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By NASA
6 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
NASA’s Perseverance rover discovered “leopard spots” on a reddish rock nicknamed “Cheyava Falls” in Mars’ Jezero Crater in July 2024. Scientists think the spots may indicate that, billions of years ago, the chemical reactions in this rock could have supported microbial life; other explanations are being considered.NASA/JPL-Caltech/MSSS An annotated version of the image of “Cheyava Falls” indicates the markings akin to leopard spots, which have particularly captivated scientists, and the olivine in the rock. The image was captured by the WATSON instrument on NASA’s Perseverance Mars rover on July 18.NASA/JPL-Caltech/MSSS The six-wheeled geologist found a fascinating rock that has some indications it may have hosted microbial life billions of years ago, but further research is needed.
A vein-filled rock is catching the eye of the science team of NASA’s Perseverance rover. Nicknamed “Cheyava Falls” by the team, the arrowhead-shaped rock contains fascinating traits that may bear on the question of whether Mars was home to microscopic life in the distant past.
Analysis by instruments aboard the rover indicates the rock possesses qualities that fit the definition of a possible indicator of ancient life. The rock exhibits chemical signatures and structures that could possibly have been formed by life billions of years ago when the area being explored by the rover contained running water. Other explanations for the observed features are being considered by the science team, and future research steps will be required to determine whether ancient life is a valid explanation.
The rock — the rover’s 22nd rock core sample — was collected on July 21, as the rover explored the northern edge of Neretva Vallis, an ancient river valley measuring a quarter-mile (400 meters) wide that was carved by water rushing into Jezero Crater long ago.
“Cheyava Falls” (left) shows the dark hole where NASA’s Perseverance took a core sample; the white patch is where the rover abraded the rock to investigate its composition. A rock nicknamed “Steamboat Mountain” (right) also shows an abrasion patch. This image was taken by Mastcam-Z on July 23.NASA/JPL-Caltech/ASU/MSSS NASA’s Perseverance used its Mastcam-Z instrument to view the “Cheyava Falls” rock sample within the rover’s drill bit. Scientists believe markings on the rock contain fascinating traits that may bear on the question of whether Mars was home to microscopic life in the distant past.NASA/JPL-Caltech/ASU/MSSS “We have designed the route for Perseverance to ensure that it goes to areas with the potential for interesting scientific samples,” said Nicola Fox, associate administrator, Science Mission Directorate at NASA Headquarters in Washington. “This trip through the Neretva Vallis riverbed paid off as we found something we’ve never seen before, which will give our scientists so much to study.”
Multiple scans of Cheyava Falls by the rover’s SHERLOC (Scanning Habitable Environments with Raman & Luminescence for Organics & Chemicals) instrument indicate it contains organic compounds. While such carbon-based molecules are considered the building blocks of life, they also can be formed by non-biological processes.
“Cheyava Falls is the most puzzling, complex, and potentially important rock yet investigated by Perseverance,” said Ken Farley,Perseverance project scientist of Caltech in Pasadena. “On the one hand, we have our first compelling detection of organic material, distinctive colorful spots indicative of chemical reactions that microbial life could use as an energy source, and clear evidence that water — necessary for life — once passed through the rock. On the other hand, we have been unable to determine exactly how the rock formed and to what extent nearby rocks may have heated Cheyava Falls and contributed to these features.”
NASA’s Perseverance rover used its Mastcam-Z instrument to capture this 360-degree panorama of a region on Mars called “Bright Angel,” where an ancient river flowed billions of years ago. “Cheyava Falls” was discovered in the area slightly right of center, about 361 feet (110 meters) from the rover.NASA/JPL-Caltech/ASU/MSSS Other details about the rock, which measures 3.2 feet by 2 feet (1 meter by 0.6 meters) and was named after a Grand Canyon waterfall, have intrigued the team, as well.
How Rocks Get Their Spots
In its search for signs of ancient microbial life, the Perseverance mission has focused on rocks that may have been created or modified long ago by the presence of water. That’s why the team homed in on Cheyava Falls.
