to increase compliance and suggests possible ways forward for decision-makers.
To learn more about this topic and access more detailed information, please click here .
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With the construction of the International Space Station, humans have been continuously living and working in space for 22 years. Microbial studies in space and other extreme environments on Earth have shown the ability for bacteria and fungi to adapt and change compared to “normal” conditions. Some of these changes, like biofilm formation, can impact astronaut health and spacecraft integrity in a negative way, while others, such as a propensity for plastic degradation, can promote self-sufficiency and sustainability in space. With the next era of space exploration upon us, which will see crewed missions to the Moon and Mars in the next 10 years, incorporating microbiology research into planning, decision-making, and mission design will be paramount to ensuring success of these long-duration missions. These can include astronaut microbiome studies to protect against infections, immune system dysfunction and bone deterioration, or biological in situ resource utilization (bISRU) studies that incorporate microbes to act as radiation shields, create electricity and establish robust plant habitats for fresh food and recycling of waste. In this review, information will be presented on the beneficial use of microbes in bioregenerative life support systems, their applicability to bISRU, and their capability to be genetically engineered for biotechnological space applications. In addition, we discuss the negative effect microbes and microbial communities may have on long-duration space travel and provide mitigation strategies to reduce their impact. Utilizing the benefits of microbes, while understanding their limitations, will help us explore deeper into space and develop sustainable human habitats on the Moon, Mars and beyond.
Introduction.
The National Aeronautics and Space Administration (NASA) has pledged to return humans to the Moon in the next two years and land the first humans on Mars by 2033. The journey beyond low Earth orbit (LEO) will expand human civilization, enable future space settlements, provide scientific knowledge of the evolution of our planet and the solar system, and create global partnerships in the quest for further space exploration 1 , 2 . Under the Artemis plan, a crewed lunar flyby is scheduled for 2024 (Artemis II), followed by a lunar landing in 2025 (Artemis III)—the first since the end of the Apollo era in 1972, and eventually a sustainable lunar presence by the end of this decade 3 . Critical to the success of the Artemis program will be Gateway, an orbiting platform where astronauts will live and conduct research, while providing support for lengthy expeditions on the lunar surface. The Artemis program will establish a base camp at the lunar south pole that will serve as a steppingstone for human missions to Mars. Research and development at the lunar base will act as prototypes for these future Mars missions, where NASA can establish best practices for long-term human exploration in these adverse extraterrestrial environments 4 .
Unlike the operation of the International Space Station (ISS), which is regularly resupplied from Earth within hours after launch, deep space missions will require self-sufficiency and sustainability independent of Earth. This will involve utilization of renewable resources, recycling of waste, power generation, and a continuous supply of food, water, and oxygen over a prolonged/indefinite period. The moon is the shortest distance beyond LEO with a deep space environment offering unique research opportunities to be conducted under the Artemis program. The lunar orbiter Gateway will function similarly to the ISS utilizing a Power and Propulsion Element that will use solar energy to propel and power the spacecraft, a Habitation and Logistics Outpost that will serve as the living quarters and research workspace, and docking ports for spacecraft such as Orion, that will be the first of its kind to transport astronauts to and from deep space 5 , 6 . The ISS and Earth-orbiting satellites capitalize on solar energy as a renewable resource for power, however in more distant outposts such as Mars, other factors like distance from the sun, angle, and weather (i.e., dust storms) affect the efficiency of energy provided by the solar arrays 7 . Such was the case with NASA’s Insight mission, where a recent Martian dust storm led to accumulated dust on the solar panels preventing adequate sunlight from reaching them, forcing the lander into battery-conserving “safe mode” 8 . Similar dust coverage issues were experienced during Apollo missions due to electrically charged lunar dust adhering to solar panels on the lunar lander 9 , 10 . Resupply cargo, like those that are frequently sent to the ISS, is costly, and may not be feasible for long-duration space missions (it takes ~7 months to get to Mars). Thus, self-sustainability in food and oxygen production on extraterrestrial outposts, such as on the Moon and Mars, is crucial 11 . In addition, communication delays between Earth and Mars can range from 5 to 20 min depending on the position of the planets 12 . Lack of cargo resupply missions and communication delays can be detrimental to human health-related emergencies making it imperative for crew members to be self-sufficient in health risk prevention and treatment. Therefore, solutions to address limited resources and human health risks that can be feasibly implemented in deep space must be established prior to the Artemis and Mars exploration missions. This could be achieved through the exploitation and engineering of microbes important to human health 13 , 14 , 15 , 16 , agriculture 17 , food production 18 , 19 , 20 , the ecosystem 21 , 22 , 23 , 24 , 25 , and the built environment 26 , 27 . Figure 1 provides an overview of the various roles microbes could play in deep space exploration.
In this review, we will examine some key considerations for planning crewed space missions that allow for self-sufficiency and sustainability and specifically the role that microbes can play in achieving these goals. We will also discuss the possible detrimental effects of microbes that could derail a mission, such as biofouling and increased pathogenicity, and suggest mitigation strategies to help alleviate some of these concerns.
Space exploration can benefit from the use of microbes in a variety of applications including incorporation into biological life support systems (BLSS), in situ resource utilization beyond LEO, and astronaut therapeutics. However, increased pathogenicity and biofilm formation during spaceflight could threaten astronaut health and spacecraft integrity so mitigation strategies will be needed to prevent such hazards. Microbial applications related to health (purple), renewable resources (green) or both (purple and green) are highlighted. Figure created with BioRender.com.
NASA has been sending astronauts to space for the last 60 years, and with the advent of deep space missions to the Moon and Mars, astronauts must be self-sufficient to provide atmospheric conditions and necessities for human life (i.e., purified water and nutrient-rich food) 28 , 29 . This self-sufficiency can be achieved by implementing bioregenerative life support systems (BLSS). BLSS generate essential resources for human survival through biological processes, with four main purposes: higher plant cultivation, water treatment, solid waste bioconversion, and atmosphere revitalization. Microbes play a vital role in these biological processes by reducing the storage and resupply of materials necessary for a life-sustaining, regenerative environment.
Research on BLSS dates back to as early as the 1960s, by researchers worldwide. Examples include NASA’s “BioHome,” a 650 sq ft closed system that utilized a wetland system for wastewater recycling, and a biological system including plants and microorganisms for reducing organic contamination from wastewater 29 ; the Soviet space program’s Biosphere 3 (BIOS-3), an underground closed system of phytotrons, that consists of a crew area and an entirely enclosed greenhouse, growing wheat and vegetables as well as algae cultivators for air revitalization 30 ; the European Space Agency’s (ESA) Micro-Ecological Life Support System Alternative (MELiSSA), which includes five compartments where plants and microorganisms purify the air, produce food, and recycle waste 31 ; and Beighan University’s Lunar Permanent Astrobase Life-support Artificial Closed Ecosystem (Palace) 1, comprising three cabins that work simultaneously to manage atmospheric conditions, produce crops, breed insects, and recover solid and liquid waste 32 . In all these support systems, microbes are an essential component in the regulation, degradation and circulation of materials and energy, ultimately enhancing the effectiveness of these life support systems.
Research and development of higher plant cultivation, a method of growing crops with increased productivity, enhanced nutritional value, higher volume utilization, and shorter production cycle, are necessary for the development of sustainable ecosystems in space. Higher plant cultivation modules within BLSS not only provide a means for food production but also the recycling and revitalization of air through photosynthesis, and water recycling through transpiration and waste management 33 . Because of their importance, plant modules, and the effects of extraterrestrial conditions on plant growth have been extensively studied 34 , 35 , 36 . For example, NASA is heavily involved in this area of research with its Advanced Plant Habitat (APH) and Vegetable Production System (Veggie) experiments on the ISS. Both APH and Veggie are automated growth chambers used by researchers to determine the effects of microgravity on plant gene expression, protein, and metabolite levels, as well as their nutritional value 37 . The Veggie system has successfully grown lettuce, Chinese cabbage, mizuna mustard, red Russian kale, and zinnia flowers on the ISS 37 and has enhanced our understanding of plant-microbe-environment interactions in microgravity 38 . Using the Veggie system, Hummerick et al. characterized microorganisms found on the leaves of three leafy greens: red romaine lettuce, mizuna mustard, and green leaf lettuce, as well as the microbial communities associated with the rhizosphere in the pillow component 39 . Characterization revealed higher microbial diversity near roots and within root substrate compared to leaves, consistent with plants grown in terrestrial soils. Molecular and culture-based methods revealed that the crops were pathogen-free and safe for human consumption. The information gained from the APH and Veggie experiments, especially as it pertains to plant-microbe interactions, provide a foundation for future research on higher plant cultivation in microgravity and the expansion of these ideas for plant production on extraterrestrial outposts.
One issue with hydroponic growth systems on Earth is microbial contamination, most often by Fusarium oxysporum 40 . Certain abiotic conditions such as high humidity, high temperature, and reduced airflow can cause undesirably high levels of microbial growth 41 , 42 . Veggie is a hydroponic system that has also succumbed to these limitations. Zinnia hybrida , an annual flowering plant, grown in the Veggie system on the ISS, developed foliar, stem, and root rot disease, due to high water stress and low airflow 43 . Whole genome sequencing analysis of the diseased tissue 44 and subsequent virulence assays 43 , identified the culprit as F. oxysporum . This illustrates the potential difficulties of growing crops in hydroponic systems, on Earth or in space.
An alternative to a hydroponic system is a soil-based one where Martian and lunar regolith can be used as an alternative to terrestrial soil. This in situ resource utilization (ISRU) of regolith would reduce the need for costly resupply missions of terrestrial soil. While many plants and crops have been successfully grown in simulated Martian and lunar regolith their characteristics do differ from what would be expected with terrestrial soil 45 , 46 , 47 , 48 , 49 . One limiting factor of regolith is the absence of reactive nitrogen, an essential nutrient for optimal plant growth and function 50 , 51 , 52 , 53 , 54 . However, the introduction of nitrogen-fixing and nitrogen-cycling bacterial species into regolith to bind nitrogen from the atmosphere and transform it into reactive nitrogen (in the form of NO3− and NH4+) could be used as a method to improve regolith soil fertility 55 .
Increased Martian soil fertility through symbiotic relationships has been examined with clover ( Melilotus officinalis ), grown in simulated regolith that had been inoculated with the nitrogen-fixing bacterium, Sinorhizobium meliloti 56 . This study found that after three months, inoculated treatments produced greater clover biomass compared to uninoculated treatments, 0.29 g and 0.01 g, respectively. However, when S. meliloti inoculated clover was grown in common terrestrial potting mix the total clover biomass was seven-fold greater than when grown in simulated regolith 56 . While plant-bacterial symbiosis could improve soil fertility and plant growth in Martian regolith, additional experiments are required to achieve terrestrial levels of plant biomass.
Other plant stressors, such as limited nutrients, may prevent plants from reaching optimal biomass 56 . Essential nutrients, such as potassium, calcium, magnesium, iron, manganese, nickel, and zinc, are present in extraterrestrial soils but not at sufficient levels for plant uptake. Zaets et al. showed that bacteria can increase the bioavailability of these minerals in simulated regolith using inoculants of Pseudomonas sp . IMBG163, Pseudomonas aureofaciens IMBG164, Stenotrophomonas maltophilia IMBG147, Paenibacillus sp . IMBG156, Klebsiella oxytoca IMBG26, and Pantoea agglomerans IMV 45 . When inoculated with these bacteria, increased bioavailability of essential nutrients in the soil and plant tissue of Tagetes patula (i.e., French marigold) led to increased plant growth, seed germination and survival 45 . Conversely, only 20–30% of plants grown in non-inoculated soils achieved seed germination 45 . In addition to increasing nutrient bioavailability, these bacteria were also able to reduce toxic levels of zinc, chromium, nickel, iron, calcium, and sodium, by up to 50%, within plant tissue 45 . By increasing nutrient availability and reducing toxic accumulation of ions within the soil, microorganisms can be used as a tool for conditioning Martian and lunar basalt for effective plant growth and plant nutrient uptake.
Water is another crucial plant resource limited on both the Moon and Mars. Previous discoveries have found evidence of liquid water flows on Mars, coming from giant ice slabs beneath the surface 57 , though extracting and recycling water from these ice slabs is energetically impractical. In addition, Martian soil has limited water-holding capacity due to low organic carbon content, however, this can be improved by using bacteria that produce polysaccharides or adhesive proteins that bind soil particles, thereby increasing the moisture content of soil 58 . This microbe-soil interaction can be exploited on Martian outposts to reduce the need for copious amounts of water, increase soil stability, and prevent soil desiccation. Several studies on agricultural soils show that the application of microalgae and cyanobacteria to the soil can improve soil fertility and health 59 , 60 , 61 . Nascimento et al. assessed the ability of the N-fixing cyanobacteria Nostoc sp . to act as an organic fertilizer and soil conditioner under normal and drought conditions 60 . Researchers applied Nostoc sp . and urea as liquid fertilizers to soil growing wheat ( Triticum aestivum ), corn ( Zea mays ), and common bean ( Phaseolus vulgaris ). Drought conditions were simulated by watering the plant to water holding capacity and drying the soil for 14–16 days. Under drought conditions, plants fertilized with Nostoc sp . reached a biomass 150% greater than plants continuously watered to water holding capacity; while plants fertilized only with urea attained only 70% of the biomass compared to those continuously held at water holding capacity. Researchers also found that untreated soils exhibited more leaf wilting from water stress compared to those plants grown in soil treated with Nostoc sp 60 . This research shows the promise that cyanobacteria can have for improving soil quality for plant growth beyond LEO.
