Astronauts Could Replace Their Own Mitochrondria To Treat Radiation Sickness

Skeptics love to bring up one particular topic regarding long-term human space exploration - radiation. So far, all of the research completed on it has been relatively limited and has shown nothing but harmful effects. Long-term exposure has been linked to an increase in cancer, cataracts, or even, in some extreme cases, acute radiation poisoning, an immediate life-threatening condition. NASA is aware of the problem and recently supported a new post-doc from MIT named Robert Hinshaw via the Institute for Advanced Concepts (NIAC) program. Dr. HHinshaw'sjob over the next year will be to study the effectiveness of an extreme type of mitochondria replacement therapy to treat the long- and short-term risks of radiation exposure in space.

Dark Matter Doesn't Decay, Whatever It Is

Dark Matter Doesn't Decay, Whatever It Is

And Then There Were Three: NASA Shuts Down More Voyager 2 Science Instruments

In an effort to conserve Voyager 2's dwindling energy and extend the spacecraft's mission, NASA has shut down another of its instruments. They did it with the Plasma Spectrometer in October 2024, and it won't be the last. In March, Voyager 2's Low-Energy Charged Particle instrument will be powered down.

What does this mean for the durable spacecraft?

"If we don’t turn off an instrument on each Voyager now, they would probably have only a few more months of power before we would need to declare end of mission." - Suzanne Dodd, Voyager Project Manager, JPL

Things have changed a lot since the pair of Voyager spacecraft were launched in 1977. Our planet is hotter, the human population has ballooned, and Battlestar Galactica came and went—twice.

Voyager 1 and 2 have surprised us all with their longevity. When they were launched, their planned mission length was a mere five years. Now, almost 50 years after their launch date, they've both reached interstellar space, a remarkable achievement.

This image shows Voyager 2 blasting off on a Titan-Centaur rocket from Cape Canaveral on August 20th, 1977. Image Credit: NASA

Though both spacecraft have proven to be durable, nothing lasts forever, not even plutonium. When they were launched, they both carried about 13.5 kg of plutonium-238 in their Radioisotope Thermoelectric Generators (RTGs). RTGs generate electricity by running the heat from the decaying plutonium through a thermocouple. However, as the plutonium decays, its power output is reduced. That necessitates lowering the spacecraft's power demands.

That's where NASA is at with both Voyagers. They've had to sequentially shut down systems that are no longer providing much scientific benefit. Fortunately, some of the spacecraft's instruments were aimed at planetary science and are less critical in interstellar space.

"The Voyagers have been deep space rock stars since launch, and we want to keep it that way as long as possible," said Suzanne Dodd, Voyager project manager at JPL. "But electrical power is running low. If we don’t turn off an instrument on each Voyager now, they would probably have only a few more months of power before we would need to declare end of mission."

Each Voyager spacecraft carries the same payload of 10 science instruments. NASA has shut down different instruments on each one at different times to achieve the best science outcomes.

In October 2024, NASA turned off Voyager 2's Plasma Spectrometer. On March 24th, NASA will shut down Voyager 2's Low-Energy Charged Particle Instrument (LECP), leaving it with only three active instruments: the Triaxial Fluxgate Magnetometer (MAG), the Cosmic Ray Subsystem (CRS), and the Plasma Wave Subsystem (PWS).

Those three instruments still allow Voyager 2 to gather valuable scientific data.

Voyager 2 captured this image of Jupiter and Io when it was 24 million km away. Image Credit: NASA/JPL

Voyager 2's MAG instrument measured the magnetic fields of Uranus and Neptune and how the solar wind interacted with their magnetospheres. It also played a vital role in determining exactly when Voyager 2 crossed the heliopause into interstellar space. Now that the spacecraft is in interstellar space, MAG is measuring the strength of interstellar magnetic fields and how they interact with the Sun's magnetic fields.

