D J Des Marais studies how to detect signs of life on other planets, especially Mars. His research involves examining the isotopic composition of materials found in Martian rocks to understand the planet's history and its potential to have supported life. He has developed tools and classification systems that assist scientists in identifying biosignatures, which are indicators of life. By investigating minerals and environmental conditions, he sheds light on ancient climates and biological cycles, which can inform our search for extraterrestrial life.
Key findings
Carbon mineral siderite was found in amounts between 4.8% and 10.5% in a study of Mars' Gale Crater, indicating a historical carbon cycle.
In measuring carbon and oxygen isotopes from Martian carbonates, values ranged from 72 to 110 for carbon and 59 to 91 for oxygen, suggesting complex atmospheric processes.
The Astrobiology Resource Metadata Standard improved data discovery, making it easier for researchers to access necessary resources for their studies.
Frequently asked questions
Does Dr. D J Des Marais study the possibility of life on Mars?
Yes, Dr. Des Marais extensively studies the potential for past life on Mars by analyzing rocks and environmental conditions on the planet.
What techniques does Dr. D J Des Marais use to search for signs of life?
He uses isotopic analysis and classifications of biosignatures to help identify life indicators in extraterrestrial environments.
Is Dr. D J Des Marais's work relevant to current space missions?
Yes, his research informs strategies and tools used in current and future space missions aimed at discovering signs of life beyond Earth.
What conditions does Dr. D J Des Marais study?
He studies ancient environments on Mars, focusing on geological formations and water-related conditions that may have supported life.
How does Dr. D J Des Marais's research help scientists?
His research provides vital insights into the history of Mars, improving our understanding of its climate and potential for past microbial life.
Publications in plain English
Carbonates identified by the Curiosity rover indicate a carbon cycle operated on ancient Mars.
Plain English Researchers studied rocks on Mars to learn about its ancient environment, discovering a mineral called siderite in amounts between 4.8% and 10.5% in a 89-meter section of Gale crater. This mineral formed when ancient water interacted with rocks, suggesting a carbon cycle was active on Mars that controlled the levels of carbon dioxide in the atmosphere. The findings indicate that Mars had a complex climate system, which is important for understanding its potential for past life.
Who this helps: This helps scientists studying Mars' climate history and the possibility of life beyond Earth.
Life Detection Knowledge Base: Taxonomy of Potential Biosignatures.
2025
Astrobiology
Davila AF, Hoehler T, Parenteau N, Neveu M, Shkolyar S +10 more
Plain English The research focused on creating a tool called the Life Detection Knowledge Base (LDKB) to improve how scientists search for signs of life beyond Earth. They developed a systematic classification system that helps evaluate different strategies for detecting life, aiming to reduce mistakes in interpreting results. This is important because it enhances our ability to identify real signs of life in future space missions more accurately.
Who this helps: This benefits scientists and researchers involved in space exploration.
Stable Isotope Abundance Patterns as Potential Biosignatures.
2025
Astrobiology
Des Marais DJ, Caro T, Dhingra R, Fox AC, Galloway T +4 more
Plain English This research paper looks at how different stable isotopes, which are variations of elements, can indicate whether a substance comes from living organisms or natural processes. The study found that certain patterns in isotopes, especially of carbon and sulfur, can hint at whether these substances were formed by life or other non-living methods, but more research is needed to understand when these patterns are reliable. This matters because it can help scientists identify signs of life in different environments, such as other planets or ancient Earth environments.
Who this helps: This helps researchers looking for signs of life beyond Earth and those studying ancient ecosystems.
Plain English This study focused on creating a new system called the Astrobiology Resource Metadata Standard (ARMS) to help researchers find relevant astrobiology data more easily. Before ARMS, it was difficult for scientists in this field to locate datasets and other resources because they often have very specific needs. The new standard streamlines the way these resources like datasets, software, and publications are described, making it easier to discover and use them in research.
Who this helps: This helps astrobiology researchers looking for specific data and resources.
Highly enriched carbon and oxygen isotopes in carbonate-derived COat Gale crater, Mars.