While Martian and lunar regolith are promising soil sources, they contain heavy metals, such as lead, cadmium, chromium, and arsenic, that can negatively impact plant growth and soil microbial fitness 62 , 63 . Microbes can be used for bioremediation to convert Martian and lunar regolith into soil capable of plant growth 64 , 65 , 66 . Huang et al. tested the ability of E. coli and B. subtilis to remove lead, cadmium, and chromium by cultivating samples in solutions containing varying heavy metal concentrations and environmental conditions, including pH, temperature, and equilibration time. Researchers found that both microbes successfully removed heavy metals under all conditions, though under optimal conditions, E. coli removed 60–69% of cadmium, lead, and chromium while B. subtilis removed 54–70% of cadmium, lead, and chromium 67 . Plant-microorganism interactions can also be a source of bioremediation by using plant growth-promoting rhizobacteria that can simultaneously remove toxic heavy metals and improve crop growth and yield 68 . Henao and Ghneim-Herrera investigated this bioremediation method by summarizing results from over 85 research articles and found that Acinetobacter , Agrobacterium , Arthrobacter, Bacillus , Enterobacter , Klebsiella , Mesorhizobium , Microbacterium , Pseudomonas , Rhizobium , Rhodococcus , and Variovorax all exhibited resistance to heavy metals and a high potential for bioremediation. Specifically, Klebsiella and Enterobacter exhibited the highest tolerance to heavy metals in soil and the greatest potential to mitigate plant growth inhibition under high arsenic, cadmium, and lead concentrations 68 . These results are mirrored by Yetunde Mutiat et al. 69 , who assessed the removal efficiency of heavy metals under varying pH levels by wild-type and mutant strains of Klebisella varicola . Isolated Klebisella strains were exposed to various concentrations of lead, cadmium, arsenic, and nickel, resulting in removal of cadmium under all conditions with a maximum removal efficiency of 97.9 and 99.4% at optimal conditions of pH 7 for both wild-type and mutant strains.
Microbes can also be used to remove toxins from Martian soil such as perchlorates, which are found in high levels in Martian soil and cause a significant reduction in plant survival and productivity 70 , 71 . Engineered CO 2 -utilizing bacteria expressing perchlorate reduction enzymes have been shown to remove harmful perchlorates from the soil while also adding essential nutrients into the soil, such as chloride ions, oxygen, and water for better plant growth 72 , 73 , 74 . Sunikumar et al. tested the ability of two perchlorate-reducing soil bacteria, Pseudomonas stutzeri and Azospirillum brasilense , to reduce perchlorates from simulated regolith and found that they removed up to 5 mM and 10 mM of perchlorates, respectively, which corresponded to a removal efficiency of 100% 75 . These results suggest that naturally occurring or genetically engineered microbes with high perchlorate and/or toxin-reducing efficiency should be further studied for bioremediation of perchlorate and other harmful toxins from Martian and lunar soils.
Just as microorganisms are a vital part of terrestrial plant production systems, microorganisms will play an important role in higher plant production and soil systems on future deep space missions and extraterrestrial outposts. Previous research indicates that plant production using hydroponic systems is a promising method for plant production in microgravity 34 , 35 , 36 , but further optimization will be required to prevent fungal contamination in these systems 43 . Using soil-based plant growth systems is a promising alternative to circumvent the limitations of hydroponics, but research is limited in this area within BLSS. Therefore, further research using soil-based plant growth systems, supplemented with microorganisms, may improve the effectiveness of BLSS and self-sufficiency of astronauts on deep space missions.
Water is the largest product consumed in bioregenerative systems, expending nearly 20 L per person per day 76 . Extensive water consumption results in large wastewater production, including urine and flush water, atmospheric condensate, sink, shower, laundry, and dish water. Microbes play a vital role in the recycling of wastewater and nutrients through recycling systems containing combinations of anaerobic digestion, distillation, and disinfectant units.
Microbes also play a crucial role in solid waste processing (including bodily waste), inedible plant material, and other solid decomposable substances within bioregenerative systems. Drying is the first step to recycling solid waste 30 , 32 , 77 . This step allows the extraction of water from solid waste, the retention of organic matter, and the removal of inorganic material 78 . Dried, solid waste is then fermented in a solid waste bioreactor containing microbes that degrade plant waste 32 , 79 , 80 . This method has shown solid waste degradation rates between 41% and 87.7% 79 . The degraded solid waste can either be taken out of the system or applied to a plant system, providing a carbon and nitrogen-rich source of residue fertilizer or soil-like substance that increases soil fertility and overall plant health and productivity 81 , 82 , 83 .
There are many proposed systems for microbe-assisted waste purification and recycling on spacecraft. The MELiSSA initiative proposed a loop of compartments that thoroughly recycle gas, liquid, and solid waste using microorganisms, where each output of the preceding compartment provides the input for the following compartment 84 . Compartment I is an anaerobic digester that utilizes thermophilic bacteria to break down inedible plant parts and solid and liquid waste. Clostridium thermocellum ferments cellulosic substrate, while Clostridium thermosaccharolyticum degrades starches and pectins, leaving volatile fatty acids, minerals and NH 4 + as an output. In compartment II, photoheterotrophic bacteria, such as Rhodospirillum rubrum , metabolize volatile fatty acids. The remaining minerals and NH 4 + enter compartment III where nitrifying bacteria, such as those in the species Nitrobacter or Nitrosomonas , nitrify NH 4 + to NO 3 − , which can be utilized in the plant compartment as a fertilizer 84 . Overall, this system results in a nitrogen-rich output that can be utilized as fertilizer in the plant compartment for improved production.
Another system proposed by Tang et al. utilizes a two-system recycling unit for either domestic water or wastewater 79 . Domestic water is purified by first running it through a two-stage membrane bioreactor and then passing it through a nanofiltration system, to produce hygiene water. The second system utilizes anaerobic, mostly Bacteroidetes, and aerobic, mostly Proteobacteria, microbial bioreactors to recover organic matter and N from wastewater 79 . Within this system, microorganisms are also utilized to degrade solid waste as part of the microbial fermentation facility or Bio-toilet. The facility includes a source separation module that separates urine from feces, a primary bioreactor where feces are combined with other inedible plant material to be degraded by microorganisms, and a secondary bioreactor for further degradation by microbes. This system was tested during 108-day experiment housing four crew members at the China Astronaut Research and Training Center. Researchers achieved 100% water regeneration with 87.7% recycled solid waste 79 , 80 .
Although BLSS can obtain 100% water recovery, nitrogen recovery efficiency is still lacking. One option to improve nitrogen recovery is to utilize urease-producing microorganisms to hydrolyze urea, a compound found in human urine at high levels (>13 g/L) 85 , 86 . Urease-producing microorganisms, such as Bacillus, Sporosarcina, Pseudomonas , and Paracoccus , used in conjunction with membrane-biological activated carbon reactor systems by Xie et al. showed that BLSS can obtain water recovery of 100% with N recovery of up to 79.33%, which are comparable to efficiencies obtained by Tang et al. 79 . Another urine-fueled system for waste recycling, proposed by Maggi et al., includes a soil-based BLSS aimed at recycling liquid wastes using a plant-microbe system 87 . The growth chambers for dwarf wheat and soybean contain three systems for water and urine injection, atmospheric circulation, and ventilation. Once injected into the soil, a number of bacteria can release nitrogen-based intermediates, such as NH 4 + and NO 3 − from organic nitrogen compounds for plants to uptake. Results indicated that urine decomposition met the nutrient demands of the plants as evidenced by successful growth of the dwarf wheat and soybean plants with comparable biomass generation to those grown on Earth.
Plant-microbe systems can provide other methods of wastewater recycling. Plants are excellent water purifiers and can release 2–10 L of water vapor from their leaves through the process of transpiration 88 . Plants uptake water through their roots, absorb nutrients into plant tissue, and transpire water through their stomata. Applying wastewater as a means of watering plants would effectively turn wastewater into clean water through this natural process. However, before plants can be exposed to wastewater, it would need to be pre-treated to reduce organic loading in soil and remove phytotoxic or other detrimental compounds that would affect plant growth and metabolism 89 , 90 . This can be achieved with microbial bioreactors through the mechanisms described above, allowing for eco-friendly water reclamation.
It is projected that crew members on a lunar mission will inhale about 1 kg of O 2 per day and exhale approximately 1.3 kg of CO 2 91 . Production of O 2 and removal of CO 2 during space missions could be achieved through photosynthesis, the process by which plants, algae and cyanobacteria convert CO 2 , sunlight, and water, into O 2 and energy 92 . Cyanobacteria are the earliest oxygenic photosynthetic organisms on Earth and have been contributing to Earth’s atmospheric oxygen for the last 2.5 billion years 93 , 94 . One advantage of using cyanobacteria over plants for air revitalization is their ability to perform photosynthesis with far less sunlight than is required for plant growth. Under normal conditions, plants and cyanobacteria use chlorophyll- a to convert visible (i.e. “white”) light into energy, but some cyanobacteria can perform far-red photosynthesis, using chlorophyll- f , a spectrally red-shifted variant of chlorophyll- a which absorbs longer wavelengths of light 95 , 96 , 97 . This allows those cyanobacteria to also perform photosynthesis and harvest energy when grown in low- or filtered- light environments 95 , 96 , 97 . This photosynthetic efficiency, coupled with the ability to survive the harsh conditions of space 98 , 99 , 100 , 101 make cyanobacteria ideal components in BLSS destined for the Moon and Mars.
Photobioreactors can be incorporated into BLSS to increase the production of oxygen by cyanobacteria or algae for enhanced air revitalization. ESA’s MELiSSA project is a BLSS concept focused on the regeneration of atmospheric gases and water, waste treatment, and food production for crewed space missions 102 , 103 . The system comprises the listed compartments, each with a specific organism contributing to the recycling pathway 104 . One of the five compartments includes a gas-lift photobioreactor containing photosynthetic cyanobacteria, specifically Spirulina platensis , that uses the CO 2 produced by its predecessor compartment to produce oxygen 84 . S. platensis was chosen for its light energy conversion efficiency, its ability to tolerate fluctuations in pH, and its high nutritional value (containing 55–70% protein, 15–25% carbohydrates, 18% essential fatty acids in addition to vitamins, minerals, and pigments 105 ). Another species of cyanobacteria that is being considered for air revitalization, nitrate removal and edible biomass production in MELiSSA is Limnospira indica . In a recent 35-day ground study, L. indica was grown in a simplified closed-loop version of MELiSSA and the effect of urea, ammonium (the prominent nitrogen forms present in non-nitrified urine) and nitrate, on the oxygen production capacity of L. indica , was measured 106 . It was observed that cyanobacteria fed nitrate or urea could effectively reach the desired (set point) O 2 level of 20.3% and maintain ambient O 2 levels, while those fed ammonium could only reach a maximum O 2 level of 19.5% 106 . This study provided preliminary evidence for the use of ammonium-rich and urea-rich media (such as urine), for L. indica cultivation and air revitalization. L. indica has also been grown in photobioreactors on the ISS, as part of the Arthrospira-B spaceflight experiment, and no inhibitory effect on oxygen production and growth was observed, as compared to ground controls 107 .
These studies show the promise of cyanobacteria-based BLSS and/or photobioreactors destined for the Moon and Mars to provide clean air for crew in spacecraft or in lunar/Mars habitats. Additional research is needed for optimization such as identifying additional candidate species, growing combinations of different cyanobacteria for synergistic effects, and testing more growth conditions to achieve enhanced biomass and increased efficiency.
In addition to BLSS which can increase self-sufficiency and sustainability beyond LEO, the ability to utilize in situ resources, will also play a role in long-term human habitats on the Moon and Mars. For instance, electricity and power can be generated with microbial fuel cells (MFC) coupled with in situ organic material, and biomining can be used to extract resources for construction, repair, and maintenance of structural components and equipment.
Microbial production of energy has gained much interest in the last decade. To keep pace with human energy consumption, many scientists have turned towards the use of microbial fuel cells as a sustainable method of energy production on Earth 108 . These alternative methods of energy production could also be applied for space exploration as a sustainable method to power the spacecraft, mission controls, and various life support systems.
MFC are small, lightweight devices that convert organic matter from renewable sources into electricity using microorganisms as catalysts 109 (Fig. 2 ). Microorganisms involved in this electrochemical activity are called exoelectrogens because of their ability to transfer electrons exogenously to electron acceptors 109 . Some examples of exoelectrogens include Pseudomonas 110 , Shewanella 111 , Geobacter 112 , and Desulfuromonas 113 .
MFC consists of two chambers, separated by a proton exchange membrane. In the anode chamber, exoelectrogens, shown as a biofilm in this figure, anaerobically oxidize organic matter releasing protons and electrons. A closer look at this interaction can be seen in the bottom image. The electrons released during the oxidation of organic matter transfer to the anode and travel to the cathode in the second chamber via an external circuit, creating an electrical current. The protons released travel through the proton exchange membrane into the cathode chamber, where the protons and electrons react with oxygen and form water.
The idea behind MFC has been around for over a century, but it is just within the past few decades that it has become a commercialized product. MFC can produce an energy output up to 5.61 W/m 2 114 , 115 , 116 , and can also be used for wastewater recycling, toxin removal, bioremediation, and resource recovery 117 , 118 , 119 , 120 , 121 . These same concepts can be utilized on future Martian or lunar extraterrestrial outposts for energy production and within BLSS. In 2007, de Vet and Rutgers were the first to test the capabilities of MFC energy production under simulated and real microgravity conditions aboard the ISS using Rhodoferax ferrireducens to produce electricity. Energy output averaged 0.1 mA in 1 G, 0.35 mA in simulated microgravity, and 0.02 mA on the ISS. While the differences were not statistically significant, the study did show the potential for MFC to operate in space 122 . This mechanism for energy production is not yet practical for space travel due to the low energy output, considering a standard 40 W light bulb draws 0.36 A to operate, but can be initially utilized for its byproducts, such as clean wastewater 123 .
Waste can accumulate during space travel in the form of urine, fecal matter, and inedible food and with the help of microbes, this waste can be repurposed for energy production as well as for nutrient recovery and production of potable water. Urine is an excellent feedstock for MFC as it contains high levels of urea, organic ammonium salts, and other organic compounds that microbes can convert into electricity 86 thus making urine MFC effective mechanisms for energy production 124 , 125 , 126 , 127 . Some urine MFC can not only produce energy but recover nutrients as well. Lu et al. designed a three-chamber MFC to remove organic pollutants, recover N, phosphorus (P), and sulfur (S), and produce energy from urine 125 . The maximum power output was 1300 mW/m 2 , with almost complete removal of pollutants, including over 97% of urea, total nitrogen, sulfate, phosphate, and chemical oxygen demand, as well as 40% of ammonium, 15% of salts, and 91-99% of organic compounds. The MFC also recovered essential nutrients, including 42% of total N, 37% of phosphate, 59% of sulfate and 33% of total salts 125 . This recovery technology can be especially valuable within other compartments of BLSS, including plant compartments, by providing nutrient-rich water free of contaminants.