The CRS instrument helped scientists measure energetic particles inside the magnetospheres of the outer planets. It also provided irreplaceable data on the composition, energy, and distribution of cosmic rays. By measuring cosmic ray nuclei, it helped scientists understand how these rays are accelerated and propagated. By measuring cosmic ray flux in interstellar space, the CRS revealed some of the details about the ISM.

The PWS measured the density of electrons near the Solar System's planets. Early in the Voyager missions, the instrument detected lightning storms on Jupiter and other giant planets, a significant development in understanding these planets. In interstellar space, it's measuring the density of the interstellar plasma. Its measurements are critical to understanding the interstellar medium (ISM).

Throughout its mission, the LECP instrument has told scientists about the energy of charged particles and the dynamics of the Sun's solar wind. It has also shown how some particles can leak out of the heliosphere into interstellar space. As Voyager 2 continues its journey into interstellar space, the LECP will tell us more about the heliopause and how particles behave differently in the heliosphere and interstellar space.

"Every minute of every day, the Voyagers explore a region where no spacecraft has gone before." - Linda Spilker, Voyager project scientist at JPL

The LECP instrument will be shut down later this month, reducing Voyager 2 to only three instruments. Nothing illustrates Voyager's longevity and robustness more than the LECP. It's only being shut down because of energy constraints, not because of degraded performance.

Voyager 2 uses a stepped motor to rotate the instrument 360 degrees and provides a 15.7-watt pulse every 192 seconds. During development and testing, the motor was tested to 500,000 steps. That was enough to see it through until the spacecraft encountered Saturn in August 1980. However, the motor will have completed more than 8.5 million steps by the time it's deactivated later this month.

Like other facets of the Voyager program, the LECP has lasted so long that its principal investigator, Stamatios Krimigis, is now 86 years old and has retired into an honorary position. He's now Emeritus Head of the Space Exploration Sector of the Johns Hopkins Applied Physics Laboratory (APL). Maybe both the man and the instrument will fully retire at the same time.

Voyager 1 and 2 are our first interstellar probes, though they were never intended to be. Everything they're showing us about interstellar space is bonus knowledge. Many of the people behind the program are gone now, but both spacecraft live on. There's a poignancy to that that goes beyond science, charged particles, and the details of the interstellar medium. They're humanity's first unintentional envoys into interstellar space and are starting to outlast their creators.

"The Voyager spacecraft have far surpassed their original mission to study the outer planets." - Patrick Koehn, Voyager Program Scientist

This graphic from 2019 shows the locations of both Voyage probes in relationship with the heliosphere. Image Credit: NASA/JPL-Caltech/Johns Hopkins APL

However, the Voyagers are scientific missions, and they're still stubbornly fulfilling those missions.

"The Voyager spacecraft have far surpassed their original mission to study the outer planets," said Patrick Koehn, Voyager program scientist at NASA Headquarters in Washington. "Every bit of additional data we have gathered since then is not only valuable bonus science for heliophysics but also a testament to the exemplary engineering that has gone into the Voyagers — starting nearly 50 years ago and continuing to this day."

NASA is determined to milk the Voyager spacecraft for as much data as possible. Once Voyager 2's LECP is turned off later this month, both Voyagers should be able to operate for another year before another instrument will need to go dark. For Voyager 1, this means it will lose its LECP. Voyager 2's CRS will be shut off in 2026.

NASA engineers say that their power conservation program should let both spacecraft operate into the 2030s, albeit with a single instrument each. However, they have been operating in deep space for almost 50 years, and it's not a benign environment. It's only rational to expect some other problems to crop up.

It's easy to gloss over the success of the Voyager program now that space missions launch every month, powerful rovers explore Mars, and high-resolution cameras deliver a steady stream of yummy images to our hungry browsers. It's also easy to forget that they've both travelled more than 20 billion km. In fact, when Voyager 2 sends us a signal, it takes 19.5 hours to reach us. For Voyager 1, the signal travel time is even greater: 23.5 hours. Those signal travel times will only grow as the spacecraft continue their journeys. And every kilometre of their journeys is a new frontier for humanity.

