The DOI matches its Crossref record; 4 of the 4 references it cites were found in a registry or an index.
On the possibility of chemosynthetic ecosystems in subsurface habitats on Mars
Abstract
We have reexamined the question of extant microbial life on Mars in light of the most recent information about the planet and recently discovered nonphotosynthetic microbial ecosystems on Earth--deep sea hydrothermal vent communities and deep subsurface aquifer communities. On Mars, protected subsurface niches associated with hydrothermal activity could have continued to support life even after surface conditions became inhospitable. Geochemical evidence from the SNC meteorites and geomorphological evidence for recent volcanism suggest that such habitats could persist to the present time. There are also extensive geological features that attest to the ubiquitous nature of volcano-ground ice interactions on Mars. We suggest a possible deep subsurface microbial ecology similar to those discovered to depths of several kilometers below the surface of the Earth. We focus on anaerobic systems utilizing CO2 as the primary source of carbon. Liquid water could be provided by the heat of geothermal or volcanic activity melting permafrost or other subsurface water sources. Gases from volcanic activity deep in the planet could provide reducing power (as CH4, H2, or H2S) percolating up from below and enabling the development of a microbial community based upon chemolithoautotrophy. We suggest a methanogen (or acetogen) and sulfur-based microbial ecology as one possible basis for microbial primary production. Our hypothetical ecosystem is neither supported, nor excluded, by current observations of Mars. Tests for such a subsurface system involve locating active geothermal areas associated with ground ice or detecting trace quantities of reduced atmospheric gases that would leak from such a system.
Overview
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
In the citing paper
“Liquid water may be possible in the subsurface of present-day Mars (e.g., Boston et al., 1992; McEwen et al., 2011; Ojha et al., 2015).”
From The Astrobiology Primer v2.0 (2016) · cites this paper as Boston et al., 1992
Citations
Cites
Woese, C. R. (1987) · Microbiological Reviews · doi:10.1128/mr.51.2.221-271.1987 · Cited by 5,042
Pyrite Formation, the First Energy Source for Life: a Hypothesis
Wächtershäuser, G. (1988) · Systematic and Applied Microbiology · doi:10.1016/s0723-2020(88)80001-8 · Cited by 374
Clifford, S. M. (1987) · Journal of Geophysical Research: Solid Earth · doi:10.1029/jb092ib09p09135 · Cited by 160
Duration of liquid water habitats on early Mars
McKay, C. P., & Davis, W. L. (1991) · Icarus · doi:10.1016/0019-1035(91)90102-y · Cited by 151
Self-citation
Research works printed but not linked: 58
- Allen, 1979, Volcano-ice interactions on Mars, J. Geophys. Res., 84, 8048, 10.1029/JB084iB14p08048 · DOI
- Bak, 1987, A novel type of energy metabolism involving fermentation of inorganic sulfur compounds, Nature, 326, 891, 10.1038/326891a0 · DOI
- Bastin, 1926, The presence of sulfate-reducing bacteria in oilfield waters, Science, 63, 21, 10.1126/science.63.1618.21 · DOI
- Broady, 1987, The biota and environment of fumaroles on Mt. Melbourne, Northern Victoria Land, Polar Biol., 7, 97, 10.1007/BF00570447 · DOI
- Clark, 1979, Solar-driven chemical energy source for a Martian biota, Origins Life, 9, 241, 10.1007/BF00932498 · DOI
- Clark, 1976, Results of the Viking X-Ray Fluorescence Experiment, Science, 194, 1283, 10.1126/science.194.4271.1283 · DOI · Paper page
- Clifford, 1991, The role of thermal vapor diffusion in the subsurface hydrologic evolution of Mars, Geophys. Res. Lett., 18, 2055, 10.1029/91GL02469 · DOI