In order for urine MFC to also be used as a mechanism to convert urine to potable water, the high level of inorganic salts present in urine (~14.2 g/L) 86 need to first be removed for MFC to function efficiently 125 . This can be achieved with an alternative type of MFC, called a microbial desalination cell, which follows the same concept as a standard MFC but with an added desalination chamber between the anode and cathode 128 . Cao et al. tested this mechanism of water desalination at concentrations comparable to the salinity of urine at 5, 20, and 35 g/L using a mixed bacterial culture, with the salt concentration determined by a change in conductivity of the solution 128 . This microbial desalination cell produced a maximum power output of 2 W/m 2 , with ~88–94% of salt removed, depending on the initial concentration 128 .
Other organic components of wastewater, such as human feces, can be a resource for electricity generation by MFC as well. Fangzhou et al. tested the capabilities of MFC to generate electricity from activated sludge obtained from a sewage treatment plant for specific use within BLSS for future crewed outposts 129 . Tests were performed using a standard or adjustable two-chamber MFC, a one-chamber MFC with one or two membrane electrode assemblies, and a fermentation pre-treatment device. The highest maximum power output was 70.8 mW/m 2 produced by the two-chamber MFC, however, the authors concluded that for space applications, the one-chamber configuration was better, as it produced a more stable output, at 0.3 V 129 . The efficiency of pollutant removal was also tested, with about 44% removal of ammonium and 71% of organic material with each configuration 129 . To further increase power generation and toxin removal from fecal wastewater, fermentation pre-treatment was proposed. This involved using reactors filled with anaerobic sludge to degrade fecal macromolecules into smaller organic molecules 129 . Pre-treating fecal wastewater by fermentation produced 47% more power than no pre-treatment, suggesting a preference of exoelectrogens within MFC for smaller organic molecules 129 . Based on these results, the authors developed an automatic human feces wastewater MFC system containing a fermentation pre-treatment device to simultaneously dispose of one day’s worth of feces and generate electricity. Indeed, the maximum power output of the system was 240 mW/m 2 , about 3.5-fold higher than the standard two-chamber MFC system 129 .
Inedible food waste will be an inevitable part of spaceflight and extraterrestrial outposts on the Moon and Mars that need to be disposed of, as on Earth. This organic material can act as substrates in MFC for energy production, Colombo et al. tested the energy producing capabilities of MFC with various food-industry organic wastes as inputs, including those rich in fibers, sugars, proteins, and acid 130 . A one-chamber MFC was fed each type of organic substrate, and the concentration of organic compounds was measured periodically to obtain the rate of degradation. The maximum power output for each organic waste substrate was 50 mV for sugar, 40 mV for fiber, 30 mV for protein, and 10 mV for acid, with each organic compound degraded by 90% 130 .
While MFC will be a useful tool to create energy and recycle organic waste beyond LEO, research and development is still ongoing to develop more efficient systems with a larger and sustained power output. Some of these ideas involve the use of different materials (such as ceramics) and configurations (large vs small, stacked vs dispersed) 131 . Gajda et al. tested a small (70 mm long, 15 mm diameter, 2 mm thickness) and a large (100 mm long, 42 mm diameter, 3 mm thickness) terracotta MFC. They found that the smaller terracotta MFC achieved a power density output 2.9-fold greater than the large MFC, at 20.4 W/m 3 and 7.0 W/m 3 , respectively. Gajda et al. also tested the performance of stacking MFC for a small-scale multi-unit system that could be utilized on future crewed outposts 132 . They compared power output of a small module containing 28 MFC units and a larger module containing 560 MFC units. Stacked 560 units created a five-fold improvement in power output of 245 mW compared to the 28 MFC unit. Another concept is the PeePower urinals which collect urine and feces directly from the source, producing energy through multiple ceramic MFC 133 . This leads to concentrated wastewater inputted into the MFC rather than diluted samples, which reduces power output. Researchers tested a 288-unit MFC on a university campus which averaged 5–10 users per day. The PeePower urinals were able to produce an average of 75 mW which powered the LED lights directly connected to the MFC stack for 75 h. Another 432-unit MFC was tested during a large music festival which averaged 1000 users per day. In this setting, the PeePower urinals were able to produce an average of 300 mW which successfully powered lighting within the urinals over a seven-day period 133 . While the success of PeePower was demonstrated on Earth, it will be important to test similar models of power generation using urine and feces in microgravity. None the less, this research provides the foundation for the development of similar toilet-like MFC to be used for power generation on deep space missions.
Plant compartments within BLSS can be used for energy production in MFC as well. Healthy soils contain organic matter from decaying plant litter as well as carbohydrate flux directed out of the roots into the rhizosphere 134 . In theory, the anode chamber of a MFC could be positioned within the rhizosphere to capitalize on the symbiotic microbes present to oxidize this continuous source of organic matter to generate an electrical current. Such a soil MFC was tested using rice plants, where 330 W/ha of power was produced in the presence of actively growing plants, a seven-fold higher energy output compared to the energy output of soil MFC not using plants 135 . This technology is not limited to only soil-based systems but can be applied to hydroponic plant systems as well, in which the anode is situated within the water chamber surrounding plant roots 136 . Research by Lee and Miller, growing Bacopa monnieri and with the addition of Escherichia coli , obtained a power density output of up to 1.9 W/m 2 with a 34% increase in plant growth fueled by plant essential nutrients supplied by E. coli acting within the fuel cell 136 . In addition to electricity generation, soil MFC can be used for the remediation of heavy metal contaminated regolith 64 . Habibul et al. tested the ability of soil MFC to remove chromium from soil using ryegrass. The soil MFC was fed a solution of varying concentrations of chromium, resulting in >90% removal efficiency by Proteobacteria and Firmicutes. In addition, the higher the concentration of chromium, the higher the current density output, reaching a maximum of 55 mA/m 2 137 . These results show the promise of energy generation through plant-system powered MFC with the added benefit of increasing plant yield for consumption by crewmembers.
Photosynthetic microorganisms, such as algae or cyanobacteria, can be utilized to convert light energy into electrical energy, termed microbial electrochemical technology 72 . Biophotovoltaics is a specific type of electrochemical technology in which phototrophic microorganisms produce electricity by utilizing incoming light energy to split water molecules, generating electrons and protons that can be used to produce an electrical current within an MFC. Several cyanobacteria species have been tested for use in biophotovoltaics, such as Synechocystis 138 , 139 , Nostoc 140 , 141 , Lyngbya 142 , 143 , and Leptolyngbia 144 , 145 . Kaushik et al. tested the energy producing capabilities of Synechococcus using a two-chamber photosynthetic MFC built with light transparent glass 146 . The MFC operated through a 12-h light/12-h dark cycle under a white light intensity of 15 W/m 2 . Maximum power density output of the photosynthetic MFC was 0.61 W/m 2 146 . This technology provides a feasible method of energy production on extraterrestrial outposts, but further research needs to be completed to increase power output and optimize light conversion.
Research on the use of in situ resources such as wastewater, plant systems, and solar radiation, shows potential for the use of MFC as a mode of power generation and sustainability on extraterrestrial outposts. Though power generation is limited from these substrates at the moment future work may enhance their efficiency. In addition, other sources of power, such as nuclear power, could supplement these MFC systems to provide adequate power generation in habitats and spacecraft beyond LEO 147 .
Biomining is an environmentally friendly and affordable alternative to traditional physical-chemical mineral processing methods to extract metals of economic interest from rock ores or mine waste. The process involves specific microorganisms that secrete organic acids and metal-binding compounds that essentially dissolve these metals, allowing them to be easily extracted from the environment 148 . Biomining is commonly applied to pyritic ores and completed by iron-oxidizing bacteria, such as Thiobacillus ferrooxidans 149 , Leptospirillum ferrooxidans 150 , and Acidimicrobium ferrooxidans 151 . With the reduced iron in the form of pyrite, the bacteria produce iron that oxidizes metal sulfides to sulfuric acid which further accelerates rock dissolution 152 , 153 , 154 . These species, along with those in the Sulfobacillus and Acidianus genera, as well as many iron-oxidizing bacteria, are used for the biomining of copper, zinc, uranium, nickel, aluminum, and cobalt 155 .
The biomining process is not limited to Earth. It may serve as an innovative method for reducing the cost of raw materials and energy requirements beyond LEO, enhancing the sustainability of life on extraterrestrial outposts. Martian and lunar basalt are known to contain many valuable metals, such as iron, nickel, copper, vanadium, and many others, that are suitable substrates that can be biomined by microbes 156 , 157 . Biomining of these metals from Martian and lunar surfaces could provide the necessary materials for the in-situ construction of buildings, electrical systems, spacecraft equipment, solar cells, and heating and lighting systems in human habitats beyond LEO 158 .
Recent research on the ISS simulating biomining of essential compounds from basalt under microgravity demonstrated the possibility for microbial mining beyond Earth 159 , 160 , 161 . Cockell et al. tested the rare Earth element (REE) biomining capabilities of three microorganisms, Sphingomonas desiccabilis, Bacillus subtilis, and Cupriavidus metallidurans , under three different levels of gravity: microgravity, simulated Martian gravity, and terrestrial gravity, and against a non-biological control 160 . Biomining reactions took place within biomining reactors. Within each reactor, researchers placed growth media, sterilized basalt slides with a known REE and single strain cultures of each microorganism. Biomining capabilities were assessed based on absolute quantities of REE in ng obtained from 6 mL bulk fluid collected from the biomining reactors and compared to the non-biological control, consisting of a sterile basalt slide without cell inoculation 160 . REEs assessed include lanthanum, cerium, praseodymium, neodymium, samarium, europium, gadolinium, terbium, dysprosium, holmium, erbium, thulium, ytterbium, and lutetium. The concentration of each REE extracted was proportional to the known abundance in the basaltic rock. At all simulated gravity levels, S. desiccabilis demonstrated enhanced biomining capabilities per gram of basalt substrate, producing 32.52 ng under microgravity, 43.09 ng under Mars gravity, and 32.26 ng under Earth’s gravity, compared to the non-biological mining control, which produced 24.67 ng under microgravity, 21.36 ng under Mars gravity, and 13.25 ng under Earth’s gravity. These values represent the combined mass of biomined REEs. B. subtilis and C. metallidurans demonstrated no differences under the simulated gravity conditions tested and underperformed compared to the non-biological control. As part of the same flight experiment, Cockell et al. tested the biomining capabilities for vanadium (a critical, high-strength element used as a building material), using the same methods and organisms as the Cockell et al. study described above 160 , 161 . S. desiccabilis and B. subtilis increased mined vanadium yield, achieving a two-fold increase in mined vanadium 184.92% and 283.22% under microgravity, 216.32% and 219.78% under Mars gravity, and 208.70% and 221.59% under Earth’s gravity, respectively, compared to the control 160 .
With the abundance of iron in Mars regolith (17.9% wt), iron may be a crucial resource produced through biomining 162 . Iron is one of the most-processed metals on Earth that is incorporated in most building materials and would be heavily relied on for construction, repair, and maintenance of buildings at extraterrestrial outposts. Copper is another important metal that can be produced through biomining, with nearly 20–30% of all copper produced on Earth extracted through biomining 162 . For over 30 years, copper has been an essential metal used in the construction of rocket engines 163 , 164 and being able to extract copper and other minerals from in situ resources on extraterrestrial outposts will allow engine maintenance and repair to occur beyond LEO, reducing the cost and time of sending replacement parts from Earth.
Other economically essential elements have been found in asteroidal material and Martian regolith and can be extracted through biomining 165 , 166 , 167 . These include those in the platinum group, including palladium and osmium, and the 17 REEs. During the Viking Mission to Mars, palladium-silver tubing was utilized in gas chromatography-mass spectrometry to detect organic compounds, and it would be important for future research on Mars in the search for extraterrestrial life 168 . In addition to machinery, REE can be used in building and fixing methods for power generation, specifically solar panels 169 . Lastly, REE are found in electronic screens and fluorescent lights, both necessary for data collection, communication, and the general well-being of those on extraterrestrial outposts 170 .
Bioreactors are necessary for biomining reactions to occur. Terrestrial biomining processes most often occur in open, non-sterile tank reactors that require constant stirring to distribute oxygen and nutrients 171 . To implement biomining on extraterrestrial outposts, it is essential to assess the extent to which differing gravity levels impact microbe-mineral interactions within these stirred-tank bioreactors. An experiment called BioRock, aimed to do this by creating a prototype biomining reactor for space experimentation on the ISS 159 . The biomining reactor has three main components: the culture chamber, the medium reservoir chamber, and a fixative reservoir chamber, where a fixative is injected to halt microbial growth after the biomining reactions take place (Fig. 3 ). Two biomining reactors are placed together within two levels of containment. Pre-test flights found the bioreactors to be successful at growing the model microorganisms, S. desiccabilis, B. subtilis , and C. metallidurans . These microorganisms were chosen as they are low-risk pathogens with the ability to survive desiccation for space flight, limited requirements for growth, and are present in mineral-rich environments. Growth was determined based on optical density in nutrient solution after three weeks. For S. desiccabilis , growth occurred in all tested geometries of biomining reactors, ranging from 0.308 to 0.804 OD 159 . BioRock has also been successfully used to test REE and vanadium biomining capabilities of S. desiccabilis, B. subtilis , and C. metallidurans in microgravity, Mars gravity and Earth’s gravity 160 , 161 .
The biomining reactor has three main components: the culture chamber, the media reservoir chamber, and a fixative reservoir chamber (shown in section 1). The culture chamber is where the biomining reactions take place and where the microorganisms reside before the media is injected. The media reservoir chamber contains the nutrients required for the biomining reaction to occur and is injected into the culture chamber to begin the biomining reaction (section 2). Once the biomining reaction is completed, a fixative is injected to halt microbial growth (section 3).