2024
Proceedings of the National Academy of Sciences of the United States of America
Burtt DG, Stern JC, Webster CR, Hofmann AE, Franz HB +11 more
Plain English This study looked at carbonates, a type of mineral found on Mars, to understand the planet's ancient environment and its potential for supporting life. The researchers, using data from the Curiosity rover in Gale crater, measured carbon and oxygen isotopes in these carbonates and found that their carbon values ranged from 72 to 110 and oxygen values from 59 to 91, which are much heavier than other materials found on Mars. This unique isotopic signature suggests that special processes, like evaporation or changes during freezing, played a role in their formation, indicating a complex history of Mars’ atmosphere and climate.
Who this helps: This helps scientists studying Mars’ environment and its ability to host life.
Plain English This study looked at rock layers in Gale Crater on Mars, which were formed around 3.5 billion years ago when there was a lake. Researchers found that within a short distance of less than 400 meters, the rocks had different mineral compositions, indicating that salty water had affected them in specific areas. This finding suggests that a process seen rarely on Earth, involving these brines affecting minerals, was common on ancient Mars and helps us understand its geological history.
Who this helps: This helps scientists studying Mars and the potential for past life there.
Carrier BL, Beaty DW, Meyer MA, Blank JG, Chou L +56 more
Plain English The conference "Mars Extant Life: What's Next?" gathered experts who discussed the possibility of finding existing microbial life on Mars. They concluded that Mars may have "oases" or refugia—like caves or deep ice—where life could survive better than in harsh areas. The group also talked about various strategies and tools to find signs of life, noting that returning samples to Earth could provide much more detailed detection methods than what we can use on Mars.
Who this helps: This research benefits scientists and astronomers as they explore the potential for life on Mars.
Evidence for Multiple Diagenetic Episodes in Ancient Fluvial-Lacustrine Sedimentary Rocks in Gale Crater, Mars.
2020
Journal of geophysical research. Planets
Achilles CN, Rampe EB, Downs RT, Bristow TF, Ming DW +27 more
Plain English This study looked at rocks and soils in Gale Crater on Mars to understand their geological history. Researchers examined four rock samples and found that their mineral makeup changed due to past water conditions, including different types and temperatures of water. They discovered that water-related activities significantly influenced the rocks, showing a shift from magnetite to hematite, indicating more oxygen-rich conditions over time.
Who this helps: This research benefits planetary scientists and geologists studying Mars.
Plain English This research focused on how to identify signs of life, called biosignatures, on Earth and in other planets. The researchers outlined three main types of biosignatures, which include specific substances, physical features, and patterns, all of which help distinguish living organisms from nonliving processes. They highlighted five key challenges that need to be addressed, such as examining the right scales and contexts to improve detection methods.
Who this helps: This benefits astrobiologists and researchers in the search for life beyond Earth.
Carbon isotopic composition of lipid biomarkers from an endoevaporitic gypsum crust microbial mat reveals cycling of mineralized organic carbon.
2019
Geobiology
Jahnke LL, Des Marais DJ
Plain English This study looked at tiny, mat-like communities of microbes living in gypsum deposits in Mexico to understand how carbon moves through these ecosystems. Researchers measured the carbon signatures in different layers of the microbial mats and found that the carbon composition changed significantly from the top layer to the bottom, with differences as large as 14.7‰, indicating that organic matter with richer carbon collects deeper underground. These findings matter because they help explain the life cycles and energy flows in these unusual ecosystems, which could have implications for understanding broader environmental carbon cycling.
Who this helps: This helps researchers and environmental scientists studying carbon cycling and microbial ecology.
Plain English This research looks at how hot springs on land can support a variety of tiny life forms and help preserve their fossils. The study highlights that these springs provide essential water and nutrients, creating environments where microbes can thrive. The findings indicate that fossils from these springs are found dating back to about 3.48 billion years, making them crucial for understanding both early life on Earth and potential life on Mars, where similar features have been detected.
Who this helps: This helps scientists studying microbial life and the search for extraterrestrial life.