“This is the kind of key observation that SHERLOC was built for — to seek organic matter as it is an essential component of a search for past life,” said SHERLOC’s principal investigator Kevin Hand of NASA’s Jet Propulsion Laboratory in Southern California, which manages the mission.
Running the length of the rock are large white calcium sulfate veins. Between those veins are bands of material whose reddish color suggests the presence of hematite, one of the minerals that gives Mars its distinctive rusty hue.
When Perseverance took a closer look at these red regions, it found dozens of irregularly shaped, millimeter-size off-white splotches, each ringed with black material, akin to leopard spots. Perseverance’s PIXL (Planetary Instrument for X-ray Lithochemistry) instrument has determined these black halos contain both iron and phosphate.
As shown in this graphic, astrobiologists catalog a seven-step scale, called the CoLD (Confidence of Life Detection) scale, to research whether a sample could indicate life. This “Cheyava Falls” sample is an example of Step One: “Detect possible signal.” Much additional research must be conducted to learn more.NASA/Aaron Gronstal “These spots are a big surprise,” said David Flannery, an astrobiologist and member of the Perseverance science team from the Queensland University of Technology in Australia. “On Earth, these types of features in rocks are often associated with the fossilized record of microbes living in the subsurface.”
Spotting of this type on sedimentary terrestrial rocks can occur when chemical reactions involving hematite turn the rock from red to white. Those reactions can also release iron and phosphate, possibly causing the black halos to form. Reactions of this type can be an energy source for microbes, explaining the association between such features and microbes in a terrestrial setting.
In one scenario the Perseverance science team is considering, Cheyava Falls was initially deposited as mud with organic compounds mixed in that eventually cemented into rock. Later, a second episode of fluid flow penetrated fissures in the rock, enabling mineral deposits that created the large white calcium sulfate veins seen today and resulting in the spots.
Another Puzzle Piece
While both the organic matter and the leopard spots are of great interest, they aren’t the only aspects of the Cheyava Falls rock confounding the science team. They were surprised to find that these veins are filled with millimeter-size crystals of olivine, a mineral that forms from magma. The olivine might be related to rocks that were formed farther up the rim of the river valley and that may have been produced by crystallization of magma.
If so, the team has another question to answer: Could the olivine and sulfate have been introduced to the rock at uninhabitably high temperatures, creating an abiotic chemical reaction that resulted in the leopard spots?
“We have zapped that rock with lasers and X-rays and imaged it literally day and night from just about every angle imaginable,” said Farley. “Scientifically, Perseverance has nothing more to give. To fully understand what really happened in that Martian river valley at Jezero Crater billions of years ago, we’d want to bring the Cheyava Falls sample back to Earth, so it can be studied with the powerful instruments available in laboratories.”
More Mission Information
A key objective of Perseverance’s mission on Mars is astrobiology, including caching samples that may contain signs of ancient microbial life. The rover will characterize the planet’s geology and past climate, to help pave the way for human exploration of the Red Planet and as the first mission to collect and cache Martian rock and regolith.
NASA’s Mars Sample Return Program, in cooperation with ESA (European Space Agency), is designed to send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis.
The Mars 2020 Perseverance mission is part of NASA’s Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet.
NASA’s Jet Propulsion Laboratory, which is managed for the agency by Caltech, built and manages operations of the Perseverance rover.