An additional method of biomining, proposed by Volger et al., utilizes a two-bioreactor system and aims to further enhance ISRU on Martian outposts compared to traditional bioreactors 172 . The first system is an algae bioreactor, which utilizes Chlorella vulgaris to produce biomass for the biomining reactor and oxygen. The algal biomass is then utilized by Shewanella oneidensis as a growth medium in the biomining reactor. In the biomining reactor, S. oneidensis mines iron ores from Martian regolith; the biomass-rich material left over after extraction can then be used for plant growth. Based on modeled algae growth and biomining performance, the system is projected to produce 0.031 kg O 2 per day and 100 kg of iron per Mars year 172 . This model needs to be further tested and future experiments should include exposure to various gravity conditions to assess the impact that this spaceflight stressor will have on growth and performance.
The BioRock experiment and other biomining endeavors using iron-oxidizing and alternative candidate bacteria demonstrate potential for biomining in differing gravity levels and the potential for biomining as a source of ISRU at future Martian and lunar outposts. Biomining for elements known to be located within Martian and lunar regolith, such as iron and REE, will be essential for proper maintenance and production of devices and technology that promote sustainability and provide a foundation by which to launch operations for deep space exploration.
Microorganisms are an important, renewable resource that can be leveraged to produce pharmaceuticals or therapeutics, biological life support systems, and manufacturing materials for human space exploration and colonization that could help reduce the need for costly resupply missions beyond LEO 173 . Candidate microbes can be chosen for these applications based on the availability of genetic tools for manipulation, desired metabolic properties, and tolerance to environmental conditions. These microbes can be further engineered to make them more well-suited for biotechnological applications for interplanetary travel or extraterrestrial settlements using synthetic biology tools. Synthetic biology involves the rational design or repurposing of living organisms and biological systems. Using synthetic biology, microorganisms can be engineered or built de novo with characterized parts and tools to endow them with new or improved functions 173 .
The risk that long-duration space missions pose for crewmembers is not yet completely understood but the extreme conditions, such as microgravity, radiation, and confinement, coupled with microbiome dysregulation may lead to or enhance the disruption of bodily functions 174 . Researchers have studied the effect of simulated or actual spaceflight conditions on gastrointestinal (GI) problems 175 , the development of diseases such as cancer and cardiovascular disorders 176 , or a predisposition to contracting infections 177 , 178 , 179 . The use of probiotics as a countermeasure to combat changes in the microbiome as a result of spaceflight is being investigated to support astronaut health on long-duration space missions 180 , 181 . Probiotics are living organisms able to survive in the gastric environment that provide health benefits and maintain or improve microbiome balance when consumed. On Earth, probiotics have been used to treat many ailments including weight and muscle loss, inflammation, dermatitis, immune disorders, mental health, and GI conditions (i.e., diarrhea, irritable bowel syndrome (IBS), inflammatory bowel disease (IBD)) 180 , 182 .
Promising probiotic candidates for space missions could include Bifidobacterium and Lactobacillus , to counteract their decrease in relative abundance in the astronaut microbiome during spaceflight 183 , 184 . While these species are commercially used on Earth their efficacy and long-term viability when used and stored in space has to still be verified. In 2017, Shao et al. examined the viability of Lactobacillus acidophilus in simulated microgravity and observed no effect on cellular morphology or adhesion. However, some biological changes were present compared to controls, such as increased growth rate at early time points, acid tolerance (pH < 2.5) by ~22–32%, bile tolerance at low concentrations, antibacterial activity, and resistance to antibiotics (i.e., cefalexin, gentamicin, penicillin) 185 . The following year, the shelf life of freeze-dried Lactobacillus casei strain Shirota press-through capsules was tested in spaceflight conditions aboard the ISS 186 . After one month of storage in ambient conditions (i.e., temperature 20–24.5 °C, absorbed dose rate 0.26 mGy/day) and six months after the start of the experiment, bacteria in flight samples were sustained in sufficient numbers that were comparable to ground controls. There were no observed changes in probiotic viability, and the basic probiotic properties of the bacteria including growth rate, carbohydrate fermentation, cell-wall polysaccharide integrity, and resistance to intracellular digestion remained intact upon thawing 186 . A lengthier shelf-life analysis of freeze-dried cells for three commercial probiotics including Bifidobacterium longum, L. acidophilus and spores of B. subtilis was then performed in a simulated three-year round-trip to Mars 187 . In under 200 days, B. longum and L. acidophilus viability was decreased by about 2-logs while B. subtilis maintained viability up to the end of the experiment (545 days). Therefore, researchers concluded that freeze-dried bacterial spores showed the most promise for withstanding long-duration space missions including ambient spacecraft conditions and radiation with an estimated shelf-life of 4.7 years 187 . Overall, these studies provide foundational information on the storage, stability, and viability of probiotic candidates when flown in space. These results suggest that with further testing, probiotic bacteria can be an essential component of the astronaut medical toolkit for the maintenance of a healthy gut microbiome, prevention and treatment of bacterial infections or medical concerns that may arise in future space missions.
In addition to the observed decrease in beneficial bacteria, microbial tracking studies have shown that spaceflight conditions can also lead to an increase in opportunistic pathogens in both the built microbiome and astronaut microbiome. This is particularly problematic due to the dysregulated immunity of astronauts in space 178 . Since antibiotics are the most commonly used therapeutic for the treatment of bacterial infections, researchers are investigating whether microbes can be used for antibiotic production in space. This is particularly relevant considering that antibiotics are known to have accelerated degradation and decreased efficacy when flown and stored in space for long periods of time 188 . On the Space Shuttle Mission STS-77, Lam et al. analyzed the effects of spaceflight on the production of monorden by Humicola fuscoatra WC5157, a marine fungus. Monorden has demonstrated antimicrobial activity against pathogenic fungi and antitumour activity on human tumor cell growth in vitro 189 . Using solid-state fermentation, researchers observed up to 190% increased yield of the antifungal in spaceflight compared to ground controls at 23.8 and 8.2 μg, respectively 190 . Similar results were obtained in another study analyzing the production of actinomycin D, an antibiotic and antitumor agent, by Streptomyces plicatus on the ISS. After 17 days in orbit, the amount of antibiotic produced by ISS samples increased by up to 577% compared to ground controls 191 , and over a 72-day period, researchers noted increased production of actinomycin D in ISS samples specifically at early time points 192 . While much work is yet to be done toward on-demand microbial production of antibiotics in space, these studies demonstrate that microbes are a promising platform for this application. Elucidating the mechanism driving this increased yield early in antibiotic production in microgravity could enable the engineering of bacteria for enhanced antibiotic or therapeutic bioprocessing in space or even be applied to increase antibiotic production on Earth.
Antibiotic-associated diarrhea (AAD) may arise in space as a side effect of administering antibiotics to treat infections. Several studies have investigated the use of Debaryomyces hansenii as a treatment for AAD in a mouse model. D. hansenii is commonly used in the food industry for the processing of cheese and has been identified as part of the human gut microbiome 193 , 194 . When administered for treatment of AAD, D. hansenii alters the composition of the microbiome by promoting the growth of beneficial lactase-producing bacteria and by inhibiting the growth of opportunistic pathogens 195 , 196 , 197 . In one study, the presence of Proteobacteria in the intestinal mucosa increased in response to diarrhea, from ~19% in a normal group to ~36% in an AAD model group, and treatment with D. hansenii was able to restore Proteobacteria to normal levels 195 . Proteobacteria abundance often positively correlates with IBD and inflammation and is generally regarded as an indicator of microbiome instability 198 . In spaceflight, the proportion of Proteobacteria in the astronaut skin microbiome was decreased, namely Gammaproteobacteria and Betaproteobacteria 175 , while it was increased in the salivary microbiome 199 .
While bacterial infections are typically treated with antimicrobials, the formation of biofilms and propagation of multi-drug resistance in the spaceflight environment (discussed later in this review) limits these therapeutic options. A promising alternative currently being investigated on Earth is the use of engineered microorganisms as live biotherapeutics (e.g., biosensors, probiotics with enhanced benefits, and drug delivery systems) 200 , 201 , 202 , 203 , 204 . Well-established microbial chassis organisms include E. coli and Saccharomyces cerevisiae , though a microbe more well-suited to the target therapeutic environment or application can also be chosen. One example using a less conventional chassis was recently performed by Garrido et al. where they engineered Mycoplasma pneumoniae , a human lung pathogen, as a live biotherapeutic to treat S. aureus and other biofilm-associated infections in vivo 205 . Researchers created an attenuated strain of M. pneumoniae able to secrete anti-biofilm and bactericidal enzymes, dispersin B and lysostaphin, and demonstrated its ability to eliminate an S. aureus biofilm in a mouse model 205 . Another candidate chassis that could be employed to eradicate pathogens is D. hansenii , which produces volatile organic compounds and mycocins that have demonstrated antimicrobial effects on several pathogenic bacteria and fungi. An alternative to secreting bactericidal proteins to kill pathogens is the incorporation of CRISPR/Cas9 gene-editing technology into synthetic designs to create engineered probiotics for targeted bacterial killing. This was demonstrated by Neil et al. by delivering CRISPR/Cas9 on a conjugative plasmid which led to 99.9% eradication of antibiotic resistant E. coli and complete eradication of Citrobacter rodentium in the GI tract of a mouse model 206 . CRISPR/Cas9 gene editing has also been demonstrated in D. hansenii 207 , and could be applied to engineer this strain for increased production of mycocins that can target C. albicans 208 , 209 .
Microbes can also be engineered as biosensors to identify or inhibit pathogenic bacteria by sensing an important indicator molecule and releasing a signal or enzyme in response. For instance, biological targeting systems have been demonstrated using engineered E. coli for directed killing of the biofilm-associated pathogen Pseudomonas aeruginosa , a bacterium that has been demonstrated to have increased biofilm formation and pathogenicity on the ISS 210 . Saeidi et al. engineered E. coli with a synthetic genetic circuit containing three modules: sensing, lysing, and killing. The sensing module includes a constitutively expressed transcription factor, lasR , which detects and binds to N -Acyl homoserine lactone (AHL), a quorum sensing molecule released from P. aeruginosa . This bound complex activates the lysing and killing modules expressing lysis E7 and pyocin S5 proteins, respectively. This leads to perforation of the E. coli cell membrane and release of the bacteriocin which targets the pathogen and killed 99% of viable cells 211 . Following this study, Hwang et al. programmed E. coli with a modular circuit containing the same sensing module coupled to a motility and killing module. The motility module expressed the chemotaxis protein CheZ to initiate motility toward the pathogen, while the killing module produced antimicrobial and biofilm-degrading proteins, MccS and DNaseI. Viability of P. aeruginosa was examined and found that E. coli harboring both the motility and killing biosensor modules resulted in the killing of 60% of cells 210 . Biological sensors to detect and/or reduce pathogenic bacteria using traditional chassis such as engineered Lactobacillus or E. coli have also been demonstrated against intestinal P. aeruginosa 212 , vancomycin-resistant Enterococcus 213 , Candida albicans 214 , and S. aureus 215 , 216 . These studies highlight the vast potential of engineered microbes to sense and kill space microbiome-associated pathogens and disrupt biofilms. Since the choice of probiotics is both bacteria- and ailment-dependent 217 , the use of synthetic biology to create genetically engineered biotherapeutics with higher complexity and multiple functions (i.e., able to target multiple pathogens) is vital to minimize the amount of cargo on future space missions. The viability of these therapeutics for humans and their ability to function in the conditions of spaceflight still need to be investigated, but these examples help to shed light on what the next generation of engineered biotherapeutics could offer.
Engineered probiotics can also be a valuable tool for the prevention or detection of more serious health issues such as GI disorders, kidney stones, cancer, and cardiovascular disease (CVD), or the treatment of their associated symptoms. Space-induced changes in the gut microbiome observed in astronauts aboard the ISS by Voorhies et al. included an increase in Parasutterella , a bacteria associated with IBD 175 . In IBD pathology, purinergic receptors are activated by extracellular adenosine triphosphate (eATP) released by commensal gut bacteria and immune cells, promoting intestinal inflammation. Engineered yeast probiotics containing a human P2Y2 purinergic receptor have been developed for the treatment of IBD by responding to physiological eATP levels and secreting the eATP-degrading enzyme apyrase 218 . This probiotic was shown to be effective in a mouse model of IBD, decreasing intestinal inflammation and dysbiosis. Bacterial probiotics can also be engineered to detect gut inflammation by sensing tetrathionate, thiosulfate or nitric oxide 219 , 220 , or with programmable memory systems to detect and respond to an environmental stimulus 221 .
The risk of kidney stones due to bone decalcification, dehydration, or increased growth rate of calcium-depositing nanobacteria 222 , 223 , 224 is increased in spaceflight, which could also be prevented or treated using probiotics. Calcium oxalate is the major component of kidney stones, therefore ideal probiotic bacteria are efficient in oxalate degradation, such as Oxalobacter formigenes 225 and B. subtilis . B. subtilis strain 168 has been presented as a novel probiotic therapy as it has been shown to break down the oxalate in kidney stones in a Drosophila model 226 . The oxalate decarboxylase (OxDC) enzyme derived from B. subtilis can also be used to engineer other bacteria as probiotics for the treatment of kidney stones. The expression and subsequent purification of this enzyme in E. coli was able to reduce oxalate concentrations in a mouse model in urine and feces by 44% and 72%, respectively, compared to controls 227 . The OxDC gene was also introduced into Lactobacillus plantarum on a plasmid, leading to expression and secretion of this enzyme where it was able to degrade 70–77% of oxalate in vitro, and reduced oxalate as well as calcium, uric acid, creatinine, serum uric acid, and BUN/creatinine ratio in urine compared to controls in a rat model 228 .