Plain English This study examined the types and amounts of clay minerals in ancient mudstones at Gale Crater on Mars, which are about 3.5 billion years old. Researchers found that these rocks contain up to 28% clay minerals, with different species indicating past environments; for example, lakes that dried up saw the formation of certain clay minerals due to changes in water levels. Understanding these changes is important because they shed light on Mars' climate history and the potential for past life.
Who this helps: This helps scientists studying Mars' history and the possibility of past life.
Low Hesperianconstrained from in situ mineralogical analysis at Gale Crater, Mars.
2017
Proceedings of the National Academy of Sciences of the United States of America
Bristow TF, Haberle RM, Blake DF, Des Marais DJ, Eigenbrode JL +9 more
Plain English This study looked at the levels of carbon dioxide in the atmosphere of Mars around 3.5 billion years ago when there were lakes on the planet. Researchers found that the carbon dioxide levels were very low, about 10 millibar, which is not enough to keep water from freezing. This finding raises questions about how Martian lakes could exist in such cold conditions and suggests that we might not fully understand the factors that influenced the planet's climate.
Who this helps: This helps scientists understand Mars' climate history and the potential for past life on the planet.
Biosignature Preservation and Detection in Mars Analog Environments.
2017
Astrobiology
Hays LE, Graham HV, Des Marais DJ, Hausrath EM, Horgan B +5 more
Plain English This research paper reviews discussions from a conference about how to find signs of life, called biosignatures, in environments similar to Mars. It focuses on five specific environments where scientists think biosignatures might be preserved and found, like hydrothermal springs and underwater settings. The findings highlighted the need for better tools and strategies to explore Mars, as well as understanding how its environment may differ from Earth's, which could impact how we detect any signs of past life.
Who this helps: This helps scientists and researchers who are studying Mars and seeking evidence of past life on the planet.
Plain English This study looked at a rock sample from Mars and found a mineral called tridymite, which usually forms in very hot volcanic environments. The researchers discovered that the rock is made up of about 74% silica and contains other minerals like plagioclase and cristobalite. These findings suggest that Mars experienced volcanic activity that may have contributed to the composition of this sediment, which is important for understanding the planet's geological history and potential for past water.
Who this helps: This helps scientists studying Mars' geological history and potential habitability.
Plain English This study focused on unusual sand formations on Mars created by wind, which are different from what we see on Earth. Researchers found that these formations, called wind-drag ripples, are about one meter long and have unique shapes that indicate they formed in Mars' thin atmosphere roughly 3.7 billion years ago. Understanding these features helps scientists learn more about the history of Mars' atmosphere and how it has changed over time.
Who this helps: This helps researchers and scientists studying Mars and its atmospheric history.
Organic molecules in the Sheepbed Mudstone, Gale Crater, Mars.
2015
Journal of geophysical research. Planets
Freissinet C, Glavin DP, Mahaffy PR, Miller KE, Eigenbrode JL +33 more
Plain English This study looked at organic molecules in the mudstone at Gale Crater on Mars using a special instrument on the Curiosity rover. Researchers found chlorobenzene at levels between 150 and 300 parts per billion, and dichloroalkanes at up to 70 parts per billion, suggesting these compounds might come from Martian sources or from materials like meteorites. This is important because discovering these organic molecules helps us understand if Mars ever had conditions that could support life and guides future searches for evidence of life on the planet.
Who this helps: This helps scientists and researchers studying Mars' habitability and the potential for past life on the planet.
Mineralogy of a mudstone at Yellowknife Bay, Gale crater, Mars.
2014
Science (New York, N.Y.)
Vaniman DT, Bish DL, Ming DW, Bristow TF, Morris RV +32 more
Plain English Researchers studied mudstone rocks at Yellowknife Bay on Mars, which were collected by the Curiosity rover. They found different minerals, including some that suggest Mars had water in its history. Notably, one type of clay showed signs of being able to hold water, indicating these materials formed later than previously thought.
Who this helps: This helps scientists studying Mars and its geological history.
Elemental geochemistry of sedimentary rocks at Yellowknife Bay, Gale crater, Mars.