For more about Perseverance:
science.nasa.gov/mission/mars-2020-perseverance
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karen.c.fox@nasa.gov / erin.morton@nasa.gov
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Last Updated Jul 25, 2024 Related Terms
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4 min read UPDATED: 10 Things for Mars 10
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By NASA
4 Min Read 10 Things for Mars 10
Both Shadow and Substance: The dramatic image of NASA’s Mars Exploration Rover Opportunity’s shadow was taken on sol 180 (July 26, 2004), by the rover’s front hazard-avoidance camera as the rover moved farther into Endurance Crater in the Meridiani Planum region of Mars. Credits:
NASA/JPL Scientists from around the world are gathering this week in California to take stock of the state of science from Mars and discuss goals for the next steps in exploration of the Red Planet. In the spirit of Mars 10, formally known as the 10th International Conference on Mars, here are 10 recent significant events that got scientists talking:
1. An International Science Fleet at Mars
July 2024: Nine spacecraft are now operating at Mars – two surface rovers and seven orbiters. NASA’s fleet includes the Perseverance and Curiosity rovers, and orbiters MAVEN, Mars Reconnaissance Orbiter, and Mars Odyssey. ESA (European Space Agency) operates Mars Express and the ExoMars Trace Gas Orbiter. Both China and the United Arab Emirates also have spacecraft studying Mars from orbit.
Mars Relay Network: Interplanetary Internet 2. Curiosity Discovers Mysterious Surge in Methane – Which Then Vanishes
June 2019: NASA’s Curiosity Mars rover found a surprising result: the largest amount of methane ever measured during the mission. “The methane mystery continues,” said Ashwin Vasavada, Curiosity’s project scientist. “We’re more motivated than ever to keep measuring and put our brains together to figure out how methane behaves in the Martian atmosphere.”
“Curiosity’s Mars Methane Mystery Continues” 3. Curiosity Discovers Evidence of Ancient Wave Ripples From a Lake Bottom
February 2023: NASA’s Curiosity rover team was surprised to discover the mission’s clearest evidence yet of ancient water ripples that formed within lakes in an area they expected to be much drier.
“NASA’s Curiosity Finds Surprise Clues to Mars’ Watery Past” 4. InSight Detects First Quake on Another Planet
April 2019: NASA’s Mars InSight lander measured and recorded for the first time ever a “marsquake.” “InSight’s first readings carry on the science that began with NASA’s Apollo missions,” said InSight Principal Investigator Bruce Banerdt. “We’ve been collecting background noise up until now, but this first event officially kicks off a new field: Martian seismology!”
“NASA’s InSight Detects First Likely ‘Quake’ on Mars” 5. InSight Provides First View of Mars’ Deep Interior
July 2021: NASA’s InSight spacecraft’s seismometer revealed details about the planet’s deep interior for the first time, including confirmation that the planet’s center is molten.
“NASA’s InSight Reveals the Deep Interior of Mars” 6. InSight Finds Stunning Impact on Mars – and Ice
October 2022: NASA’s InSight felt the ground shake during the impact while cameras aboard the Mars Reconnaissance Orbiter spotted the yawning new crater surrounded by boulder-sized chunks of ice from space.
“NASA’s InSight Lander Detects Stunning Meteoroid Impact on Mars” 7. Opportunity Rover Comes to an End After Nearly 15 Years
July 2021: One of the most successful and enduring feats of interplanetary exploration, NASA’s Opportunity rover mission ended after almost 15 years exploring the surface of Mars and helping lay the groundwork for NASA’s return to the Red Planet.
“NASA’s Opportunity Rover Mission on Mars Comes to End” 8. Massive Dust Storm Spreads Across Mars
July 2018: For scientists watching the Red Planet from NASA’s orbiters, summer 2018 was a windfall. “Global” dust storms, where a runaway series of storms create a dust cloud so large they envelop the planet, only appear every six to eight years (that’s 3-4 Mars years). In June 2018, one of these dust events rapidly engulfed the planet. Scientists first observed a smaller-scale dust storm on May 30. By June 20, it had gone global.
“’Storm Chasers’ on Mars Searching for Dusty Secrets” 9. NASA Maps Water Ice on Mars for Use by Future Astronauts
October 2023: The map could help the agency decide where the first astronauts to the Red Planet should land. The more available water, the less missions will need to bring.
“NASA Is Locating Ice on Mars With This New Map” 10. Mars Reconnaissance Orbiter Images Used to Make Massive Interactive Globe of Mars
April 2023: Cliffsides, impact craters, and dust devil tracks are captured in mesmerizing detail in a new mosaic of the Red Planet composed of 110,000 images from NASA’s Mars Reconnaissance Orbiter (MRO).