"Every minute of every day, the Voyagers explore a region where no spacecraft has gone before," said Linda Spilker, Voyager project scientist at JPL. "That also means every day could be our last. But that day could also bring another interstellar revelation. So, we’re pulling out all the stops, doing what we can to make sure Voyagers 1 and 2 continue their trailblazing for the maximum time possible."

• Press Release: NASA Turns Off 2 Voyager Science Instruments to Extend Mission

• Press Release: 40 Years Ago: Voyager 2 Explores Jupiter

• Published Research: Whistlers observed by Voyager 1: Detection of lightning on Jupiter

Lucy Sees its Next Target: Asteroid Donaldjohanson

NASA's asteroid-studying spacecraft Lucy captured an image of its next flyby target, the asteroid Donaldjohanson. On April 20th, the spacecraft will pass within 960 km of the small, main belt asteroid. It will keep imaging it for the next two months as part of its optical navigation program.

Donaldjohanson is an unwieldy name for an asteroid, but it's fitting. Donald Johanson is an American paleoanthropologist who discovered an important australopithecine skeleton in Ethiopia's Afar Triangle in 1974. The female hominin skeleton showed that bipedal walking developed before larger brain sizes, an important discovery in human evolution. She was named Lucy.

NASA named their asteroid-studying mission Lucy because it also seeks to uncover clues about our origins. Instead of ancient skeletal remains, Lucy will study asteroids, which are like fossils of planet formation.

During its 12-year mission, Lucy will visit eight asteroids. Two are in the main belt, and six are Jupiter trojans. Asteroid Donaldjohanson is a main-belt, carbonaceous C-type asteroid—the most common variety—about 4 km in diameter and is Lucy's first target. It's not one of the mission's primary scientific targets. Instead, the flyby will give Lucy mission personnel an opportunity to test and calibrate the spacecraft's navigation system and instruments.

This image depicts the two areas where most of the asteroids in the Solar System are found: the asteroid belt between Mars and Jupiter and the Trojans, two groups of asteroids moving ahead of and following Jupiter in its orbit around the Sun. Image Credit: NASA

The animation below blinks between images captured by Lucy on Feb. 20th and 22nd. It shows the perceived motion of Donaldjohanson relative to the background stars as the spacecraft rapidly approaches the asteroid.

via GIPHY

The flyby is like a practice run before Lucy visits the Jupiter trojans. These asteroids are clusters of rock and ice that never coalesced into planets when the Solar System formed. These are the "fossils of planet formation," the most well-preserved evidence from the days of Solar System formation.

Currently, Donaldjohanson is 70 million km away and will remain a tiny point of light for weeks. Only on the day of the encounter will the spacecraft's cameras capture any detail on the asteroid's surface. In the images above, the dim asteroid still stands out from the dimmer stars of the constellation Sextans. Lucy's high-resolution L'LORRI instrument, the Long Lucy LOng Range Reconnaissance Imager, captured the images.

Lucy is following a unique flight pattern. It's essentially a long figure-eight.

Illustration of the Lucy spacecraft's orbit around Jupiter, which will allow it to study its Trojan population. Though the image lists 6 flybys, the spacecraft will visit 8 asteroids. One of the listed ones is a binary, and the spacecraft already encountered the asteroid Dinkinesh. Image Credit: SwRI

Even this early in its mission, Lucy has delivered some surprising results. In November 2023, it flew past asteroid 152830 Dinkinesh. The flyby was intended as a test for the spacecraft's braking system, but instead, it revealed that Dinkinesh has a small satellite. Closer observations showed that the satellite is actually a contact binary, which means it's composed of two connected bodies. This was a valuable insight into asteroids.