- Clifford, 1983, The stability of ground ice in the equatorial regions of Mars, J. Geophys. Res., 88, 2456, 10.1029/JB088iB03p02456 · DOI
- Coradini, 1979, A thermodynamical study of the Martian permafrost, J. Geophys. Res., 84, 8115, 10.1029/JB084iB14p08115 · DOI
- Daumas, 1986, A bacteriological study of geothermal spring waters dating from the dogger and trias period in the Paris basin, Geomicrobiol. J., 4, 423, 10.1080/01490458609385947 · DOI
- Drobner, 1990, Pyrite formation linked with hydrogen evolution under anaerobic conditions, Nature, 346, 742, 10.1038/346742a0 · DOI
- Fanale, 1974, Exchange of adsorbed H2O and CO2 between the regolith and atmosphere of Mars caused by changes in surface insolation, J. Geophys. Res., 79, 3397, 10.1029/JC079i024p03397 · DOI
- Farmer, 1977, Mars: Water vapor observations from the Viking orbiters, J. Geophys. Res., 82, 4225, 10.1029/JS082i028p04225 · DOI
- Fischer, 1983, Chemolithoautotropic metabolism of anaerobic extremely thermophilic archaebacteria, Nature, 301, 511, 10.1038/301511a0 · DOI
- Friedmann, 1980, Endolithic microbial life in hot and cold deserts, Origins Life, 10, 223, 10.1007/BF00928400 · DOI
- Friedmann, 1972, Endolithic blue-green algae in the dry valleys: Primary producers in the Antarctic cold desert ecosystem, Science, 193, 1247, 10.1126/science.193.4259.1247 · DOI
- Gulick, 1989, Fluvial valleys and Martian paleoclimates, Nature, 341, 514, 10.1038/341514a0 · DOI
- Gulick, 1990, Origin and evolution of valleys on Martian Volcanoes, J. Geophys. Res., 95, 14,325, 10.1029/JB095iB09p14325 · DOI
- Head, 1981, Tectonic evolution of the terrestrial planets, Science, 213, 62, 10.1126/science.213.4503.62 · DOI
- Horowitz, 1977, Viking on Mars: The carbon assimilation experiments, J. Geophys. Res., 82, 4659, 10.1029/JS082i028p04659 · DOI
- Huber, 1990, Hyperthermophilic archaebacteria within the crater and open-sea plume of erupting Macdonald Seamount, Nature, 345, 179, 10.1038/345179a0 · DOI
- Hudson, 1988, Enumeration of thermophilic heterotrophs in geothermally heated soils from Mount Erebus, Ross Island, Antarctica, Appl. Environ. Microbiol., 54, 622, 10.1128/AEM.54.2.622-624.1988 · DOI
- Jackson, 1965, Circulation of water in soil under a temperature gradient, Nature, 205, 314, 10.1038/205314b0 · DOI
- Jones, 1989, Anaerobic metabolic processes in the deep terrestrial subsurface, Geomicrobiol. J., 7, 117, 10.1080/01490458909377854 · DOI
- Kahn, 1985, The evolution of CO2 on Mars, Icarus, 62, 175, 10.1016/0019-1035(85)90116-2 · DOI
- Kelly, 1989, Genus Thiobacillus, Vol. 3, 1842
- Kieffer, 1977, Thermal and albedo mapping of Mars during the Viking primary mission, J. Geophys. Res., 82, 4249, 10.1029/JS082i028p04249 · DOI
- Klein, 1978, The Viking biological experiments on Mars, Icarus, 34, 666, 10.1016/0019-1035(78)90053-2 · DOI
- Klein, 1979, The Viking mission and the search for life on Mars, Rev. Geophys. Space Phys., 17, 1655, 10.1029/RG017i007p01655 · DOI
- Kong, 1977, Photochemistry of the Martian atmosphere, Icarus, 32, 168, 10.1016/0019-1035(77)90058-6 · DOI
- Lake, 1988, Origin of the eukaryotic nucleus determined by rate-invariant analysis of rRNA sequences, Nature, 331, 184, 10.1038/331184a0 · DOI
- Laul, 1986, The Shergotty consortium and SNC meteorites: An overview, Geochim. Cosmochim. Acta, 50, 875, 10.1016/0016-7037(86)90370-4 · DOI
- Levin, 1977, Recent results from the Viking labeled release experiment on Mars, J. Geophys. Res., 82, 4663, 10.1029/JS082i028p04663 · DOI
- Levin, 1981, A search for a nonbiological explanation of the Viking labeled release life detection experiment, Icarus, 45, 494, 10.1016/0019-1035(81)90048-8 · DOI
- Levin, 1988, A reappraisal of life on Mars, Vol. 71, 187