2014
Science (New York, N.Y.)
McLennan SM, Anderson RB, Bell JF, Bridges JC, Calef F +46 more
Plain English Researchers studied rocks at Yellowknife Bay on Mars using the Curiosity rover to understand their chemistry and formation. They found that the rocks originated from a mix of common Martian materials and alkaline lava, with no signs of weathering, which suggests Mars had dry and possibly cold conditions in the past. This research gives us insights into the different environments that shaped Mars early on, showing it had varied conditions for rock formation and alteration.
Who this helps: This helps scientists studying Mars' climate history and geology.
Volatile and organic compositions of sedimentary rocks in Yellowknife Bay, Gale crater, Mars.
2014
Science (New York, N.Y.)
Ming DW, Archer PD, Glavin DP, Eigenbrode JL, Franz HB +53 more
Plain English Researchers studied two mudstone samples from Mars's Yellowknife Bay to discover what gases were released when these rocks were heated. They found various gases, like water vapor, carbon dioxide, and sulfur dioxide, with some mudstone samples showing higher amounts of chlorinated hydrocarbons, which could indicate the presence of organic material on Mars. This is important because it suggests that there may be native Martian organic carbon preserved in the rocks, which could mean that Mars had the conditions to support life.
Who this helps: This helps scientists studying the potential for life on Mars.
Molecular and lipid biomarker analysis of a gypsum-hosted endoevaporitic microbial community.
2014
Geobiology
Jahnke LL, Turk-Kubo KA, N Parenteau M, Green SJ, Kubo MD +3 more
Plain English This study examined a microbial community found in gypsum deposits in Guerrero Negro, Mexico, to learn more about how early life on Earth may have worked. Researchers found two different layers of microbes with cell densities of 1.6 billion and 4.2 billion cells per cubic centimeter. They identified specific biomolecules that are linked to certain bacteria, which provide insights into the types of microorganisms living in these unique environments.
Who this helps: This research benefits scientists studying ancient life and microbial ecosystems.
Spatial variability in photosynthetic and heterotrophic activity drives localized δ13C org fluctuations and carbonate precipitation in hypersaline microbial mats.
Plain English In this study, researchers examined how different microbial activities in highly salty environments influence carbon signatures and the formation of carbonate minerals. They found that the balance between photosynthesis by cyanobacteria and decomposition by bacteria changes the carbon signatures significantly, with variations as large as 2.0‰ in some areas, depending on the microbial community present. This is important because it helps scientists understand how ancient sedimentary records reflect carbon cycling and the environmental conditions that existed when those sediments were formed.
Who this helps: This research benefits scientists studying climate change, ancient environments, and carbon cycling.
Plain English This study looked at a sand deposit on Mars called Rocknest, finding that about 55% of the sand consisted of solid crystals, while the remaining 45% was a less structured, iron-rich material. This less structured material holds important chemicals like water and carbon dioxide, suggesting that these sand deposits contain resources that can be useful for future exploration. The findings indicate that the materials found at Rocknest are similar to those seen at other Martian locations, supporting the idea that they have a common origin.
Who this helps: This helps researchers and scientists exploring Mars for signs of past life and potential resources for human missions.
Preservation of martian organic and environmental records: final report of the Mars biosignature working group.
2011
Astrobiology
Summons RE, Amend JP, Bish D, Buick R, Cody GD +5 more
Plain English Researchers studied Mars to see if it ever had conditions that could support life, using data from a NASA instrument designed to analyze Mars' past and present environment. They found that certain layered rocks on Mars, which can be up to a kilometer thick, might preserve evidence of life, and identified various types of biological signatures, including organic molecules and gases, that their instruments could detect. This research helps us understand Mars' history and its potential to have hosted life, which is important for future explorations of the planet.
Who this helps: This helps scientists and researchers studying Mars and its potential for past life.
The role of biofilms in the sedimentology of actively forming gypsum deposits at Guerrero Negro, Mexico.