“New Interactive Mosaic Uses NASA Imagery to Show Mars in Vivid Detail” Read More
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By NASA
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
The cockpit of an old MD-90 aircraft arrived at NASA’s Armstrong Flight Research Center in Edwards, California, in March 2024. Parts will be used to build a simulator for NASA’s X-66, the demonstration aircraft for the Sustainable Flight Demonstrator project.NASA/Steve Freeman NASA’s X-66 aircraft, the centerpiece of its Sustainable Flight Demonstrator project, is taking the term “sustainable” to heart by reusing an old MD-90 cockpit as a base for its new X-66 simulator.
When airplanes are retired, they often wind up in “boneyards” — storage fields where they spend years being picked over for parts by manufacturers, researchers, engineers, and designers. That’s where the X-66 team found their new X-66 simulator cockpit, before sending it to NASA’s Armstrong Flight Research Center in Edwards, California.
The project will catalog, clean, and disassemble the MD-90 cockpit to use for the simulator. This is where the Simulation Engineering Branch at NASA Armstrong steps in. The team develops high-fidelity engineering simulators that allow pilots and engineers to run real-life scenarios in a safe environment.
The cockpit of an old MD-90 aircraft arrived at NASA’s Armstrong Flight Research Center in Edwards, California, in March 2024. Parts will be used to build a simulator for NASA’s X-66, the demonstration aircraft for the Sustainable Flight Demonstrator project.NASA/Steve Freeman As with any X-plane, a simulator allows researchers to test unknowns without risking the pilot’s safety or the aircraft’s structural integrity. A simulator also affords the team the ability to work out design challenges during the build of the aircraft, ensuring that the final product is as efficient as possible.
To assemble the X-66, the project team will use the airframe from another MD-90, shortening it, installing new engines, and replacing the wing assemblies with a truss-braced wing design.
The Sustainable Flight Demonstrator project is NASA’s effort to develop more efficient airframes as the nation moves toward sustainable aviation. In addition to the X-66’s revolutionary wing design, the project team will work with industry, academia, and other government organizations to identify, select, and mature sustainable airframe technologies.
The project seeks to inform the next generation of single-aisle airliner, the workhorse of commercial aviation fleets around the world. Boeing and NASA are partnering to develop the experimental demonstrator aircraft.
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Last Updated Jul 18, 2024 Related Terms
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By NASA
The latest crew chosen by NASA to venture on a simulated trip to Mars inside the agency’s Human Exploration Research Analog. From left are Sergii Iakymov, Erin Anderson, Brandon Kent, and Sarah Elizabeth McCandless.Credit: C7M3 Crew NASA selected a new team of four research volunteers to participate in a simulated mission to Mars within HERA (Human Exploration Research Analog) at the agency’s Johnson Space Center in Houston.
Erin Anderson, Sergii Iakymov, Brandon Kent, and Sarah Elizabeth McCandless will begin their simulated trek to Mars on Friday, Aug. 9. The volunteer crew members will stay inside the 650-square-foot habitat for 45 days, exiting Monday, Sept. 23 after a simulated “return” to Earth. Jason Staggs and Anderson Wilder will serve as alternate crew members.
The HERA missions offer scientific insights into how people react to the type of isolation, confinement, work and life demands, and remote conditions astronauts might experience during deep space missions.
The facility supports more frequent, shorter-duration simulations in the same building as CHAPEA (Crew Health and Performance Analog). This crew is the third group of volunteers to participate in a simulated Mars mission in HERA this year. The most recent crew completed its HERA mission on June 24. In total, there will be four analog missions in this series.
During this summer’s simulation, participants will perform a mix of science and operational tasks, including harvesting plants from a hydroponic garden, growing shrimp, deploying a small, cube-shaped satellite (CubeSat) to simulate gathering virtual data for analysis, “walking” on the surface of Mars using virtual reality goggles, and flying simulated drones on the simulated Mars surface. The team members also will encounter increasingly longer communication delays with Mission Control throughout their mission, culminating in five-minute lags as they “near” Mars. Astronauts traveling to Mars may experience communications delays of up to 20 minutes.