- Levine, 1989, Trace gases in the atmosphere of Mars: An indicator of microbial life, Vol. 75, 277
- Lovely, 1985, Minimum threshold for hydrogen metabolism in methanogenic bacteria, Appl. Environ. Microbiol., 49, 1530, 10.1128/AEM.49.6.1530-1531.1985 · DOI
- Lucchita, 1987, Recent mafic volcanism on Mars, Science, 235, 565, 10.1126/science.235.4788.565 · DOI
- Lucchita, 1990, Young volcanic deposits in the Valles Marineris, Mars?, Icarus, 86, 476, 10.1016/0019-1035(90)90230-7 · DOI
- McKay, 1988, Are there carbonate deposits in Valles Marineris, Mars?, Icarus, 73, 142, 10.1016/0019-1035(88)90088-7 · DOI · Paper page
- McKay, 1989, The early environment and its evolution on Mars: Implications for life, Rev. Geophys., 27, 189, 10.1029/RG027i002p00189 · DOI
- McElroy, 1977, Photochemistry and evolution of Mars' atmosphere: A Viking perspective, J. Geophys. Res., 82, 4379, 10.1029/JS082i028p04379 · DOI
- Mouginis-Mark, 1985, Volcano/ground ice interactions in Elysium Planitia, Mars, Icarus, 64, 265, 10.1016/0019-1035(85)90090-9 · DOI
- Mouginis-Mark, 1990, Recent water release in the Tharsis region of Mars, Icarus, 84, 362, 10.1016/0019-1035(90)90044-A · DOI
- Nedell, 1987, Origin and evolution of the layered deposits in the Valles Marineris, Mars, Icarus, 70, 409, 10.1016/0019-1035(87)90086-8 · DOI
- Olson, 1981, Sulfate-reducing and methanogenic bacteria from deep aquifers in Montana, Geomicrobiol. J., 2, 327, 10.1080/01490458109377772 · DOI
- Oyama, 1977, The Viking gas exchange experiments results from Chryse and Utopia surface samples, J. Geophys. Res., 82, 4669, 10.1029/JS082i028p04669 · DOI
- Phelps, 1989, Methods for recovery of deep terrestrial subsurface sediments for microbiological studies, J. Microbiol. Methods, 7, 267, 10.1016/0167-7012(89)90069-9 · DOI
- Sargent, 1989, Geology and hydrology of the deep subsurface microbiology sampling sites at the Savannah River Plant, South Carolina, Geomicrobiol. J., 7, 3, 10.1080/01490458909377846 · DOI
- Sharp, 1988, Properties of Thermus ruber strains isolated from Icelandic hot springs and DNA: DNA homology of Thermus ruber and Thermus aquaticus, Appl. Environm. Microbiol., 54, 2049, 10.1128/AEM.54.8.2049-2053.1988 · DOI
- Solomon, 1978, On volcanism and thermal tectonics on one-plate planets, Geophys. Res. Lett., 5, 461, 10.1029/GL005i006p00461 · DOI
- Squyres, 1986, Geomorphic evidence for the distribution of ground ice on Mars, Science, 231, 249, 10.1126/science.231.4735.249 · DOI
- Squyres, 1987, Large-scale volcano-ground ice interactions on Mars, Icarus, 70, 385, 10.1016/0019-1035(87)90085-6 · DOI
- Wächtershäuser, 1990, The case for the chemoautotrophic origin of life in an iron-sulfur world, Origin Life Evol. Biosphere, 20, 173, 10.1007/BF01808279 · DOI
- Wilson, 1987, Volcanic input to the atmosphere from Alba Patera on Mars, Nature, 330, 354, 10.1038/330354a0 · DOI
- Zent, 1986, Possible Mars brines: Equilibrium and kinetic considerations, J. Geophys. Res., 91, D439, 10.1029/JB091iB04p0D439 · DOI
- ZoBell, 1947, Microbial transformation of molecular hydrogen in marine sediments, with particular reference to petroleum, Bull. Am. Assn. Petrol. Geol., 31, 1709
- ZoBell, 1958, Ecology of sulfate reducing bacteria, Producers Monthly, 22, 12
Cited by
Sorted by citations
Items 101–200 of 275
On developing thermal cave detection techniques for earth, the moon and mars
Wynne, J. J., Titus, T. N., & Chong, G. (2008) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2008.04.037 · Cited by 48
“These features are considered important for the exploration of life (Mazur et al., 1978; Boston et al., 1992; Klein, 1998; Grin et al., 1998, 2001; Boston et al., 2001) because they offer protection from low surface temperatures, unfiltered ultraviolet radiation (Mazur et al.”