These two images from Lucy show the asteroid Dinkinesh and its satellite Selam. The first image (L) shows Selam just coming into view behind Dinkinesh. The second image (R) reveals that Selam is actually two objects, a contact binary. Image Credits: By NASA/Goddard/SwRI/Johns Hopkins APL/NOIRLab - Public Domain, https://ift.tt/fzc18R4

There are surprising discoveries in every mission, and Lucy is no exception. As it makes its way through its list of targets, it will almost certainly show us some surprises.

The Trojans are difficult to study from a distance. They're a long way away. Scientists aren't certain how many there are; there may be as many Trojans as there are main-belt asteroids. The Trojans exhibit a wide variety of compositions and characteristics, which could indicate that they came from different parts of the Solar System. By studying the Trojans in all their diversity, Lucy will hopefully help scientists reconstruct their origins and how they were captured by Jupiter.

The Solar System has a long history and we've only just become a part of it. Some of the clues to our origins are out there among the battered rocks of the asteroid belt and the Jupiter Trojans. Lucy will give us our best look at the Trojans. Who knows what it might reveal?

Press Release: NASA's Lucy Spacecraft Takes Its 1st Images of Asteroid Donaldjohanson

Press Release: NASA Lucy Images Reveal Asteroid Dinkinesh to be Surprisingly Complex

ASU Institute of Human Origins: Lucy's Story

For the Sake of Astronaut Health, Should we Make the ISS Dirtier?

There are several well-documented health risks that come from spending extended periods in microgravity, including muscle atrophy, bone density loss, and changes to organ function and health. In addition, astronauts have reported symptoms of immune dysfunction, including skin rashes and other inflammatory conditions. According to a new study, these issues could be due to the extremely sterile environment inside spacecraft and the International Space Station (ISS). Their results suggest that more microbes could help improve human health in space.

The study was led by Rodolfo A. Salido and Haoqi Nina Zhao, a bioengineer and an environmental analytical chemist at the University of California San Diego (UCSD), respectively. They were joined by researchers from multiple UCSD programs and centers, the University of Denver, the Chiba University-UC San Diego Center for Mucosal Immunology Allergy and Vaccines (cMAV), Space Research Within Reach, the Baylor College Center for Space Medicine, the Blue Marble Space Institute of Science (BMSIS), the Biotechnology and Planetary Protection Group at NASA JPL, and the Astronaut Office at NASA Johnson.

The study was a collaborative effort with astronauts aboard the ISS, who swabbed 803 different surfaces – 100 times that of previous surveys – to get a census of microbes aboard the station. The researchers identified which bacterial species and chemicals were present in each sample and created three-dimensional maps to illustrate where each of them was found and how they might be interacting. Their results indicate that the ISS has a much lower diversity of microbes compared to human-built environments on Earth.

NASA astronaut Catherine (Cady) Coleman, Expedition 26 flight engineer, is pictured with a stowage container and its contents in the Harmony node of the International Space Station. Credit: NASA

Overall, the team found that chemicals from cleaning products and disinfectants were ubiquitously throughout the station and that astronauts mostly introduce microbes aboard the ISS through shed human skin cells. They also found that different modules hosted different microbial communities and chemical signatures based on the module’s use. For example, dining and food preparation areas contained more food-related microbes, whereas the ISS’s space toilet contained more urine- and fecal matter-related microbes and bioproducts of metabolism (metabolites).

“We noticed that the abundance of disinfectant on the surface of the International Space Station is highly correlated with the microbiome diversity at different locations on the space station,” said Zhao in a Cell Press release. These results suggest that more microbes from Earth could help improve astronaut health. Said Salido:

“Future built environments, including space stations, could benefit from intentionally fostering diverse microbial communities that better mimic the natural microbial exposures experienced on Earth, rather than relying on highly sanitized spaces. If we really want life to thrive outside Earth, we can’t just take a small branch of the tree of life and launch it into space and hope that it will work out. We need to start thinking about what other beneficial companions we should be sending with these astronauts to help them develop ecosystems that will be sustainable and beneficial for all.” 