2009
Astrobiology
Vogel MB, Des Marais DJ, Turk KA, Parenteau MN, Jahnke LL +1 more
Plain English This study examined the role of microbial communities, called biofilms, in the formation of gypsum deposits in Guerrero Negro, Mexico. Researchers found that these deposits came in various forms, such as thick crusts or layered mats, each supporting diverse types of microbes that contribute to how gypsum forms. Specifically, they categorized the environments where gypsum forms and noted that biofilms help shape the chemical and physical aspects of these sedimentary processes, which is important for understanding both Earth’s geology and potential life on other planets.
Who this helps: Scientists studying geology and astrobiology, as well as anyone interested in the origins of life.
Characterization and spatial distribution of methanogens and methanogenic biosignatures in hypersaline microbial mats of Baja California.
2008
Geobiology
Orphan VJ, Jahnke LL, Embaye T, Turk KA, Pernthaler A +2 more
Plain English This study explored the different types of microorganisms that produce methane in salt-loving microbial mats in Baja California. Researchers found that specific groups of methane-producing organisms, mainly from the Methanosarcinales family, thrive in different layers of these mats, especially when certain substances are added. The findings showed that the makeup of these organisms changes with depth: surface layers had one type (Methanolobus), while deeper layers had others (Methanococcoides). Understanding this microbial diversity is important for grasping how methane is generated in extreme environments.
Who this helps: This helps researchers studying microbial ecosystems and their role in the environment.
Lipid biomarker and phylogenetic analyses to reveal archaeal biodiversity and distribution in hypersaline microbial mat and underlying sediment.
2008
Geobiology
Jahnke LL, Orphan VJ, Embaye T, Turk KA, Kubo MD +2 more
Plain English This study looked at tiny microorganisms called archaea in a salty lagoon in Baja California by analyzing the types of lipids they produce and their genetic makeup. Researchers found that archaea made up 1 to 4% of all cells in the top layers of the sediment and microbial mat, and even more were found deeper down, with a significant dominance of specific groups like Thermoplasmatales and Halobacteriaceae. These findings help us understand the biodiversity of these unique microorganisms, which play a crucial role in the ecosystem of hypersaline environments.
Who this helps: This helps scientists and environmental researchers studying microbial life in extreme environments.
Des Marais DJ, Nuth JA, Allamandola LJ, Boss AP, Farmer JD +6 more
Plain English This research outlines NASA's Astrobiology Roadmap, which guides studies on life in the universe, including how life began and evolved and whether it exists elsewhere. The roadmap emphasizes seven key goals, such as finding habitable environments and studying early life on Earth, with 18 specific objectives planned for the next few years to support these investigations. This is important because understanding life on Earth and beyond can expand our knowledge of biology and the potential for life elsewhere in space.
Who this helps: This helps scientists and researchers studying the origins of life and the conditions necessary for life to thrive.
An integrated view of the chemistry and mineralogy of martian soils.
2005
Nature
Yen AS, Gellert R, Schröder C, Morris RV, Bell JF +31 more
Plain English This study looked at the makeup of Martian soil to understand its weathering processes. Researchers found that the soil on both sides of Mars has similar characteristics, indicating that it is part of a larger global system rather than just influenced by local rocks. They discovered that Martian soils have high levels of bromine, suggesting some interaction with liquid water, but also contain olivine, showing that significant wet alteration hasn’t occurred. Notably, nickel levels at the surface hint that the top layer of soil includes up to 1% material from space.
Who this helps: This research helps scientists studying Mars and planning future missions to the planet.
Water alteration of rocks and soils on Mars at the Spirit rover site in Gusev crater.
2005
Nature
Haskin LA, Wang A, Jolliff BL, McSween HY, Clark BC +25 more
Plain English The study focused on examining rocks and soils around the Spirit rover's landing site in Gusev crater on Mars to find signs that water may have once existed there. The researchers found strong evidence of water's interaction with volcanic rocks, including softer rock interiors and higher levels of certain chemicals like sulfur, chlorine, and bromine. This is important because it suggests that the area may have had a wet environment in the past, which is critical for understanding Mars' history and potential for life.
Who this helps: This benefits scientists and researchers studying Mars' geology and the possibility of past life on the planet.