Probiotics including Lactobacillus and Bifidobacterium can also be used to improve cardiovascular health by reducing weight, cholesterol, and adipose tissue while also preventing or attenuating injuries to the heart (e.g., heart failure, ischemia, cardiac hypertrophy) 229 . Using a rat model, Lactobacillus rhamnosus or a placebo was administered to subjects following coronary artery occlusion for a six-week duration. Compared to placebo controls, rats given the probiotic treatment showed attenuation of left ventricular hypertrophy, improved systolic and diastolic left ventricular function, and additional improvements up to six weeks after withdrawing treatment 230 . Other Lactobacillus species have had positive effects on CVD including L. plantarum which helped to reduce serum levels of leptin and fibrinogen, which are CVD risk factors 231 . These probiotics can also be genetically engineered to enhance their potential benefits. For instance, E. coli Nissle 1917 has been genetically engineered to produce N-acylphosphatidylethanolamines which, when administered to mice, led to decreased adiposity, insulin resistance and lipid accumulation in the liver 232 . This has important implications for astronauts as spaceflight can induce negative, aging-like effects on the cardiovascular system (i.e., decreased fitness, arterial stiffening, and insulin resistance) and radiation exposure has been well-characterized to increase the risk of developing radiation-induced cardiovascular disease (RICVD) 233 , 234 .
Crewmembers are at an elevated risk of cancer development due to radiation and other spaceflight factors 235 , 236 , 237 . As such, methods for cancer prevention and treatment are important to implement during deep space exploration and bacterial-mediated cancer therapies could be a promising approach Bacteria can be used naturally or engineered for cancer therapy to specifically target and colonize tumors, or as a drug delivery system for anticancer agents 238 . Many bacteria have been investigated for these applications including Bifidobacterium 239 , E. coli 240 , 241 , 242 , Clostridium 243 , 244 , Salmonella 245 , 246 , 247 , 248 , 249 , and Streptococcus 250 species. A study using E. coli engineered with synthetic adhesins to target a tumor antigen in vivo found that lower doses of engineered E. coli were required to colonize tumors compared to wild-type controls 240 . Tumor targeting was also demonstrated in an attenuated strain of Salmonella typhimurium harboring a short hairpin RNA expression plasmid. It was engineered to target inhibin, a tumor marker, resulting in significant inhibition of colon cancer and melanoma growth in a mouse tumor model 247 . Bacteria can also be engineered to improve tumor and metastasis visualization within mammalian hosts, facilitating their use as diagnostic and therapeutic microbial agents. For example, E. coli was engineered to express an acoustic reporter gene allowing them to be imaged noninvasively in vivo and to produce protein-nanoparticle gas vesicles for targeted breast cancer therapy 242 . E. coli was also engineered with lacZ , encoding the β-galactosidase reporter, which can be easily detected in urine as an indicator of liver metastasis 251 .
Bacteria hold great potential for the development of easily modifiable biotherapeutics that could be invaluable for treatment or prevention of health issues during long-duration space missions. However, additional research and clinical validation is necessary before employing engineered bacteria as biotherapeutics for space-associated disorders and diseases.
BLSS can provide crew members with oxygen, food, and water, and will be imperative for long-duration space missions and for the establishment of sustainable human habitats on the Moon or Mars. Due to their diverse applications for spaceflight, microalgae and cyanobacteria are often studied for their incorporation in BLSS and photobioreactors. They produce oxygen, remove carbon dioxide from the environment and help with water purification 104 , 105 , 252 , 253 . These microbes are also edible allowing their biomass to provide nutritional and therapeutic benefits without the need for protein purification 35 , 254 .
Oxygen for astronauts on the ISS is currently transported in pressurized tanks from Earth or is produced using water onboard through electrolysis 255 . Therefore, the ability to improve carbon uptake and oxygen output using microbes on the ISS, for space travel and in future extraterrestrial habitats, is an essential step toward the creation of sustainable and self-sufficient systems. Oxygen production, CO 2 capture, and photosynthetic capacity could be enhanced in BLSS using synthetic biology tools to address the bottleneck of photosynthesis: the carbon fixation cycle. Metabolic engineering of cyanobacteria can improve photosynthetic capacity as demonstrated by Berepiki et al. where expression of mammalian cytochrome P450 (CYP1A1) acting as an electron sink in Synechococcus PCC 7002 improved photosynthetic efficiency and increased electron flow rate by ~30% 256 . Using the same cytochrome P450 gene, Santos-Marino et al. engineered metabolic pathways for sucrose production and cytochrome P450 as a carbon and electron sink, respectively, into Synechococcus elongatus . Ultimately, this resulted in increased photosynthesis, and simultaneous expression of both sinks had an additive effect on photosystem I oxidation and photosystem II efficiency 257 . Another strategy to improve this cycle is by increasing the substrate concentration of ribulose-1,5-bisphosphate carboxylase-oxygenase (RuBisCo) to improve carbon uptake. In the cyanobacterium Synechocystis sp. PCC6803, one study found that genetic installation of additional bicarbonate transporters resulted in a 2-fold increase in carbon uptake and biomass 258 . Metabolic engineering of cyanobacteria can also be used to produce industrially relevant high-value chemicals and bioproducts such as biofuels. Some engineering efforts have been demonstrated in the model cyanobacteria species, S. elongatus PCC7942 and Synechocystis sp. PCC6803, to produce ethanol, ethylene, isobutyraldehyde, and isoprene 259 , 260 , 261 , 262 . The biotechnologically relevant bacteria, Ralstonia eutropha (i.e., C. necator ) has also been engineered by Dogutan and Nocera to capture CO 2 to produce biofuels and edible biomass, in an artificial photosynthetic cycle that is much more efficient than those that are naturally occurring 263 .
In addition to oxygen, microalgae can provide a sufficient source of proteins, carbohydrates, fatty acids, minerals, and vitamins required for a balanced diet 264 , 265 . These nutritional outputs can be further enhanced using synthetic biology approaches. Genome editing technologies for these marine species have expanded over the last 20 years, namely due to improvements in DNA sequencing, manipulation techniques and availability of genomic information 266 . Some of these methods and technologies include DNA delivery via conjugation, the generation of auxotrophic strains, and DNA-free or plasmid-based genome editing (e.g., using CRISPR/Cas9) 267 , 268 , 269 , 270 . Therefore, it is possible to create cell factories using metabolic engineering to alter the composition or nutritional output of these species 271 , 272 , 273 . For example, mutagenesis and CRISPR/Cas9 gene editing technologies have been used to modify the biomass composition of the model algae species Chlamydomonas reinhardtii . Irradiated mutant strains have been generated with double the starch content compared to the wild-type strain through increased expression of phosphoglucomutase 1 (PGM1) and decreased expression of downstream enzymes in the glycolytic pathway 274 . C. reinhardtii has also been engineered to knock out the zeaxanthin epoxidase gene resulting in 47-fold increased production of the carotenoid zeaxanthin, which is important in the prevention of macular degeneration 275 , a concern facing astronauts during prolonged spaceflight 276 .
Synthetic biology approaches are also being used to genetically engineer microorganisms for the production and long-term storage of nutrients as part of NASA’s BioNutrients projects 277 . Nutrient production and storage on long-duration space missions is a challenge as they can degrade over time. Therefore, this project aims to develop a system for on-demand microbial production of micronutrients on the ISS, whereby packages of dehydrated, edible yeast can be hydrated and consumed. In the first segment of the project, BioNutrients-1, Saccharomyces cerevisiae and S. boulardii species were engineered to produce antioxidants with genes for zeaxanthin and beta-carotene biosynthesis pathways, respectively 277 . The S. boulardii genome was also engineered to stimulate increased trehalose stores and with tardigrade-derived cytosolic abundant heat soluble (CAHS) genes, both resulting in increased tolerance to desiccation. Along with these strains, several other edible microorganisms are being tested for their storage and survival in stasis packages in the ambient conditions of the space environment. These include yogurt-producing and milk-coagulating bacteria ( Lactobacillus delbrueckii subsp. bulgaricus, Streptococcus salivarius subsp. thermophilus, B. subtilis and Bacillus coagulans ), yeasts ( Kluyveromyces lactis and Komagataella phaffii Kurtzman ) and C1-utilizing bacteria ( Methylobacterium extorquens and C. necator) . The production and stasis packages were delivered to the ISS and will be analyzed for growth and nutrient expression for a five-year duration. After 47 days, initial stasis package data showed no significant difference in the viability of bacteria stored on the ISS compared to ground controls 278 . These organisms are all attractive candidates for biological engineering to produce vitamins, therapeutics, or other useful enzymes for maintaining crew health. In addition to continued testing of the production of carotenoids, BioNutrients-2 279 aims to further develop the bioproduction system from BioNutrients-1 by expanding the variety of probiotic products on the ISS to include yogurt and kefir and investigate the production of follistatin by the engineered yeast K. lactis 279 . The results of the BioNutrients project will provide invaluable information for the feasibility of using microbes as a platform for nutrient storage and production for long-term space travel.
In-space manufacturing and development can be challenging as necessary materials and supplies are not readily available and currently need to be transported or resupplied from Earth. Microbes offer a solution as they can be reprogrammed for the production of biologically derived materials (i.e., bioplastics, nanomaterials) 280 to generate useful components such as plastics, adhesives, composites, and rubbers for structural space applications.
One material that would be beneficial to produce in situ beyond LEO is aerogels. Aerogels, first created by Kistler in 1931, are human-made, low-density solid materials with an interconnected porous network composed of 99.8% air, with the most common type being silica-based 281 . Photosynthetic organisms that can produce silica, primarily algae diatoms ( e.g., Phaeodactylum tricornutum ), are of interest for the generation of silica-based aerogels and have recently been incorporated into cellulose aerogel composites 282 , 283 . Aerogels are useful materials for space applications due to their low thermal conductivity, light weight, and high porosity 284 , 285 , 286 . To improve the habitability of other planets for humans and photosynthetic organisms, silica aerogels provide the benefit of allowing for the transmission of visible light for photosynthesis while simultaneously blocking hazardous UV radiation 284 . In addition, since aerogels are a thermally insulating material, they can raise surface temperatures through the solid-state greenhouse effect 284 . NASA is currently taking advantage of the thermal insulating properties of aerogels to protect spacecraft and rovers from the cold Martian surface temperature, such as for the Mars Pathfinder lander, Mars exploration rovers (Spirit and Opportunity) and Mars Science Laboratory mission (Curiosity rover) 286 . Aerogels have also been used as a method for capturing particles from space without damaging them, as demonstrated in the Stardust Mission 286 . Therefore, using a synthetic biology approach to generate aerogels from silica-producing organisms could be interesting to investigate further.
Other gel-based materials can also be synthesized using synthetic biology. For instance, Kim et al. took advantage of the structural properties of synthetic spider silk 287 , 288 and mussel adhesive proteins, which can act as biological adhesives 289 , 290 , to engineer E. coli with a spidroin-amyloid-mussel foot hybrid protein that can ultimately assemble into a hydrogel with high strength and underwater adhesion 291 . The hybrid protein consisted of a zipper domain from an amyloid protein, a flexible domain from spider silk, and a dihydroxyphenylalanine (DOPA)-containing mussel foot protein. This is a great example of how synthetic biology can be used to generate bacterial hosts expressing recombinant proteins with novel or desirable functions and properties, which can be applied to tackle specific manufacturing challenges in space. In addition, methods to spatially control the distribution of microbial cells into hydrogel structures have been developed using a Stereolithographic Apparatus for Microbial (SLAM) Bioprinting 3D printer 292 . Bioresins composed of synthetic polymers were used to contain the microorganisms and mimic extracellular polymeric substances (EPS) that are fundamental to biofilm formation in nature 293 . The power of this technology was demonstrated by printing engineered Caulobacter crescentus as uranium biosensors within this biomaterial using a uranium responsive promoter fused to GFP and measuring the fluorescence output 292 . This technology could enable genetic engineering of single strains, microbiomes, and biofilms to be used not only for biomanufacturing but also for biomining, biotherapeutics, and bioremediation.
Plastic materials continue to play a vital role in the manufacturing of spacesuits and spacecraft. Progress has been made towards the sustainable production of high-strength, biodegradable plastics in engineered microorganisms. Specifically, efforts have been made to increase the production of polyhydroxyalkanoate (PHA) or polyhydroxybutyrate (PHB) in engineered cyanobacteria, Synechococcus 294 and Synechocystis sp. PCC6803 295 , 296 . Synechocystis sp. PCC6803 has been engineered with the PHA biosynthetic pathway of R. eutropha (i.e., Cupriavidus necator) 296 or the overexpression of sigE 295 to increase PHA and PHB production, respectively. Metabolic engineering of the shikimate pathway in B. subtilis or S. cerevisiae for the increased production of para -aminobenzoic acid (pABA) has also been studied, which can act as a precursor for high-strength polymers (e.g., aramid fibers) 297 , 298 . Ultimately, these biologically derived materials can be used to manufacture parts or even 3D-print hardware in space 299 .
To make in-space manufacturing and construction off-planet more sustainable, ISRU or recycling of existing material components to produce feedstock for new materials is necessary 300 . Microorganisms offer a solution to this problem as many can naturally degrade polymers for metabolic products. Black fungi, which are a diverse group of extremophilic melanized fungi, have been investigated for this application due to their demonstrated ability to hydrolyze synthetic polymers 301 ). For instance, Aureobasidium pullulans , a black fungus, has demonstrated microbial deterioration of plasticized polyvinyl chloride (PVC) and dioctyl adipate plasticizers 302 . Knufia chersonesos , another black fungus, has been shown to completely break down the synthetic copolymer polybutylene adipate terephthalate (PBAT) 303 . Secretome screening identified seven polyesterase enzymes that could potentially be involved in this observed polymer degradation, which lays the foundation for the possibility of further engineering of this biosynthetic pathway for more efficient degradation 303 . Therefore, this group of extremophilic organisms are promising candidates for plastic degradation, however, this process still needs to be investigated in simulated or spaceflight microgravity.