The team found that microbial communities were less diverse aboard the ISS than most places on Earth, except where urban, industrialized, and isolated environments (i.e., hospitals) were concerned. They further found that ISS surfaces lacked free-living environmental microbes usually found in soil and water. Similar to the well-documented benefits gardening has for the human immune system, the researchers conclude that incorporating these microbes and their substrates into the ISS could improve astronaut health without sacrificing hygiene.

Astronauts on the International Space Station experience an orbital reboost. Credit: NASA/ESA

“There’s a big difference between exposure to healthy soil from gardening versus stewing in our own filth, which is kind of what happens if we’re in a strictly enclosed environment with no ongoing input of those healthy sources of microbes from the outside,” said co-author Robin Knight, a computational microbiologist and professor at UCSD and leader of the Knight Lab.

Looking to the future, the researchers hope to refine their analyses to detect potentially pathogenic microbes and how environmental metabolites could be used as indicators for astronaut health. The team claims that these methods could also help improve the health of people living and working in similarly sterile environments on Earth.

This research was supported by the National Institute of Health (NIH), the Alfred P. Sloan Foundation, UCSD, the Center for the Advancement of Science in Space (CASIS), and the ISS National Laboratory. The paper detailing their findings, “The International Space Station has a unique and extreme microbial and chemical environment driven by use patterns,” was published on February 27th in the journal Cell.

Further Reading: EurekAlert!

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Good News! The Subaru Telescope Confirms that Asteroid 2024 YR4 Will Not Hit Earth.

On December 27th, 2024, the Chilean station of the Asteroid Terrestrial-impact Last Alert System (ATLAS) detected 2024 YR₄. This Near-Earth Asteroid (NEA) belongs to the Apollo group, which orbits the Sun with a period of approximately four years. For most of its orbit, 2024 YR4 orbits far from Earth, but sometimes, it crosses Earth’s orbit. The asteroid was spotted shortly after it made a close approach to Earth on Christmas Day 2024 and is now moving away. Additional observations determined it had a 1% probability of hitting Earth when it makes its next close pass in December 2032.

This led the International Asteroid Warning Network (IAWN) – overseen by the United Nations Office for Outer Space Affairs (UNOOSA) – to issue the first-ever official impact risk notification for 2024 YR₄. The possibility of an impact also prompted several major telescopes to gather additional data on the asteroid. This included the Subaru Telescope at the Mauna Kea Observatory in Hawaii, which captured images of the asteroid on February 20th, 2025. Thanks to the updated positional data from these observations, astronomers have refined the asteroid’s orbit and determined that it will not hit Earth.

This is not the first time the odds of the asteroid hitting Earth have been reevaluated. Throughout February, refined measurements of the asteroid altered the estimated likelihood multiple times, first to 2.3% and then to 3.1%, before dropping significantly to 0.28%. Thanks to the observations of the Subaru Telescope, which were conducted at the request of the JAXA Planetary Defense Team and in response to the IAWN’s call for improved orbital tracking, the chance of impact has been downgraded to 0.004%.

Monte Carlo modeling of 2024 YR4’s swath of possible locations as of February 23rd, 2025 – 0.004% probability of impact. Credit: iawn.net

The updated estimate was calculated by NASA’s Center for NEO Studies (CNEOS), the ESA’s Near-Earth Objects Coordination Centre (NEOCC), and the NEO Dynamic Site (NEODyS). The Subaru observations were conducted using the telescope’s Hyper Suprime-Cam (HSC), a wide-field prime-focus camera that captured images of 2024 YR₄ as it grew dimmer. The observations have since been forwarded to the Minor Planet Center (MPC) of the International Astronomical Union (IAU). Dr. Tsuyoshi Terai of the National Astronomical Observatory of Japan (NAOJ), who led the observations, explained:

“Although 2024 YR₄ appeared relatively bright at the time of its discovery, it has been steadily fading as it moves away from the Earth. By late February, observations would have been extremely challenging without a large telescope. This mission was successfully accomplished thanks to the Subaru Telescope’s powerful light-gathering capability and HSC’s high imaging performance.”