Key science questions from the second conference on early Mars: geologic, hydrologic, and climatic evolution and the implications for life.
2005
Astrobiology
Beaty DW, Clifford SM, Borg LE, Catling DC, Craddock RA +9 more
Plain English Scientists gathered to discuss the first billion years of Mars' history, a time when the planet was highly active and experienced significant geological changes. They explored questions about how processes like volcanism and erosion shaped Mars' atmosphere and surface, and whether conditions for life existed during this period. This research is important because it helps us understand how Mars evolved and whether it might have supported life.
Who this helps: This helps researchers studying potential life on other planets and the evolution of planetary environments.
Stable carbon isotope ratios of lipid biomarkers of sulfate-reducing bacteria.
2004
Applied and environmental microbiology
Londry KL, Jahnke LL, Des Marais DJ
Plain English This study looked at how sulfate-reducing bacteria (SRB) use different food sources and how their fatty acids can reveal this information. The researchers found that when these bacteria eat in various ways, their fatty acids mostly contain less carbon-13, with values dropping between -4 to -17 per thousand. This finding is important because it can help scientists understand how SRB function in nature and their role in the environment.
Who this helps: This research aids environmental scientists studying bacteria's roles in ecosystems.
The Spirit Rover's Athena science investigation at Gusev Crater, Mars.
2004
Science (New York, N.Y.)
Squyres SW, Arvidson RE, Bell JF, Brückner J, Cabrol NA +45 more
Plain English The study focused on the Spirit Rover's exploration of Gusev Crater on Mars, a site believed to have once contained a lake. Researchers found mostly basalt rocks and signs of past impacts rather than clear evidence of lakebed sediments. This is important because it helps us understand Mars' geology and past water presence, which is key to exploring potential habitability.
Who this helps: This benefits scientists and researchers studying Mars and its history of water.
Surficial deposits at Gusev Crater along Spirit Rover traverses.
2004
Science (New York, N.Y.)
Grant JA, Arvidson R, Bell JF, Cabrol NA, Carr MH +19 more
Plain English The study examined the surface of Gusev Crater on Mars, where the Spirit Rover traveled across a flat area filled with rocks created by impacts from space. Researchers found that the rocks came from lava flows located at least 10 meters deep and noted that wind played a role in shaping the landscape, with some rocks affected by small windblown particles. Importantly, the analysis showed no signs that an ancient lake ever existed in this crater.
Who this helps: This helps scientists studying Mars and its geological history.
Basaltic rocks analyzed by the Spirit Rover in Gusev Crater.
2004
Science (New York, N.Y.)
McSween HY, Arvidson RE, Bell JF, Blaney D, Cabrol NA +30 more
Plain English Researchers examined rocks on Mars in Gusev Crater, finding that they are mostly a type of volcanic rock called picritic basalt. These rocks contain crystals and varied coatings, and their chemical makeup suggests they are similar to other known Martian rocks but also broaden the types of materials we know exist on Mars. This research is important because it gives scientists more information about the composition of Mars, helping us understand the planet's history and geology better.
Who this helps: This helps researchers and scientists studying Mars and planning future missions.
Dimethyl sulphide and methanethiol formation in microbial mats: potential pathways for biogenic signatures.
2003
Environmental microbiology
Visscher PT, Baumgartner LK, Buckley DH, Rogers DR, Hogan ME +3 more
Plain English This study examined how certain compounds, dimethyl sulphide (DMS) and methanethiol (MT), are produced and consumed by microbial mats in Guerrero Negro, Mexico. Researchers found that DMS and MT levels increased with lower salinity, higher temperatures, and less oxygen; they observed that significantly more DMS was released at night than during the day. These findings indicate that DMS and MT can serve as markers for the health and activity of microbial communities, revealing important information about carbon and sulfur cycles in these ecosystems.
Who this helps: This helps scientists studying ecosystems and climate change, as well as environmental policymakers.
Biogeochemistry of hypersaline microbial mats illustrates the dynamics of modern microbial ecosystems and the early evolution of the biosphere.