Microgravity studies of K. cheronesos that analyzed the effects of simulated microgravity on the proteome and secretome found that scytalone dehydratase gene expression was upregulated in the wild-type strain and downregulated in a melanin-deficient mutant strain 304 . This enzyme is involved in the biosynthesis of dihydroxynaphthalene melanin, which is believed to have protective qualities that fungi use to withstand the extreme conditions of space 305 . This suggests that Knufia species, and potentially other black fungi have the properties to withstand space conditions and are good candidates for plastic degradation in space. Since then, various other extremophilic fungi have been tested for their survival in space, through exposure to simulated Mars conditions 306 , 307 . These include 12 Chernobyl-isolated strains (i.e., Cladosporium , Acremonium , Beauveria , Fusarium , Trichoderma , Penicillium , Aureobasidium , Aspergillus and Apiospora ), the black fungi Exophiala jeanselmei , and the microcolonial fungi Cryomyces antarcticus and Knufia perforans . Plastic degradation has also been investigated in extremophilic bacteria, for example Streptomyces thermoviolaceus , Geobacillus thermocatenulatus and Clostridium thermocellum 308 . As these extremophilic fungi and bacteria have been shown to withstand space conditions, thus they are promising candidates to use or engineer for plastic degradation in space. Ultimately, the capacity for manufacturing in space will be beneficial for long-duration space missions, reducing the need to bring materials as cargo or have them launched from Earth, and allowing for on-demand production of materials based on immediate need.
Astronauts venturing out beyond Earth’s protective magnetosphere will be exposed to hazardous radiation during deep-space exploration missions. This includes high-energy electromagnetic waves from our sun such as UV radiation, gamma, and X-rays or sub-atomic particles from the cosmos (electrons, protons, neutrons, and heavy metal ions), known as galactic cosmic radiation. These forms of radiation strip electrons from molecules resulting in protein or DNA damage through production of reactive oxygen and nitrogen species 309 , 310 . The result is short-term or long-term health problems such as cancer, acute radiation sickness, radiation-induced cardiovascular disease, and neurological damage 278 . Developing a solution for passive radiation protection for astronauts will be a critical step towards sustaining long-term presence on the Moon and Mars. The average person on Earth is exposed to about 6.2 mSv of radiation over a period of a year, while the average astronaut on the ISS is exposed to approximately 144 mSv 311 . One year into a three-year mission to Mars, an astronaut would already have been exposed to some 400 mSv of radiation 311 , 312 . Due to the complex nature of space radiation, there is likely no one-size-fits-all solution to this problem. Some proposed architectural concepts for radiation production include building below ground in lava tubes or piling meters of regolith outside of a structure 313 , 314 and while materials like lead and aluminum may be effective, they would be costly to transport 315 . As a result, the search for innovative radiation shields will depend in part on biotechnology, which holds unique advantages such as suitability for ISRU, self-regeneration, and adaptability. By selecting model organisms such as extremophiles, that use radiation as an energy source, we can begin to understand their properties and refine testing for technology development.
Fungi on Earth have been isolated in high-radiation environments, such as the contamination zone of the Chernobyl Nuclear Power Plant 316 , 317 , inside the ISS 317 , and exteriors of spacecraft in LEO 305 . Analogous to phototrophy, fungi appear to perform radiosynthesis, using pigments known as melanin to convert gamma radiation into chemical energy 318 , 319 . Melanin has the capability to absorb electromagnetic radiation, resist acids, and perform powerful antioxidant activity allowing some fungi to thrive in the most extreme environments on Earth or beyond, including those with high levels of ionizing radiation 320 , 321 . Studies examining the survival rates of melanized and non-melanized yeasts with gamma radiation have shown that melanin-rich fungi were able to shield ionizing radiation at efficacies comparable to lead and twice as effective as charcoal, whereas the non-melanized strains lacked the capability to provide shielding 322 . This may not only be due to the presence of melanin itself but the spatial arrangement of it within the cell, as it was observed that in Cryptococcus neoformans , melanin arranged in a spherical shape, covering the inner surface of the cell membrane, resulted in superior shielding from radiation 323 , hypothesized to be due to the increase in scattering of incident photons 318 . Melanin is not the sole mechanism by which fungi survive radiation exposure. In a study using melanized yeast Exophiala dermatitidis , it was found that nutrient availability, culture density, metabolic state and DNA repair mechanisms were better determinants of cell survival after gamma radiation exposure than melanin 324 . Other mechanisms that protect fungi against radiation involve enzymes that remove reactive oxygen species or those that promote DNA repair, either through nucleotide excision or photoreactivation 325 , and various other secondary metabolites, such as the antioxidant pyranonigrin A 326 . Due to the ability of various fungi to withstand, thrive, and even attenuate space-relevant doses of radiation 306 , 316 , 318 , 327 , 328 , 329 , 330 there is keen interest in their use for the development of radiation-resistant shields or structures 305 , 330 , 331 , 332 .
Fungal mycelium, a filamentous network of hyphae, is a fibrous material that can be used as structural components for the construction of habitats, buildings, furniture, etc. 333 . Fungal mycelium as a construction material has attractive characteristics including self-healing potential, impressive compressive strength, flexibility, insulation, and hydrophobicity 333 . The use of mycelium-based materials and structures in space would be a sustainable, biodegradable option with demonstrated uses for generating textiles 332 and as an alternative to plastic packaging. Haneef et al. used two edible and medicinal fungi, Ganoderma lucidum and Pleurotus ostreatus , to produce mycelium films composed of polysaccharides, lipids, protein, and chitin 334 . The fungi were grown on two different substrates; cellulose or cellulose with PDB, and the final composition and characteristics of the film differed based on which substrate they were exposed to 334 . This suggests that myco-architecture properties could be modulated simply by varying the growth substrate. Biocomposites combining fungal mycelium with cellulose plant fibers 335 or with wood and cellulose nanofibrils have also been investigated 336 . Since they are living organisms, synthetic biology could be used to engineer fungi to secrete other useful structural components such as polymers, for even more complex structures. Indeed, CRISPR-Cas9 methodology has been used to create gene deletions in Paecilomyces variotii , a Chernobyl fungal isolate, and was used to identify the gene responsible for its radiation resistance 337 . This technology could be further employed to enhance various fungi for deep space applications, such as making them better suited for radiation shielding.
Another promising construction material to shield humans, plants and (possibly even) animals from the harsh Lunar and Martian environments is concrete. Concrete is a promising material for space applications as it is strong (it has proven to be the most durable material against natural disasters and extreme weather events), resistant to burns, rust and rot and could be made with engineered microbes and in situ resources. Concrete is composed of three main components: water, cement, and an aggregate (i.e., sand, gravel). Researchers have discovered that the use of human serum albumin combined with regolith from the Moon or Mars as the concrete aggregate can produce a concrete-like biocomposite that is made even stronger with the addition of urea 338 . Alternatives for cement, one of the main components of concrete, can be made using engineered bacteria to express recombinant or structural proteins, such as bovine or human serum albumin 339 and spider silk 340 . This way, protein production and purification can be scaled-up and ultimately mixed with in situ regolith, rather than extracting them directly from the source.
Microbes can further aid in the production of concrete through soil biocementation using microbially induced calcite precipitation (MICP) 341 . This is a process wherein microorganisms precipitate calcium carbonate, the main component of limestone and cement, by urea hydrolysis or CO 2 -concentration 341 . For this reason, candidate microbes are typically highly urease-active bacteria, such as Sporosarcina pasteurii (formerly known as Bacillus pasteurii ) 342 , 343 . One of the limitations of concrete is that it can often crack due to shrinkage. Incorporation of microorganisms into these structures can provide a sustainable solution for in-space construction but also a long-term biotechnological solution for concrete maintenance through crack remediation. Bacteria embedded in the concrete, resulting in what is often termed “living” or “self-healing” concrete, can repair cracks that form over time through the precipitation of calcium carbonate crystals 344 . This has been investigated using microorganisms including microalgae ( Synechococcus and Spirulina ) 345 , 346 , Bacillus 347 , and Deinococcus radiodurans 348 . Concrete is a harsh, alkaline environment (~pH 12) and therefore relies on hardy microbes tolerant of these conditions. The ability for Bacillus to form spores and its resistance to alkaline conditions makes this microbe a promising candidate for survival in the high pH concrete environment. Concrete remediation using MICP by spore-forming Bacillus species was demonstrated by Ramachandran et al. 349 and later by Jonkers et al., who demonstrated that the spores remained viable for up to four months 350 . While this is a promising start, experiments need to be performed to determine whether bacterial spores can remain viable for longer durations. The B. subtilis gene cluster and molecular mechanism involved in calcium carbonate biomineralization have been identified 351 and therefore could be used to engineer novel bacteria with enhanced self-healing capabilities or resistance to the concrete environment.
Using extremophilic bacteria that can tolerate both the concrete and space environment to produce calcium carbonate may allow for the construction of Lunar or Martian structures with increased durability or radiation resistance. One such candidate is the cyanobacterium Synechococcus , a photosynthetic organism that can withstand extreme environmental conditions. Using Synechococcus PCC8806, Zhu et al. incorporated cyanobacteria into a mixture of hydrated concrete powder and sand. Results showed that 38% more calcium was precipitated in conditions containing cyanobacteria than in controls, and the microbial calcite layer on the concrete surface was thicker, more adhesive, and decreased water absorption by twofold 345 . More recently, Synechococcus sp. PCC 7002, was tested for incorporation in a sand-hydrogel scaffold 352 , 353 . Following inoculation into a scaffold of sand, gelatin and media, the microbial viability was analyzed in varying temperature and humidity conditions. While the scaffold was strongest at ambient conditions, cells were not viable after seven days, however at 50% or 100% humidity, 9% and 14% of the cells remained viable after 30 days, respectively 352 . Since desiccation appeared to reduce cell viability, another study analyzed whether changes in component ratios or addition of trehalose would allow for increased viability. They found that using a desiccation protectant like trehalose led to increased cell viability at ambient temperature without sacrificing the mechanical properties of the structure 353 . Maintaining cell viability of cyanobacteria in the concrete structure is vital for enhancing the crack-healing potential, which was shown to be promising in a recent study using S. elongatus and S. platensis at varying concentrations (i.e., 4, 8 and 12%) 346 . An alternative strategy to combat desiccation would be the use of a desiccation-resistant organism such as D. radiodurans , which is a polyextremophilic bacteria known for its resistance to radiation. Unlike some of the other candidate bacteria, D. radiodurans is non-spore forming and therefore has applications for low-temperature conditions 348 . D. radiodurans was shown to be viable for up to 28 days in concrete, providing significant crack healing and increasing the compressive strength of the mortar by 42% at room temperature and 38% at near-freezing temperatures 348 . Strategies enlisting microbes in combination with Lunar or Martian regolith provide a blueprint for ISRU for manufacturing strong, radiation-resistant structures that could further space exploration efforts and the possibility for human habitation on the Moon and Mars.
While microbes offer many benefits and biotechnological solutions for extended spaceflight and the development of sustainable habitats beyond LEO, they can also have a negative impact on space exploration. This can manifest as increased microbial pathogenicity, horizontal gene transfer (HGT) of problematic genes, and biofilm formation which have direct effects on crew health and spacecraft integrity. Understanding how microbes respond to the space environment, will allow for mitigation strategies to be developed and implemented, to ensure successful long-duration space exploration.
Several studies have demonstrated that the conditions and stress of spaceflight can enhance microbial virulence or pathogenicity, as has been observed with many human-associated pathogens either grown or isolated on the ISS and/or in simulated microgravity conditions. Examples include Klebsiella pneumonia 354 , P. aeruginosa 355 , Salmonella enterica serovar Typhimurium 356 , 357 , Serratia marcescens 358 , enterotoxigenic E. coli 359 , and Aspergillus fumigatus 360 . The presence of microorganisms with heightened virulence could increase the risk of crewmembers contracting infections, even more problematic due dysregulated immunity during spaceflight 179 . S. typhimurium grown under modeled microgravity (MMG) 356 and in spaceflight 357 showed increased virulence compared to ground controls as demonstrated by an increased mortality rate in a murine infection model. Similarly, S. marcescens 358 and the pathogenic fungi, Aspergillus fumigatus 360 , grown on the ISS or in simulated microgravity exhibited enhanced virulence compared to terrestrial strains and were more lethal in a Drosophila and zebrafish model, respectively. The specific mechanism responsible for increased microbial virulence in space conditions is still under investigation but genes with altered expression in-flight may contribute to this virulence response. These include biofilm-associated genes which were found to be upregulated in S. typhimurium (e.g., wca/wza genes for colanic acid synthesis, ompA , fimH ) and bacterial motility genes which were downregulated 361 . In addition, transcriptional, and proteomic analysis of P. aeruginosa identified genes that were upregulated in spaceflight including virulence- and adhesin-associated lectin genes ( lecA and lecB ) and rhlA which is involved in biosurfactant production 355 . However, the most common factor contributing to space-induced virulence seems to be transcriptional regulation by Hfq, the expression of which was shown to be decreased under both low shear modeled microgravity (LSMMG) and spaceflight conditions in S. typhimurium 361 , 362 and P. aeruginosa 355 , 363 . Hfq is an RNA chaperone and global transcriptional regulator responsible for controlling the expression of a large array of genes and is necessary for the virulence of several bacterial pathogens 355 . Consistent with previous studies, hfq was found to be downregulated in S. aureus grown in LSMMG, however, unlike previous studies the virulence potential was reduced 364 .
Conversely, some studies have concluded that while microorganisms with pathogenic potential are present in these space environments, spaceflight conditions do not lead to increased virulence or microbial characteristics that would directly impact crew health 365 , 366 , 367 . For example, using a macrophage infection assay, O’Rourke et al. found that there was no significant difference in the virulence of Burkholderia species isolated from the ISS compared to Earth controls 368 . In addition, investigation of four common clinical pathogens, Listeria monocytogenes , methicillin-resistant S. aureus , Enterococcus faecalis , and C. albicans revealed that they were less virulent in space regarding their ability to kill Caenorhabditis elegans nematodes 369 . Similar conclusions were drawn in the ISS experiment EXTREMOPHILES, where sequencing analysis and physiological tests were performed on microbial communities from several surfaces aboard the spacecraft 370 . Researchers proposed that while the ISS environment selects for bacteria with more natural resistance and tolerance to extreme conditions, it does not induce genetic or phenotypic changes that result in more extremophilic, or antibiotic resistant bacteria compared to a built, enclosed environment on Earth 370 . Indeed, a pan-genomic analysis of microbes from the ISS and built environments on Earth found that the antimicrobial resistance (AMR) genes present in ISS samples were also present in control samples, and that functional changes common to built environments do not have a direct impact on astronaut health 371 . Collectively, these studies demonstrate the impact of spaceflight on individual pathogenic microbes in built environments and, for many, it remains to be determined if the virulence phenotype depicted in their models will directly translate to mixed bacterial populations or lead to enhanced pathogenicity in humans. Therefore, assessing the microbiome within the host and continuing to elucidate the mechanism involved in potential spaceflight-enhanced virulence will be necessary. Although there is some debate regarding the increased pathogenicity of microbial populations in space, there is evidence of indirect health concerns caused by harmful biofilm formation 370 .