Based on these latest observations, the IAWN reports that 2020 YR₄ will “pass at a distance beyond the geosynchronous satellites and possibly beyond the Moon.” They also indicate that there is no significant potential that the asteroid will impact Earth in the next century. The IAWN also states that it will continue to track 2024 YR4 through early April. At this point, it will be too faint to image and won’t be observable from Earth again until 2028.

Further Reading: NAOJ

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How Brine Shrimp Adapted to Mars-like Conditions

The effects of Climate Change on Earth’s living systems have led to a shift in biological studies, with attention now being focused on the boundaries within which life can survive. Studying life forms that can thrive in extreme environments (extremophiles) is also fundamental to predicting if humans can live and work in space for extended periods. Last, but not least, these studies help inform astrobiological studies, allowing scientists to predict where (and in what form) life could exist in the Universe.

In a recent study, a team of Italian researchers used brine shrimp (Artemia franciscana) in the earliest stage of development (nauplii) and subjected them to Mars-like pressure conditions. Their results indicate that while the nauplii experienced physiological changes, their development remained largely unchanged. This not only demonstrates that extremophiles show great adaptability and can survive in Mars-like conditions. It also indicates that similar life forms could be found elsewhere in the Universe, representing new opportunities for astrobiological research.

Maria Teresa Muscari Tomajoli, an Astrobiology PhD Candidate at the Parthenope University of Naples, led the study. She was joined by Paola Di Donato, a Professor of Organic and Biological Chemistry at Parthenope. They were joined by researchers from the Federico II University, the INAF-Institute of Space Astrophysics and Planetology (INAF-ISAP), the INAF-Osservatorio Astronomico di Capodimonte, and the Italian Institute for Nuclear Physics (INFN). The paper that details their findings was part of a special volume titled Comparative Biochemistry and Physiology A: Molecular & Integrative Physiology.

Brine Shrimp Artemia franciscana. Credit: Wikipedia

On Earth, extremophiles belong to all three domains of life (Archaea, Bacteria, and Eukarya). They are characterized by their ability to withstand pressure, acidity, temperatures, and other conditions that would be fatal to other organisms. After Earth, Mars is considered the most habitable planet after Earth in the Solar System, hence why most of humanity’s astrobiology efforts are focused there. In addition to the low atmospheric pressure (1/100th of Earth’s at sea level), the surface is subject to extreme temperature variations and is contaminated by perchlorites and toxic metals.

Scientists speculate that if life exists on Mars today, it will likely take the form of microbes living in high-salinity briny patches beneath the surface. As Tomajoli told Universe Today via email, this makes extremophiles (like Artemia franciscana) ideal test subjects for predicting what life is like in similar planetary environments:

“The definition of life is crucial, especially when searching for traces of it on other planetary bodies (e.g., Mars), where life might not exist as we traditionally imagine it. Artemia cysts present an interesting case: in their dormant state, they cannot be classified as living but rather as potential life. Studying organisms with such characteristics helps broaden the perspective in astrobiological research.”

In particular, extremophiles present opportunities for researching species adaptation, which has become a major focus of scientific research due to anthropogenic Climate Change. Worldwide, rising carbon emissions and increasing temperatures are leading to changes in weather patterns, increased ocean acidity, drought, wildfires, and the loss of habitats. As a result, countless marine and terrestrial species are forced to adapt to conditions that are becoming more extreme.

In this April 30, 2021, file image taken by the Mars Perseverance rover and made available by NASA, the Mars Ingenuity helicopter, right, flies over the surface of the planet. Credit: NASA/JPL-Caltech/ASU/MSSS

“In the context of climate change, life conditions are shifting toward extreme boundaries, making survival more challenging for many organisms,” Tomajoli added. “Extremophiles, which thrive in Earth’s most remote environments, are valuable models for understanding metabolic adaptations. Their apparent simplicity is, in fact, an advantage, allowing them to adapt better than more complex organisms to extreme environmental constraints.”