BackgroundEffects of drift-gas polarizability on glycine peptides in ion mobility spectrometry
Beegle, L., Kanik, I., Matz, L. M., & Hill, H. (2002) · doi:10.1016/s1387-3806(02)00626-7 · Cited by 51
The next frontier for planetary and human exploration
Stamenković, V., Beegle, L. W., Zacny, K. A., Arumugam, D. D., Baglioni, P., Barba, N. J., Baross, J. A., Bell, M. S., Bhartia, R., Blank, J. G., et al. (2019) · Nature Astronomy · doi:10.1038/s41550-018-0676-9 · Cited by 54
Self-citationUrey prize lecture: Planetary evolution and the origin of life
McKay, C. P. (1991) · Icarus · doi:10.1016/0019-1035(91)90128-g · Cited by 63
Ion mobility spectrometry in space exploration
Johnson, P. V., Beegle, L. W., Kim, H. I., Eiceman, G. A., & Kanik, I. (2006) · International Journal of Mass Spectrometry · doi:10.1016/j.ijms.2006.11.001 · Cited by 53
Muller, A. W. J. (1995) · Progress in Biophysics and Molecular Biology · doi:10.1016/0079-6107(95)00004-7 · Cited by 48
Templeton, A. S., & Caro, T. A. (2023) · Annual Review of Earth and Planetary Sciences · doi:10.1146/annurev-earth-031920-081957 · Cited by 68
Schulze‐Makuch, D., Dohm, J. M., Fairén, A. G., Baker, V. R., Fink, W., & STROM, R. G. (2005) · Astrobiology · doi:10.1089/ast.2005.5.778 · Cited by 47
“…slope northeast respectively Terra impact equatorial basement bedrock more than approximately 3.6 Ga, possible vast subterranean voids crust (Boston et al. , 1992; Rodriguez hypothesized to exist in the Thar-sis 783 surrounding regions, gives rise to the distinct Mars, but has also been…”
InfluentialYoung volcanic terrains are windows into early microbial colonization
Hadland, N., Hamilton, C. W., & Duhamel, S. (2024) · Communications Earth & Environment · doi:10.1038/s43247-024-01280-3 · Cited by 41
“Lava tubes are of interest to astrobiology because of their stable environmental conditions (e.g., temperature, humidity), lack of harmful UV, entrapment of water, and secondary mineral precipitation, leading to diverse microbial communities and biosignature preservation 114,129 .”
The search for life on Mars: What we learned from Viking
Klein, H. (1998) · Journal of Geophysical Research Atmospheres · doi:10.1029/98je01722 · Cited by 41
A roadmap to cave dwelling on the Moon and Mars
Blamont, J. (2012) · Advances in Space Research · doi:10.1016/j.asr.2014.08.019 · Cited by 40
Kovacik, W. P., Takai, K., Mormile, M. R., McKinley, J. P., Brockman, F. J., Fredrickson, J. K., & Holben, W. E. (2005) · Environmental Microbiology · doi:10.1111/j.1462-2920.2005.00876.x · Cited by 36
“…lack of direct reliance on solar radiation, and the fact that they represent a large percentage of the earth’s biosphere, but also because subsurface environments represent perhaps the most likely location for the origin or persistence of life on other planets (Boston et al ., 1992; Gold, 1992).”
BackgroundA Biosignature Suite from Cave Pool Precipitates, Cottonwood Cave, New Mexico
Melim, L., Liescheidt, R., Northup, D., Spilde, M., Boston, P. J., & Queen, J. (2009) · Astrobiology · doi:10.1089/ast.2009.0345 · Cited by 39
“The subsurface of Mars may reveal some of the only clues to life through preserved biosignatures (Boston et al., 1992).”
Self-citationBeaty, D. W., Clifford, S. M., BORG, L. E., Catling, D. C., Craddock, R. A., Marais, D. J. D., Farmer, J. D., Frey, H. V., Haberle, R. M., McKay, C. P., et al. (2005) · Astrobiology · doi:10.1089/ast.2005.5.663 · Cited by 36
“Of particular relevance for Mars are chemolithoautotrophic forms of life that utilize hydrogen, methane, and sulfur (Boston et al., 1992; Max and Clifford, 2000).”