Microorganisms in the space environment, as on Earth, can exist in a planktonic (freely suspended) state, but more commonly form robust biofilms as a tactic for growth and survival. A biofilm is an assemblage of surface-associated microbial cells surrounded by an extracellular matrix of polysaccharides, extracellular DNA (eDNA), proteins, lipids, and other components, with a defined architecture 372 , 373 . Biofilm-associated organisms differ from their planktonic counterparts with respect to the genes that are transcribed, proteins that are translated and growth rate 372 . Although most bacterial biofilms are harmless, some threaten human health and safety and can be difficult to eradicate due to increased resistance to the immune system’s defenses, UV radiation, extreme temperatures, pH, high salinity, high pressure, limited nutrients, and various antimicrobials 374 , 375 .
Environmental stressors are known to induce biofilm formation 374 and spaceflight is one such stressor. The impact of microgravity on biofilm formation was investigated for the first-time using P. aeruginosa 376 , and later during two NASA-funded studies, Micro-2 and Micro-2A 377 . In these NASA studies, P. aeruginosa grown on the ISS displayed different biofilm characteristics compared to ground controls such as an increased number of viable cells, biomass, and thickness and a novel column-and-canopy shaped architecture 377 . However, this novel architecture was only observed in biofilms formed by motile bacteria, as non-motile strains produced flat structures similar to those seen with the ground controls 377 . In another early biofilm investigation experiment conducted in space, Burkholderia cepacia was grown in sterile water, tryptic soy broth (TSB), and an iodine solution (a disinfectant), for six days on stainless-steel coupons 378 . Results showed that bacteria grown in space, in sterile water, had a biofilm plate count (measured as CFU/m 2 ) five times larger compared to ground controls, however, the space grown TSB population was one quarter of that on Earth 378 . Those grown in the iodine solution in space, also had a higher biofilm growth compared to the ground controls, suggesting increased resistance to disinfectants during spaceflight 378 . In addition, spaceflight conditions have been demonstrated to upregulate gene expression for the production of extracellular matrix proteins leading to enhanced cell aggregation compared to ground controls in C. albicans 361 . Differential expression of genes related to motility, which is important for the formation of biofilms, has also been observed in flight conditions 379 .
Microbially influenced corrosion (MIC), refers to the deterioration of metals and nonmetallic materials due to microbial activity, most often due to biofilms. As biofilms increase in quantity more microbial-surface reactions occur, enhancing structural and/or functional damage, causing accelerated biocorrosion 380 .
In a recent Microbial Tracking study (MT-1) of the ISS, the bacterial bioburden quantified from various surfaces was as high as 10 9 CFU/m 2 381 . Some of the biofilm-forming microorganisms that were identified, Methylobacterium, Sphingomonas, Bacillus, Penicillium , and Aspergillus have been implicated in MIC on Earth 382 , 383 , 384 , 385 with Bacillus polymira , Penicillium rubens and Aspergillus sp. responsible for progressive destruction of a navigation window on board Mir 386 . Sphingomonas sp . and Methylobacterium sp . have not only been detected on surfaces but also in portable drinking water on the ISS 387 . Over the course of 15 years (from its launch in 1986 to 2001), 234 species of bacteria and fungi were identified onboard the MIR space station, with many exhibiting potential polymer biodegradation properties 388 .
Biofilm growth has been observed in the Soviet/Russian (Salyuts and Mir), American (Skylab), and International (ISS) Space Stations. Aboard spacecraft, biofilms can jeopardize vital equipment and threaten astronaut health by corroding surfaces or clogging life-support systems including air and water purification systems, spacesuits, navigation windows and radiators 368 , 389 , 390 , 391 , 392 . Most notable on the ISS, is the microbial contamination and biofilm formation that occurs in the wastewater tank of the Water Recovery System (WRS), which is a part of the Environmental Control and Life Support System (ECLSS) and used to process wastewater from various sources (i.e., urine, cabin condensate) into potable water for crew and other functions 393 . For future planned missions beyond LEO to the Moon and Mars, resupplying spare parts or support materials to repair the listed spaceflight systems would be impractical as missions could be in the order of years, in the case of a Mars missions, thus various strategies to control biofilms, especially in critical life support systems are essential 394 . Ways to detect, monitor and control biofilms are being explored, such as the current spaceflight BAC (Bacterial Adhesion and Corrosion) study. The aim of this study is to identify bacterial genes relevant to biofilm growth in space, examine whether the formed biofilms corrode stainless steel surfaces mimicking those in the ISS water system, and determine whether silver-based disinfectants can prevent or control extensive biofilm formation.
Biofilm formation is an important characteristic in the infectious disease process of microorganisms. It has been demonstrated that bacteria can genetically and physically modify their tolerances to LEO conditions, with one such mechanism being biofilm formation 395 , 396 , 397 . Human opportunistic pathogens that form or increase biofilms under simulated microgravity conditions or when grown on the ISS include E. coli , S. typhimurium , P. aeruginosa and Micrococcus luteus 379 , 398 . It has also been observed that many species of bacteria and fungi become more antibiotic resistant and pathogenic when exposed or grown in spaceflight conditions 174 . In cases of S. typhimurium 17 and P. aeruginosa 355 , the observed increased virulence (discussed earlier in this review) was attributed to molecular and phenotypic changes consistent with biofilm formation. In the case of Klebsiella pneumoniae grown aboard the Shenzhou VIII spacecraft, the enhanced antibiotic resistance was associated with adaptations related to biofilm formation 354 , 399 . As biofilm formation can increase the risk of human illnesses, through harder-to-treat infections, biofilm properties under space conditions need to be well understood to enable safe, long-duration, human space missions. This is even more imperative considering the immune dysregulation of astronauts and lower efficacy of pharmaceuticals during spaceflight 174 .
While biofilms can be detrimental to astronaut health and structural stability, they can be beneficial in areas such as plant protection, bioremediation, wastewater treatment, and corrosion inhibition, amongst others 400 . Thus, strategies for manipulating biofilms should not focus on complete eradication, but rather regulation, to promote the growth of beneficial ones while inhibiting the growth of harmful ones 400 . These beneficial applications of biofilms may also be extended to spaceflight. Ichikawa et al. developed a long-term life support system that uses an electrochemically activated biofilm reactor 401 . This system was tested for the removal of nitrate produced from biological nitrification and is an important process to allow for long-term survival of aquatic organisms in a closed system 401 . Results from this biofilm-electrode reactor study showed that neither ammonia nor nitrite accumulated, and nitrate could be suppressed to about 10 ppm 401 . Biofilms can also provide insight into how humans tolerate spaceflight. Biological dosimetry is an internationally approved method to perform an exposure assessment following a suspected radiation overexposure. In contrast to physical methods, which measure the actual dose, biological dosimeters measure dose effects, at the cellular level, when assessing the impact of radiation exposure on humans 402 . In the BIODOS project, four DNA-based biological dosimeters (phage T7, uracil thin layer, spores, and biofilms) were validated for their effectiveness in determining the biological hazards of environmental UV exposure (i.e., sunlight), and were shown to be reliable field dosimeters 403 . This same biofilm dosimeter was then used in a study by Rettberg et al. to determine the biological effectiveness of the UV radiation climate at different locations in the space station, with the aim of ensuring that astronauts had enough UVB to synthesize vitamin D 404 . Conclusions from this study showed that the amount of UV radiation inside the station was not sufficient for an adequate supply of vitamin D and that specialized UV lamps were needed to maintain healthy levels of Vitamin D for astronaut health 404 . Overall, more work on biofilm applications for spaceflight is needed to tease out the benefits biofilms may offer, while reducing any harmful properties.
The ability for bacteria to survive or even thrive in the spaceflight environment, with potentially increased pathogenicity and biofilm formation, may be attributed to DNA transfer. Horizontal gene transfer (HGT), also known as lateral gene transfer, is the movement of genetic material from one organism to another by means other than sexual reproduction or vertical transfer from a parent cell. This typically occurs through one of three main mechanisms: direct contact of microbial cells by a pilus (i.e., conjugation), natural DNA uptake from the environment (i.e., transformation), or introduction by bacteriophages (i.e., transduction) 405 , 406 , 407 . More recently, gene transfer agents and membrane vesicles are being recognized for their contributions to HGT as well 408 . HGT is central to microbial evolution because it allows microorganisms to acquire novel genetic material, which may confer a fitness advantage to adapt to or thrive within a specific environment 22 , 409 , 410 , 411 .
In the sealed spaceflight environment, bacteria must adapt to extreme conditions including microgravity and cosmic radiation 412 , which could have an impact on the prevalence of genetic transfer. The three main mechanisms of HGT (transduction, transformation, and conjugation) were first investigated for their occurrence in space by Ciferri et al. during the Spacelab D1 mission (STS-61-A, 1986) 413 . They discovered no significant difference in transduction, inconclusive transformation results, and increased transmission of antibiotic resistance genes by conjugation in E. coli exposed to microgravity 413 . It was postulated that this increase in conjugation frequency could be due to a decrease in mating pair disruptions in microgravity compared to Earth gravity, as continuous cell-to-cell contact is required for conjugation to occur. Another spaceflight experiment was performed on the Discovery Mission (STS-63) where researchers concluded that transformation efficiency to E. coli was decreased in microgravity 414 . Later, during the Soyuz Mission 8S on the ISS, the Mobilisatsia/Plasmida experiment examined plasmid-mediated conjugation through triparental mating of both Gram-positive and Gram-negative bacteria 415 . They found that conjugation was increased in experiments between Bacillus thuringiensis strains (Gram-positive), while no trends were observed in conjugation experiments from E. coli to C. metallidurans (Gram-negative) 415 . This increase in conjugation efficiency could be attributed to the mechanistic differences between Gram-positive and Gram-negative conjugation, as Gram-positive bacteria facilitate contact between donor and recipient cells through surface adhesins rather than conjugative pili 416 . However, authors caution the drawing of conclusions due to failure to obtain transconjugants in some replicates of ground controls. Conversely, conjugation experiments performed using the same Gram-positive species ( B. thuringiensis ) in simulated microgravity showed that there was no significant difference in plasmid transfer frequency for a plasmid mobilizing itself ( cis ) or mobilizing a separate plasmid ( trans ) compared to standard laboratory conditions 417 . Most recently, Urbaniak et al. tracked HGT of two antimicrobial resistance (AMR) genes by co-culturing of two species, Acinetobacter pittii and S. aureus , isolated from the ISS as part of the Microbial-1 tracking study 381 . The results indicated an approximately 100-fold increase of HGT in simulated microgravity compared to Earth gravity controls (1- g ) 418 . Combined, these results indicate that HGT occurs in spaceflight conditions within and between Gram-negative and Gram-positive bacteria and is typically not hampered, and is more often increased, by spaceflight conditions.
The human gut houses a diverse microbial population with ecologically favorable conditions for HGT given its continuous supply of nutrients and consistent environmental conditions (e.g., temperature, pH) 14 . Phylogeny-based research suggests that over the course of their evolution, more than half of total genes in the genomes of human-associated microbiota were introduced by HGT 419 . While HGT is a normal occurrence within the human microbiome, an increased number of transfer events passing AMR genes from commensal bacteria to opportunistic pathogens during spaceflight could cause changes in these microbial communities 175 . These transfer events have been investigated in Staphylococcus epidermidis , a bacterium normally present in the human epithelial microbiome, which harbors the methicillin resistance gene mecA on a mobile genetic element. HGT was found to be an important factor for the acquisition of mecA by the pathogen S. aureus , leading to methicillin-resistant S. aureus (MRSA) 420 , 421 . Recent research has also demonstrated the transfer of AMR and virulence-associated genes from commensal E. coli to pathogenic E. coli 422 . The transfer of AMR genes can cause increased bacterial resistance and virulence, which could have significant health implications 423 , 424 for astronauts due to their dysregulated immunity on long-duration space missions 425 . Numerous studies have shown that HGT is the common mechanism by which AMR genes are disseminated within an environment, leading to the emergence of multi-drug resistant bacteria 426 , 427 , 428 , which limits treatment options for bacterial infections.
Some research has proposed that the increased virulence or pathogenicity observed in some organisms grown under spaceflight conditions is attributed to possible increased HGT in spaceflight conditions 357 , 429 , 430 . In a study comparing similar species from two extreme built environments, one on Earth (Concordia Research Station in Antarctica) and one in space (ISS), it was observed that 76% of the isolates from the ISS were resistant to one or more antibiotics tested compared to only 44% of the Concordia isolates 429 . This increased resistance amongst the ISS isolates could be attributed to the higher number of mobile genetic elements (involved in HGT) within their genomes compared to the Antarctic strains 429 . The reason for this increase in mobile genetic elements is unclear but it could be a response to the unique stressors of the space environment. Further, in a study published by Urbaniak et al. examining the ISS ‘resistome’, whole genome sequencing revealed AMR gene clusters in Enterobacter bugandensis isolated from the waste and hygiene compartment on the ISS. Further examination showed that these isolates shared AMR gene clusters with known pathogens from different genera which were not present in any Enterobacter species isolated on Earth 430 . The researchers proposed that these AMR genes may have been acquired through HGT, but further analysis is necessary to conclude this with certainty. Changes in HGT-associated gene expression were also identified in ISS-derived isolates of S. typhimurium during Space Shuttle mission STS-115, which exhibited enhanced virulence and increased biofilm formation in a mouse model compared to the ground control 357 . The expression of hfq , an RNA chaperone and negative regulator of the F plasmid-encoded tra genes, was decreased in spaceflight. TraJ is an activator of the tra operon, and hfq has been shown to specifically repress traJ expression by destabilizing its mRNA 431 . As a result, several tra genes were upregulated in response to spaceflight 357 . Mating assays performed in an hfq mutant showed an increase in protein levels of TraJ confirmed by immunoblotting as well as increased conjugation efficiency compared to wild-type controls 431 . Due to the multiple AMR genes found on the environmental surfaces of the ISS 430 and possible enhanced HGT activity during spaceflight, further studies into HGT and the effect on crew health are is important to understand for the development of mitigation strategies 432 , 433 , 434 . In addition, further elucidation of differentially expressed genes and their effect on HGT could identify novel gene targets for modulating or reducing HGT in the space environment.