2003
The Biological bulletin
Des Marais DJ
Plain English This study looked at photosynthetic microbial mats, which are tiny ecosystems that thrive in very salty environments. Researchers found that these mats play a crucial role in environmental processes and could be directly linked to some of the earliest forms of life on Earth. Understanding how these microbial communities work together helps us learn more about the origins of life and ecosystems.
Who this helps: This helps scientists and researchers studying the evolution of life and microbial ecosystems.
Stable carbon isotope fractionation by sulfate-reducing bacteria.
2003
Applied and environmental microbiology
Londry KL, Des Marais DJ
Plain English This study examined how sulfate-reducing bacteria (SRB) process carbon under different growth conditions, specifically when they feed on organic materials or carbon dioxide (CO2). The researchers found that for most SRB, the difference in carbon isotopes between the substances they consumed and what they produced was low, typically around 0 to 2 per thousand. However, one type of SRB, Desulfotomaculum acetoxidans, showed a significant difference, incorporating heavier carbon into its biomass by 8 to 9 per thousand, and the growth conditions influenced how these bacteria discriminated against various carbon isotopes.
Who this helps: This research benefits scientists studying environmental processes and the history of carbon cycles in ecosystems.
Des Marais DJ, Allamandola LJ, Benner SA, Boss AP, Deamer D +15 more
Plain English The NASA Astrobiology Roadmap directs research on how life starts and develops, the existence of life beyond Earth, and the future of life both here and in space. It sets seven main goals for exploration, including finding places in the universe where life could exist and understanding how life on Earth has changed over time. The next 3-5 years will focus on 18 specific projects that further these aims.
Who this helps: This benefits scientists and researchers working on questions about life in the universe.
Comparative ecology of H2 cycling in sedimentary and phototrophic ecosystems.
2002
Antonie van Leeuwenhoek
Hoehler TM, Albert DB, Alperin MJ, Bebout BM, Martens CS +1 more
Plain English This study looked at how hydrogen (H2) is managed in two different ecosystems: underwater sediments in North Carolina and light-sensitive microbial mats in Mexico. In North Carolina's sediments, H2 levels were kept consistently low due to bacteria that consume it, while in Mexico, H2 levels varied widely because bacteria produced it in response to light. These differences are important because they affect other microbial processes, such as methane production, which was suppressed in the North Carolina sediments but occurred freely in the Mexican mats when certain conditions were present.
Who this helps: This research benefits environmental scientists studying ecosystem dynamics and methane emissions.
Remote sensing of planetary properties and biosignatures on extrasolar terrestrial planets.
2002
Astrobiology
Des Marais DJ, Harwit MO, Jucks KW, Kasting JF, Lin DN +5 more
Plain English Researchers from NASA and the European Space Agency studied how to detect planets outside our solar system that might support life. They recommend using specific light wavelengths to look for important signs like oxygen and carbon dioxide in these planets' atmospheres. Their findings indicate that certain features, like the size and mass of a planet, are crucial indicators of whether it could be habitable.
Who this helps: This helps astronomers and scientists searching for life beyond Earth.
Long-term manipulations of intact microbial mat communities in a greenhouse collaboratory: simulating earth's present and past field environments.
2002
Astrobiology
Bebout BM, Carpenter SP, Des Marais DJ, Discipulo M, Embaye T +10 more
Plain English This study looked at microbial mats from salty ponds to understand how changes in salt levels affect these communities, which are similar to ancient marine life. Researchers found that after a year in a greenhouse, these mats remained largely unchanged and continued to produce oxygen and other gases like methane, just like they do in their natural habitats. This matters because it helps us learn about the history of life on Earth and how these ecosystems evolved over billions of years.
Who this helps: This research benefits scientists studying the evolution of life and ancient environments.
Signature lipids and stable carbon isotope analyses of Octopus Spring hyperthermophilic communities compared with those of Aquificales representatives.