Evidence for Seismogenic Hydrogen Gas, a Potential Microbial Energy Source on Earth and Mars
McMahon, S., Parnell, J., & Blamey, N. J. F. (2016) · Astrobiology · doi:10.1089/ast.2015.1405 · Cited by 46
“It is widely recognized that the most hospitable environments for life on present-day Mars are likely to occur in the deep subsurface ( e.g. , Boston et al. , 1992; Fisk and Gio-vannoni, 1999; Westall et al. , 2013; Cockell, 2014).”
A First Analysis of Metallome Biosignatures of Hyperthermophilic Archaea
Cameron, V., House, C. H., & Brantley, S. L. (2012) · Archaea · doi:10.1155/2012/789278 · Cited by 38
“…between trace metals and biological processes in modern environments including the biogeo-chemical cycling of metals (e.g., [16, 33–37]), weathering processes (e.g., [38–42]), mineral transformations (e.g., [43– 47]), microbial metabolisms (e.g., [48–54]), and biomarkers (e.g., [55–59]).”
Chastain, B. K., & Kral, T. A. (2010) · Astrobiology · doi:10.1089/ast.2010.0480 · Cited by 17
“…as terrestrial models for possible martian life-forms long before methane was discovered in Mars’ atmosphere, and the actual discovery of their primary metabolic by-product on Mars reinvigorates this hypothesis (Boston et al., 1992; Kral et al., 1998; Weiss et al., 1999; Chapelle et al., 2002).”
Jepsen, S., Priscu, J., Grimm, R., & Bullock, M. (2007) · Astrobiology · doi:10.1089/ast.2007.0124 · Cited by 36
“The possibility of chemoautotrophs exploiting deep subsurface niches on Mars was considered by Boston et al. (1992).”
Pellenbarg, R. E., Max, M. D., & Clifford, S. M. (2003) · Journal of Geophysical Research Atmospheres · doi:10.1029/2002je001901 · Cited by 38
“the Martian surface and near subsurface (see also Boston, et al., 1992 ).”
BackgroundGeomicrobiology of Caves: A Review
Northup, K. H. L. D. E. (2001) · Geomicrobiology Journal · doi:10.1080/01490450152467750 · Cited by 35
“This article reviews work on microbial activities in caves that can be applied to the recognition of biomarkers for subsurface life on other planets (Boston, Ivanov, and McKay 1992; Boston 2000; Boston et al. 2001; Cunningham et al. 1995; McKay, Ivanov, and Boston 1994).”
BackgroundFactoring Origin of Life Hypotheses into the Search for Life in the Solar System and Beyond
Longo, A., & Damer, B. (2020) · Life · doi:10.3390/life10050052 · Cited by 38
Schirmack, J., Böhm, M., Brauer, C., Löhmannsröben, H.-G., de Vera, J. D., Möhlmann, D., & Wagner, D. (2014) · Planetary and Space Science · doi:10.1016/j.pss.2013.08.019 · Cited by 34
“For this reason several scientific publications have previously dealt with methanogenic archaea as model organisms for possible life on Mars (Boston et al., 1992, Jakosky et al., 2003, Kral et al., 2004, 2011; Krasnopolsky et al., 2004; Morozova et al., 2007; Morozova and Wagner 2007; Ulrich et…”
BackgroundBoston, P., Hose, L., Northup, D., & Spilde, M. (2006) · Geological Society of America eBooks · doi:10.1130/2006.2404(28 · Cited by 34
Self-citationShallow transient liquid water environments on present-day mars, and their implications for life
Jones, E. (2018) · Acta Astronautica · doi:10.1016/j.actaastro.2018.02.027 · Cited by 33
Mickol, R. L., & Kral, T. A. (2016) · Origins of Life and Evolution of Biospheres · doi:10.1007/s11084-016-9519-9 · Cited by 28
Impact Excavation and the Search for Subsurface Life on Mars
Cockell, C., & Barlow, N. (2002) · Icarus · doi:10.1006/icar.2001.6725 · Cited by 33
Relevance of Earth-Bound Extremophiles in the Search for Extraterrestrial Life
Carré, L., Zaccaı̈, G., Delfosse, X., Girard, É., & Franzetti, B. (2022) · Astrobiology · doi:10.1089/ast.2021.0033 · Cited by 38
“The possibility of a present or past deep martian bio-sphere in subsurface brines, based on chemosynthesis and analogous to terrestrial subsurface ecosystems, has been widely hypothesized (Boston et al. , 1992; Michalski et al. , 2013; Grotzinger et al. , 2014; Mikucki et al. , 2015).”