NASA’s Human Research Program will conduct 18 human health experiments during each of the 2024 HERA missions. Collectively, the studies explore how a Mars-like journey may affect the crew members’ mental and physical health. The work also will allow scientists to test certain procedures and equipment designed to keep astronauts safe and healthy on deep space missions.
Primary Crew
Erin Anderson
Erin Anderson is a structural engineer at NASA’s Langley Research Center in Virginia. Her work focuses on manufacturing and building composite structures — using materials engineered to optimize strength, stiffness, and density — that fly in air and space.
Anderson earned a bachelor’s degree in Aerospace Engineering from the University of Illinois at Urbana-Champaign in 2013. After graduating, she worked as a structural engineer for Boeing on NASA’s SLS (Space Launch System) in Huntsville, Alabama. She moved to New Orleans to support the assembly of the first core stage of the SLS at NASA’s Michoud Assembly Facility. Anderson received a master’s degree in Aeronautical Engineering from Purdue University in West Lafayette, Indiana, in 2020. She started her current job in 2021, continuing her research on carbon fiber composites.
In her free time, Anderson enjoys playing rugby, doting on her dog, Sesame, and learning how to ride paddleboard at local beaches.
Sergii Iakymov
Sergii Iakymov is an aerospace engineer with more than 15 years of experience in research and design, manufacturing, quality control, and project management. Iakymov currently serves as the director of the Mars Desert Research Station, a private, Utah-based research facility that serves as an operational and geological Mars analog.
Iakymov received a bachelor’s degree in Aviation and Cosmonautics and a master’s in Aircraft Control Systems from Kyiv Polytechnic Institute in Ukraine. His graduate research focused on the motion of satellites equipped with pitch flywheels and magnetic coils.
Iakymov was born in Germany, raised in Ukraine, and currently splits his time between southern Utah and Chino Hills, California. His hobbies include traveling, running, hiking, scuba diving, photography, and reading.
Brandon Kent
Brandon Kent is a medical director in the pharmaceutical industry, supporting ongoing global efforts to develop new therapies across cancer types.
Kent received a bachelor’s degrees in Biochemistry and Biology from North Carolina State University in Raleigh. He earned his doctorate in Biomedicine from Mount Sinai School of Medicine in New York City, where his work primarily focused on how genetic factors regulate early embryonic development and cancer development.
Following graduate school, Kent moved into scientific and medical communications consulting in oncology, primarily focusing on clinical trial data disclosures, scientific exchange, and medical education initiatives.
Kent and his wife have two daughters. In his spare time, he enjoys spending time with his daughters, flying private aircraft, hiking, staying physically fit, and reading. He lives in Kinnelon, New Jersey.
Sarah Elizabeth McCandless
Sarah Elizabeth McCandless is a navigation engineer for NASA’s Jet Propulsion Laboratory in Southern California. McCandless’ job involves tracking the location and predicting the future trajectory of spacecraft, including the Mars Perseverance rover, Artemis I, Psyche, and Europa Clipper.
McCandless received a bachelor’s in Aerospace Engineering from the University of Kansas in Lawrence, and a master’s in Aerospace Engineering from the University of Texas at Austin, focused on orbital mechanics.
McCandless is originally from Fairway, Kansas, and remains an avid fan of sports teams from her alma mater and hometown. She is active in STEM (science, technology, engineering, and mathematics) outreach and education and enjoys camping, running, traveling with friends and family, and piloting Cessna 172s. She lives in Pasadena, California.
Alternate Crew
Jason Staggs
Jason Staggs is a cybersecurity researcher and adjunct professor of computer science at the University of Tulsa. His research focuses on systems security engineering, infrastructure protection, and resilient autonomous systems. Staggs is an editor for the International Journal of Critical Infrastructure Protection and the Critical Infrastructure Protection book series.