2001
Applied and environmental microbiology
Jahnke LL, Eder W, Huber R, Hope JM, Hinrichs KU +4 more
Plain English This study looked at the types of lipids, or fats, found in unique microbial communities living in a hot spring called Octopus Spring. Researchers found that the lipids from these microbes showed specific patterns and were different from other types of bacteria, with some fatty acids being less heavy in carbon, indicating a different food source. This matters because it helps us understand how these extreme environments sustain life, revealing potential new metabolic processes.
Who this helps: This helps researchers studying extremophiles and the ecosystems of hot springs.
Chuar Group of the Grand Canyon: record of breakup of Rodinia, associated change in the global carbon cycle, and ecosystem expansion by 740 Ma.
2000
Geology
Karlstrom KE, Bowring SA, Dehler CM, Knoll AH, Porter SM +8 more
Plain English This study looked at rock layers in the Chuar Group of the Grand Canyon, dating back about 742 million years. Researchers found evidence of geological activity and major changes in ocean chemistry that coincided with the breakup of the supercontinent Rodinia. These changes also show an increase in variety among living organisms at that time, highlighting the early steps toward more complex ecosystems.
Who this helps: This benefits scientists and researchers studying Earth's geological history and the evolution of life.
Depositional facies and aqueous-solid geochemistry of travertine-depositing hot springs (Angel Terrace, Mammoth Hot Springs, Yellowstone National Park, U.S.A.).
2000
Journal of sedimentary research. Section A, Sedimentary petrology and processes : an international journal of SEPM (Society for Sedimentary Geology)
Fouke BW, Farmer JD, Des Marais DJ, Pratt L, Sturchio NC +2 more
Plain English This study looked at the hot springs at Angel Terrace in Yellowstone National Park to understand how different temperatures and conditions affect the formation of travertine, a type of mineral deposit. Researchers identified five different types of mineral deposits, with spring water temperatures ranging from 28 to 73 degrees Celsius. They found that while microbes play a role in these environments, the main factors influencing mineral formation are physical and chemical processes rather than biological ones.
Who this helps: This research benefits geologists and environmental scientists studying geothermal systems and sediment formation.
Plain English This study looked at White Smoke Lake in East Antarctica, which is always covered by ice. Researchers found that the lake has a mix of different sediment types and that its environment has been stable for the past 3,000 years, with only small changes. This information is important because it helps scientists understand how glaciers and lakes interact, informing climate change models and the effects on polar regions.
Who this helps: This helps climate scientists and researchers studying the impact of climate change in polar environments.
Carbon isotopic fractionation in lipids from methanotrophic bacteria II: the effects of physiology and environmental parameters on the biosynthesis and isotopic signatures of biomarkers.
1999
Geochimica et cosmochimica acta
Jahnke LL, Summons RE, Hope JM, Des Marais DJ
Plain English This research explored how certain bacteria, which use methane as their main source of carbon, produce specific biomarkers and how their physical and environmental conditions affect these processes. The study found that bacteria growing under certain conditions produced biomarkers with carbon signatures showing a notable difference: those using a specific enzyme type had an isotopic signature of -23.9%, while those using a different type had a signature of -12.6%. These findings are important because they can help identify methanotrophic bacteria in different environments and understand their roles in the carbon cycle, especially when methane is scarce.
Who this helps: This helps scientists studying environmental change and carbon cycling.
Plain English Researchers are planning how to search for signs of ancient life on Mars by studying how fossils are preserved on Earth. They found that certain rocks, like those made of silica or phosphate, keep tiny fossils safe for a long time, which is important for finding similar fossils on Mars. Understanding how these fossils survive can help improve the chances of discovering Martian life forms that may have existed billions of years ago.
Who this helps: This helps scientists and researchers involved in space exploration and astrobiology.
Astrobiology: exploring the origins, evolution, and distribution of life in the Universe.
1999
Annual review of ecology and systematics
Des Marais DJ, Walter MR
Plain English This research studied how life might have started and evolved on Earth and whether it exists elsewhere in the universe. Scientists found that life can thrive in extreme conditions and that many planets suitable for life are out there. By understanding how planets support life, researchers aim to better identify signs of life on other worlds.
Who this helps: This benefits scientists and researchers working in astrobiology and space exploration.