InfluentialThaler, A. D., & Amon, D. J. (2019) · PeerJ · doi:10.7717/peerj.7397 · Cited by 38
Kimble, J. C., Winter, A. S., Spilde, M., Sinsabaugh, R., & Northup, D. (2018) · FEMS Microbiology Ecology · doi:10.1093/femsec/fiy173 · Cited by 30
The search for life beyond Earth through fuzzy expert systems
Furfaro, R., Dohm, J., Fink, W., Kargel, J., Schulze-Makuch, D., Fairén, A., Palmero-Rodriguez, A. J., Baker, V., Ferré, P., Hare, T., et al. (2008) · Planetary and Space Science · doi:10.1016/j.pss.2007.09.006 · Cited by 30
Martin, Y. E., & Johnson, E. A. (2012) · Progress in Physical Geography Earth and Environment · doi:10.1177/0309133312457107 · Cited by 45
“This is a unique category as it considers the earliest time periods in the Earth’s history (e.g. Bada et al., 1994; Kasting et al., 1993; Schopf, 1983), and it also focuses on life outside Earth in the rest of the Universe (with a large focus on the planet Mars) (Bell, 1996; Boston et al., 1992; Carr, 1996; Clark, 199…”
BackgroundThe Geology and Habitability of Terrestrial Planets: Fundamental Requirements for Life
Southam, G., Rothschild, L. J., & Westall, F. (2007) · Space Science Reviews · doi:10.1007/s11214-007-9148-8 · Cited by 23
Borruso, L., Sannino, C., Selbmann, L., Battistel, D., Zucconi, L., Azzaro, M., Turchetti, B., Buzzini, P., & Guglielmin, M. (2018) · Scientific Reports · doi:10.1038/s41598-018-25079-3 · Cited by 31
Circumstellar habitable zones for deep terrestrial biospheres
McMahon, S., O’Malley-James, J. T., & Parnell, J. (2013) · Planetary and Space Science · doi:10.1016/j.pss.2013.07.002 · Cited by 32
“…our own solar system, however, some of the most promising candidates for habitable extraterrestrial environments are in the subsurface of planets and moons outside the conventional HZ, such as Mars and Jupiter’s moon Europa (e.g. Boston et al., 1992; Fisk and Giovannoni, 1999; Gaidos et al., 1999).”
BackgroundThe Potential for Biologically Catalyzed Anaerobic Methane Oxidation on Ancient Mars
Marlow, J. J., LaRowe, D. E., Ehlmann, B. L., Amend, J. P., & Orphan, V. J. (2014) · Astrobiology · doi:10.1089/ast.2013.1078 · Cited by 20
“Based on assumed martian geochemical conditions, several microbial metabolisms have been proposed, including iron or manganese reduction or oxidation, methanogenesis, acetogenesis, and sulfur-processing pathways (Boston et al., 1992; Varnes et al., 2004).”
Zero-valent iron on Mars: An alternative energy source for methanogens
Chastain, B. K., & Kral, T. A. (2010) · Icarus · doi:10.1016/j.icarus.2010.02.024 · Cited by 23
Understanding Microbially Active Biogeochemical Environments
Gleeson, D. B., McDermott, F. P., & Clipson, N. (2007) · Advances in applied microbiology · doi:10.1016/s0065-2164(07)62004-8 · Cited by 26
Kral, T. A., Birch, W., Lavender, L. E., & Virden, B. T. (2014) · Planetary and Space Science · doi:10.1016/j.pss.2014.07.008 · Cited by 26
Amils, R., Escudero, C., Oggerin, M., Puente‐Sánchez, F., Arce‐Rodríguez, A., Fernández‐Remolar, D. C., Rodríguez, N., García‐Villadangos, M., Sanz, J. L., Briones, C., et al. (2022) · Environmental Microbiology · doi:10.1111/1462-2920.16291 · Cited by 43
Bonaccorsi, R., & Stoker, C. (2008) · Astrobiology · doi:10.1089/ast.2007.0152 · Cited by 26
“from those that might be expected on Mars, i.e. , subsurface chemolithoautotrophs ( e.g. , Boston et al. , 1992).”