Tomajoli and her colleagues chose Artemia franciscana for their study, a species of brine shrimp known to thrive in high-salinity environments. The eggs they produce, known as cysts, are dormant and can be stored indefinitely, making them extremely useful for aquaculture and scientific research. As Tomajoli indicated, they have also been used in previous space missions, including the Biostack experiment on the Apollo 16 and 17 missions and the ESA’s EXPOSE platform mounted on the International Space Station’s (ISS) exterior.

These experiments all tested the resilience of certain life forms and their progeny to cosmic rays. However, as Tomajoli added, no further studies have been conducted regarding the physiological adaptations of Artemia franciscana, and there is currently no scientific literature available on the topic:

“In particular, Artemia brine shrimps are considered halophiles (literally “salt-loving” organisms) and thrive in environments that can be considered Mars analogs (or laboratories for Mars studies) such as temporary lakes that undergo frequent evaporation, prompting Artemia to produce cryptobiotic cysts. Additionally, Artemia is an easily cultivable model, making it suitable for biological and astrobiological experiments. A recent article by Kayatsha et al., 2024  also showed that Artemia franciscana was among all the microinvertebrates that were tested, the more resistant one to perchlorates salts present in the regolith of simulated martian soil.”

Artist’s impression of water under the Martian surface. Credit: ESA

For their experiment, Tomajoli and her colleagues placed dormant cysts in Mars-like pressure conditions. Once they hatched into nauplii, the team analyzed their aerobic and anaerobic metabolism, mitochondrial function, and oxidative stress. As indicated in their paper, brine shrimp born in Martian pressure conditions managed to adapt quite well. They further share how these results could lead to further studies to evaluate the metabolic adaptations of the cysts to longer exposure times, combinations of different Mars-like conditions, or studies of the adaptations of the nauplii in other stages of development:

“Artemia franciscana showed an exciting potential for physiological adaptations, enabling organisms to cope with the environmental challenges they encounter in space… Nauplii’s cells appear to activate responses to avoid mitochondrial dysfunction and continue their growth processes. These adaptation mechanisms highlight Artemia franciscana’s resilience and ability to thrive in hostile environmental conditions. The results reported in this study further support the potential use of Artemia franciscana for astrobiological purposes, highlighting the animals’ metabolic and redox state changes as a response to adaptation to an extreme condition mimicking the space.”

The implications of this research are far-reaching, embracing astrobiology, human space exploration, and mitigating the effects of Climate Change. Not only could it help point the way toward potential life on Mars, in the interior oceans of icy bodies, and other extreme environments. It could also inform future missions to Mars and other deep-space destinations, where astronauts will need to rely on closed-loop bioregenerative life support systems (BLSS), grow their own food, and conduct research into the effects of exposure to lower gravity, elevated radiation, and other harsh conditions.

At home, the study of extremophiles and adaptation mechanisms could provide insight into climate resilience and adaptation, consistent with the goals outlined in the Sixth Assessment Report (AR6) by the Intergovernmental Panel on Climate Change (IPCC). As they summarize in their paper:

“Understanding the mechanisms of Artemia franciscana adaptations to space-simulated conditions could provide new insights into the study of the limits of life, as well as contribute to the search for biosignatures—traces of past life on other planetary bodies. Additionally, it could offer a viable solution for the long-term survival of human space missions, helping establish self-sustaining populations in confined environments. Artemia could serve as a renewable food source for astronauts, given its richness in essential nutrients, including proteins, lipids, and vitamins.”

Tomajoli and her colleagues have also conducted simulations with a full Mars-like atmosphere for longer periods of time. The paper describing this experiment will be released soon. In the meantime, the search for life on Mars and beyond continues. Knowing it can exist out there and under what conditions will help narrow that search and encourage us to keep investigating.

Further Reading: Science Direct

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