As previously discussed, biofilms can be detrimental to spacecraft and astronaut health; thus, understanding the factors that can influence biofilm formation will be imperative for predicting, preventing, and mitigating spacecraft contamination. HGT may contribute to biofilms as their formation can be induced by conjugative plasmids that express factors to enhance cell-to-cell contact and pilus formation. Conjugative pili can act as adhesion factors as demonstrated by Ghigo who monitored biofilm formation on Pyrex slides submerged in cultures of E. coli K12. They observed that strains carrying a conjugative F plasmid (F+) formed thick biofilms after one day (2 × 10 10 CFU/cm 2 ), while plasmid-free strains (F−) only formed microcolonies (8 × 10 5 CFU/cm 2 ) 435 . Conjugative pili specifically were shown to be a contributing factor to biofilm formation as strains carrying plasmids with mutations in the pilin gene, traA , were unable to form biofilms 435 . Reisner et al. confirmed Ghigo’s findings as the presence of the F plasmid pOX38 in E. coli led to the formation of mushroom-shaped biofilms with increased biomass, surface coverage and thickness compared to F- controls 436 . To further analyze the contribution of the pilus to this phenotype, the authors created plasmid mutants for several of the genes required for pilus synthesis: traQ , traX , traD , traS , and traT 436 . Mutants involved in pilus assembly and modification (i.e., traQ, traX ) displayed a weak biofilm phenotype similar to the plasmid-free strain ( traQ ) or decreased biomass and thickness ( traX ), while those involved in DNA transfer (i.e., traD ) displayed rapid confluent growth and tower-like structures 436 . In a different study performed with 403 natural E. coli isolates researchers observed biofilm formation in 56 isolates and of those, 89% contained conjugative plasmids 437 . These recipients of conjugative plasmids were able to induce biofilms to a greater extent than their plasmid-free controls 437 . Finally, one study validated that conjugative plasmids enhanced biofilm formation but concluded that this did not directly correlate with conjugation frequency for all plasmids tested, suggesting other factors may be involved 438 .
Other studies suggest that conjugative plasmid-encoded fimbriae, biofilm-associated pili, and cell wall-anchoring proteins can also increase biofilm formation. Type III fimbriae encoded as accessory proteins on conjugative plasmids have been demonstrated to mediate cell–cell and cell-surface adhesion 439 , as well as increased biofilm formation 440 in K. pneumoniae 441 . Further evidence of this was demonstrated in a uropathogenic strain of E. coli where Tn5 mutagenesis was used to identify biofilm-deficient mutants 442 . All Tn5 insertions were found to be within the type III fimbriae genes ( mrkABCDF ) encoded on the conjugative plasmid pMAS2027. This suggests that type III fimbriae were necessary for biofilm formation which was confirmed when this locus was cloned into biofilm-deficient mutants and was able to restore biofilm formation 442 .
When analyzed in a space environment it appears that pili and fimbriae contribute to increased biofilm formation in the short term but decreased biofilm formation in the long term. In a spaceflight study, researchers compared biofilm formation of Acinetobacter schindleri over a short duration (15 days) and long-duration (64 days) from the Shenzhou-10 spacecraft and Tiangong-2 space lab, respectively 443 . They observed reduced biofilm formation after 64 days and following transcriptional analysis proposed that this reduction was potentially due to downregulation of the pil and algR genes associated with conjugative pili and alginate biosynthesis, or upregulation of genes involved in metal iron binding (as available iron increases biofilm formation) 443 . In another study analyzing Proteus mirabilis biofilm formation following short-term or long-term SMG, researchers found that long-term exposure resulted in downregulation of genes associated with fimbriae, impeding adhesion, and ultimately decreasing biofilm formation 444 .
The rate of HGT amongst bacterial communities in biofilms is increased as it contains a diversity of bacteria, the structured extracellular matrix (ECM) provides the ideal environment to stabilize mating pair formation and bacterial contact for genetic exchange, and eDNA accumulates within the ECM allowing for natural transformation 435 , 445 , 446 , 447 . Lécuyer et al. analyzed the conjugative transfer of an integrative and conjugative element (ICE) between B. subtilis strains on normal media compared to biofilm-inducing media. Results indicated that conjugative transfer was increased by 100-fold and 10,000-fold on biofilm-inducing media using minimal media and rich media, respectively 446 . Conjugation experiments performed between S. aureus strains using donors harboring a mobilizable plasmid and the multi-drug resistant conjugative plasmid, pGO1 yielded similar results 448 . Conjugation was performed with standard filter mating or a cellulose disk static biofilm model and conjugation frequency in the biofilm-promoting conditions was found to be ~16,000-fold higher than in standard conditions 448 . Overall, HGT promotes biofilm formation which, in turn, promotes HGT transfer, and both can contribute to increased bacterial pathogenicity (Fig. 4 ). If HGT is increased under space conditions which can consequently lead to the production of more biofilms, the effect that biofilms have on spacecraft integrity and function could be even more severe during long-duration space travel if this feedback loop goes uninterrupted.
In microgravity, bacterial HGT can increase cell–cell adhesion, and production of eDNA and extracellular polysaccharides contributing to increased biofilm formation. Reciprocally, biofilms promote HGT as they contain high microbial diversity and an ECM structure allowing for increased cell aggregation, stable mating pair formation and eDNA accumulation. Both HGT and biofilms increase bacterial virulence through cellular adhesion and dissemination of antimicrobial resistance, and increased biomass and resistance to disinfectants, respectively. Created with BioRender.com.
Although HGT has the potential to negatively impact astronaut health and jeopardize spacecraft during long-duration space missions, conjugation machinery can also be harnessed as a tool for the development of novel mitigation strategies. Conjugation has been demonstrated within and between many species of Gram-negative and Gram-positive bacteria in a laboratory setting, and from bacteria to eukaryotic cells. Conjugative tool development for many of these species could have implications for their use in the space environment including those developed to target opportunistic pathogens (e.g., Enterococcus , Listeria, Staphylococcus 449 , Streptomyces 450 , and S. enterica 451 ), or those that could be used to engineer useful strains such as probiotic candidates (e.g., Bacillus 449 , Bifidobacterium 452 and Lactobacillus 453 ) or extremophilic microbes (e.g., D. radiodurans 454 , yeast 455 or algae 267 , 268 ). When coupled with CRISPR/Cas technologies conjugation can be used for the modulation of microbiomes and as a method for targeted eradication of human pathogens on Earth. This has been demonstrated using a cis - and trans - conjugative plasmid encoding the I-TevI nuclease domain fused to Streptococcus pyogenes or S. aureus Cas9 (TevSpCas9 or TevSaCas9) targeting S. enterica 451 . This study demonstrated S. enterica killing efficiencies ranging from 1 to 100% following conjugation using 65 single or multiplexed sgRNAs, allowing for the ability to modulate bacterial populations based on the chosen sgRNA. Another study using a similar strategy and a trans -conjugative system has demonstrated specific bacterial killing and targeting of a plasmid-born carbapenem resistance gene in E. coli 456 . Other Cas nucleases can be used to target pathogens as well, including CRISPR/Cas13a-based antibacterial nucleocapsids, which have been shown to kill resistant E. coli and S. aureus species by targeting AMR genes 457 . CRISPR/Cas technologies can also be used to inhibit conjugation in human pathogens 458 , 459 , including species that have been isolated from the ISS such as K. pneumonia 460 , E. faecalis 461 , and Staphylococcus 462 . The biotechnological applications of CRISPR/Cas systems in space are extensive, from using Cas proteins to understand the biological impact of microgravity to detecting the presence of pathogenic bacteria or viruses, as demonstrated on Earth using Cas12 or Cas13 for SARS-CoV-2 RNA detection 463 , 464 , 465 . The use of CRISPR/Cas systems for these in-space applications is feasible as genome editing using a CRISPR-based assay has been performed in S. cerevisiae onboard the ISS 466 . The mitigation strategies discussed here will require further testing and adaptation for space which could be carried out in synthetic human gut microbiomes 467 or in simulated spaceflight biofilms 394 . However, these results indicate that harnessing the power of conjugation and CRISPR/Cas technologies could provide a promising strategy for detection of pathogenic bacteria, mitigation of HGT and modulation of human and environmental microbiomes in spacecraft.
To minimize the health risks associated with extended spaceflight, it is critical that methods for preventing and treating spaceflight-induced illnesses be developed before astronauts embark upon long-duration space missions. Specifically, increased HGT, pathogenicity and biofilm formation by microorganisms in the space environment presents the need for highly effective antimicrobials and targeted solutions for use on spacecraft. Aside from traditional antibiotics 468 , the use of live engineered organisms, and the use of the conjugation and CRISPR-based strategies discussed above, other mitigation strategies have been investigated to inhibit HGT and the development of biofilms 394 . One well-studied method is antibacterial photodynamic inactivation employing the use of a photoactive compound which accumulates in target bacteria where it is illuminated to produce a cytotoxic reaction with oxygen resulting in cellular damage and bacterial death (reviewed in ref. 469 ). Additional examples of mitigation strategies include the use of specialized material coatings or surfaces (e.g., copper-based antimicrobial surfaces 470 , 471 , silver and ruthenium bio-deterrent surfaces 472 ), engineered lantibiotics 473 , chemical water treatment, UV light, sound waves, and phenols 474 . Other promising antimicrobial materials include AGXX 472 , which was shown to prevent the growth of Staphylococcus and Enterococcus pathogens on the ISS, and sterilization using cold atmospheric plasma 441 . Some potential antibiofilm coating issues that need to be explored include the longevity and chemical stability of the coatings 475 . While several coatings give extremely promising results in the short term, their chemical and physical stability may diminish over time 476 . Regarding long-term space exploration, replenishing these antimicrobial coatings will prove challenging. The use of plant-based extracts is thus gaining in popularity for their antimicrobial and antibiofilm properties along with the added benefit of being able to harvest the necessary compounds during spaceflight, as needed 390 .
Within the next decade, great strides will be made in space exploration with the combined efforts of NASA and other space agencies to reach the Moon and Mars, as well as the expansion of commercialized spaceflight. The Artemis missions will work towards establishing a lunar base camp by 2025 with the purpose of utilizing the Moon as a precursor to Mars exploration. These missions will involve long-duration spaceflight and prolonged extraterrestrial occupation, requiring further exploration of health risks and resource sustainability than what was needed for the decades spent in LEO on the ISS. This review has discussed the role of microbes and their beneficial or detrimental impacts on long-duration space missions as demonstrated in Earth-based simulated space environments or experiments conducted in spaceflight. Microbes heavily contribute to the success of our ecosystem on Earth and can therefore be repurposed for the space environment to help generate a sustainable habitat. We have summarized the advantageous properties of microbes in plant cultivation, wastewater treatment, solid and liquid waste reuse, and atmospheric revitalization. This review has also considered the use of microbial fuel cells to generate energy from waste, plant decay, and solar light conversion. Although more research is needed for efficient energy conversion in the space environment, we present microbial fuel cells as an ideal and possible future alternative for energy generation. We also examined the advantages of bioengineered microbes for in-flight therapeutics, increased production of nutrients and oxygen, and the creation or recycling of infrastructure materials. Most of these microbial technologies have been successfully demonstrated on Earth, but as suggested, should be further tested, and applied in the space environment. Microbes are ideal candidates to aid in human survival during long-term space travel due to their many beneficial characteristics, ease of manipulation, and microscopic size, allowing them to be easily stowed without the concern of added weight. In terms of health and safety risks, the possibility of increased microbial virulence and pathogenicity in spaceflight was discussed, as well as the detrimental effects of increased HGT and biofilm formation on astronaut health and equipment integrity. Suggestions were also made regarding mitigation strategies for further investigation, including antimicrobial metallic surface materials and coatings that prevent increased HGT or biofilm formation. This review has presented the vast contributions that microbes can make towards future crewed missions, human habitability and sustainability and hopefully encourages more space-related microbial research interconnected with technological development, to continue to safely advance deep space exploration in the upcoming decade.
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The authors acknowledge funds from a NASA 2020 Space Biology (NNH18ZTT001N-FG2) grant (80NSSC21K0320) awarded to C.U.
These authors contributed equally: Allison P. Koehle, Stephanie L. Brumwell.
Department of Plant Science, Pennsylvania State University, University Park, PA, USA
Allison P. Koehle
Department of Biochemistry, Schulich School of Medicine and Dentistry, The University of Western Ontario, London, ON, Canada
Stephanie L. Brumwell
Honeybee Robotics, Altadena, CA, USA
Emily P. Seto
Department of Pulmonary Medicine, The University of Texas MD Anderson Cancer Center, Houston, TX, USA
Anne M. Lynch
Graduate Program in Developmental Biology, Baylor College of Medicine, Houston, TX, USA
ZIN Technologies Inc, Middleburg Heights, OH, USA
Camilla Urbaniak
NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
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A.K., S.B., E.S., A.L., and C.U. wrote the manuscript; A.K., S.B., and C.U. edited the manuscript; C.U. prepared the concept and outline of the manuscript and provided feedback to all authors. All authors reviewed the final draft and approved it for submission.
Correspondence to Camilla Urbaniak .
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Koehle, A.P., Brumwell, S.L., Seto, E.P. et al. Microbial applications for sustainable space exploration beyond low Earth orbit. npj Microgravity 9 , 47 (2023). https://doi.org/10.1038/s41526-023-00285-0
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