Staggs supported scientific research expeditions with the National Science Foundation at McMurdo Station in Antarctica. He also previously served as a space engineer and medical officer while working as an analog astronaut in the Hawaii Space Exploration Analog and Simulation (HI-SEAS) atop the Mauna Loa volcano.
Staggs received his bachelor’s degree in Information Assurance and Forensics at Oklahoma State University and master’s and doctorate degrees in Computer Science from the University of Tulsa. During his postdoctoral studies at Idaho National Laboratory, Idaho Falls, he investigated electric vehicle charging station vulnerabilities.
In his spare time, Staggs enjoys hiking, building radio systems, communicating with ham radio operators in remote locations, and volunteering as a solar system ambassador for NASA’s Jet Propulsion Laboratory — sharing his passion for astronomy, oceanography, and space exploration with his community.
Anderson Wilder
Anderson Wilder is a Florida Institute of Technology in Melbourne graduate student working on his doctorate in psychology. His research focuses on team resiliency and human-machine interactions. Wilder also works in the campus neuroscience lab, investigating how spaceflight contributes to astronaut neurobehavioral changes.
Wilder previously served as an executive officer and engineer for an analog mission at the Mars Desert Research Station in Utah. There, he performed studies related to crew social dynamics, plant growth, and geology.
Wilder received bachelor’s degrees in Linguistics and Psychology from Ohio State University in Columbus. He also received a master’s degree in Space Studies from International Space University in Strasbourg, France, and is completing a second master’s in Cognitive Experimental Psychology from Cleveland State University in Ohio.
Outside of school, Wilder works as a parabolic flight coach, teaching people how to experience reduced-gravity environments. He also enjoys chess, reading, video games, skydiving, and scuba diving. On a recent dive, he explored a submerged section of the Great Wall of China.
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NASA’s Human Research Program
NASA’s Human Research Program (HRP) pursues the best methods and technologies to support safe, productive human space travel. Through science conducted in laboratories, ground-based analogs, and the International Space Station, HRP scrutinizes how spaceflight affects human bodies and behaviors. Such research drives HRP’s quest to innovate ways to keep astronauts healthy and mission-ready as space travel expands to the Moon, Mars, and beyond.
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By NASA
5 min read
NASA: Life Signs Could Survive Near Surfaces of Enceladus and Europa
Europa, a moon of Jupiter, and Enceladus, a moon of Saturn, have evidence of oceans beneath their ice crusts. A NASA experiment suggests that if these oceans support life, signatures of that life in the form of organic molecules (e.g. amino acids, nucleic acids, etc.) could survive just under the surface ice despite the harsh radiation on these worlds. If robotic landers are sent to these moons to look for life signs, they would not have to dig very deep to find amino acids that have survived being altered or destroyed by radiation.
“Based on our experiments, the ‘safe’ sampling depth for amino acids on Europa is almost 8 inches (around 20 centimeters) at high latitudes of the trailing hemisphere (hemisphere opposite to the direction of Europa’s motion around Jupiter) in the area where the surface hasn’t been disturbed much by meteorite impacts,” said Alexander Pavlov of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, lead author of a paper on the research published July 18 in Astrobiology. “Subsurface sampling is not required for the detection of amino acids on Enceladus – these molecules will survive radiolysis (breakdown by radiation) at any location on the Enceladus surface less than a tenth of an inch (under a few millimeters) from the surface.”
The frigid surfaces of these nearly airless moons are likely uninhabitable due to radiation from both high-speed particles trapped in their host planet’s magnetic fields and powerful events in deep space, such as exploding stars. However, both have oceans under their icy surfaces that are heated by tides from the gravitational pull of the host planet and neighboring moons. These subsurface oceans could harbor life if they have other necessities, such as an energy supply as well as elements and compounds used in biological molecules.
Dramatic plumes, both large and small, spray water ice and vapor from many locations along the famed “tiger stripes” near the south pole of Saturn’s moon Enceladus. NASA/JPL/Space Science Institute The research team used amino acids in radiolysis experiments as possible representatives of biomolecules on icy moons. Amino acids can be created by life or by non-biological chemistry. However, finding certain kinds of amino acids on Europa or Enceladus would be a potential sign of life because they are used by terrestrial life as a component to build proteins. Proteins are essential to life as they are used to make enzymes which speed up or regulate chemical reactions and to make structures. Amino acids and other compounds from subsurface oceans could be brought to the surface by geyser activity or the slow churning motion of the ice crust.
This view of Jupiter’s icy moon Europa was captured by JunoCam, the public engagement camera aboard NASA’s Juno spacecraft, during the mission’s close flyby on Sept. 29, 2022. The picture is a composite of JunoCam’s second, third, and fourth images taken during the flyby, as seen from the perspective of the fourth image. North is to the left. The images have a resolution of just over 0.5 to 2.5 miles per pixel (1 to 4 kilometers per pixel).
As with our Moon and Earth, one side of Europa always faces Jupiter, and that is the side of Europa visible here. Europa’s surface is crisscrossed by fractures, ridges, and bands, which have erased terrain older than about 90 million years.
Citizen scientist Kevin M. Gill processed the images to enhance the color and contrast.
NASA/JPL-Caltech/SwRI/MSSS Image processing: Kevin M. Gill CC BY 3.0 To evaluate the survival of amino acids on these worlds, the team mixed samples of amino acids with ice chilled to about minus 321 Fahrenheit (-196 Celsius) in sealed, airless vials and bombarded them with gamma-rays, a type of high-energy light, at various doses. Since the oceans might host microscopic life, they also tested the survival of amino acids in dead bacteria in ice. Finally, they tested samples of amino acids in ice mixed with silicate dust to consider the potential mixing of material from meteorites or the interior with surface ice.
This image shows experiment samples loaded in the specially designed dewar which will be filled with liquid nitrogen shortly after and placed under gamma radiation. Notice that the flame-sealed test tubes are wrapped in cotton fabric to keep them together because test tubes become buoyant in liquid nitrogen and start floating around in the dewar, interfering with the proper radiation exposure. Candace Davison The experiments provided pivotal data to determine the rates at which amino acids break down, called radiolysis constants. With these, the team used the age of the ice surface and the radiation environment at Europa and Enceladus to calculate the drilling depth and locations where 10 percent of the amino acids would survive radiolytic destruction.
Although experiments to test the survival of amino acids in ice have been done before, this is the first to use lower radiation doses that don’t completely break apart the amino acids, since just altering or degrading them is enough to make it impossible to determine if they are potential signs of life. This is also the first experiment using Europa/Enceladus conditions to evaluate the survival of these compounds in microorganisms and the first to test the survival of amino acids mixed with dust.
The team found that amino acids degraded faster when mixed with dust but slower when coming from microorganisms.
“Slow rates of amino acid destruction in biological samples under Europa and Enceladus-like surface conditions bolster the case for future life-detection measurements by Europa and Enceladus lander missions,” said Pavlov. “Our results indicate that the rates of potential organic biomolecules’ degradation in silica-rich regions on both Europa and Enceladus are higher than in pure ice and, thus, possible future missions to Europa and Enceladus should be cautious in sampling silica-rich locations on both icy moons.”
A potential explanation for why amino acids survived longer in bacteria involves the ways ionizing radiation changes molecules — directly by breaking their chemical bonds or indirectly by creating reactive compounds nearby which then alter or break down the molecule of interest. It’s possible that bacterial cellular material protected amino acids from the reactive compounds produced by the radiation.
The research was supported by NASA under award number 80GSFC21M0002, NASA’s Planetary Science Division Internal Scientist Funding Program through the Fundamental Laboratory Research work package at Goddard, and NASA Astrobiology NfoLD award 80NSSC18K1140.
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Last Updated Jul 18, 2024 Editor wasteigerwald Contact wasteigerwald william.a.steigerwald@nasa.gov Location NASA Goddard Space Flight Center Related Terms
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