Templeton, A. S., Ellison, E. T., Glombitza, C., Morono, Y., Rempfert, K. R., Hoehler, T. M., Zeigler, S. D., Kraus, E., Spear, J. R., Nothaft, D. B., et al. (2021) · Journal of Geophysical Research Biogeosciences · doi:10.1029/2021jg006315 · Cited by 68
“Sulfate is also expected to be an important oxidant in extraterrestrial systems where peridotite/water interactions and H2 generation may occur, such as in subsurface aquifers on Mars (Boston et al., 1992; Clifford et al., 2010; Marlow et al., 2014; Michalski et al., 2013; Tarnas et al., 2018), and within the ocean of…”
BackgroundInfluentialHabitability of Mars: How Welcoming Are the Surface and Subsurface to Life on the Red Planet?
Sielaff, A. C., & Smith, S. A. (2019) · Geosciences · doi:10.3390/geosciences9090361 · Cited by 29
“Apart from escaping these challenging environmental conditions on the surface, the subsurface physicochemical characteristics are favorable for harboring present chemolithoautotrophic life [83] through the use of inorganic compounds for the production of metabolic energy, as has been shown in Earth’s deep biosphere [8…”
BackgroundHigh Tolerance of Hydrogenothermus marinus to Sodium Perchlorate
Beblo‐Vranesevic, K., Huber, H., & Rettberg, P. (2017) · Frontiers in Microbiology · doi:10.3389/fmicb.2017.01369 · Cited by 28
“In subsurface of Mars pressure and temperature increases with depth and thereby the probability of liquid, additionally radiation protected, water reservoirs (such as subsurface aquifers) rises, too (Boston et al., 1992; Dartnell et al., 2007).”
BackgroundFluid Inclusion Studies of Chemosynthetic Carbonates: Strategy for Seeking Life on Mars
Parnell, J., Mazzini, A., & Honghan, C. (2002) · Astrobiology · doi:10.1089/153110702753621330 · Cited by 22
“Since subsurface existence would preclude photosynthesis, chemosynthesis would likely be the preferred metabolic strategy for a biota in such an environment (Rothschild, 1990; Boston et al ., 1992).”
Cockell, C. S., Holt, J. W., Campbell, J., Groseman, H., Josset, J. L., Bontognali, T. R. R., Phelps, A., Hakobyan, L., Kuretn, L., Beattie, A., et al. (2018) · International Journal of Astrobiology · doi:10.1017/s1473550418000186 · Cited by 26
“On Mars, the deep subsurface is recognized to be a location that may have hosted habitable conditions in its past and has a high possibility of hosting such conditions today (Boston et al. , 1992; Hofmann, 2008).”
Melim, L., Northup, D., Boston, P., & Spilde, M. (2016) · Palaios · doi:10.2110/palo.2015.033 · Cited by 24
“…earth-like subsurface environments are interesting targets in the search for life on Mars or icy moons around gas giants because they could provide refuge from harsh surface conditions including desiccation and ionizing radiation (Boston et al. 1992, 2001; Westall et al. 2000; Boston 2010).”
BackgroundSelf-citationPrime candidate sites for astrobiological exploration through the hydrogeological history of Mars
Fairén, A., Dohm, J., Uceda, E. R., Rodriguez, A., Baker, V., Fernández-Remolar, D., Schulze-Makuch, D., & Amils, R. (2005) · Planetary and Space Science · doi:10.1016/j.pss.2005.06.007 · Cited by 24
“A continual source of energy for their metabolism possibly was the diffusion of H2 and CO downward into the regolith (Boston et al., 1992; Weiss et al., 2000), readily produced in the atmosphere by the photochemical breakup of H2O and CO2, respectively.”
BackgroundSinha, N., Nepal, S., Kral, T. A., & Kumar, P. (2016) · Planetary and Space Science · doi:10.1016/j.pss.2016.11.012 · Cited by 30
Studies of Antibiotic Production by Cave Bacteria
Montaño, E. T., & Henderson, L. (2013) · doi:10.1007/978-1-4614-5206-5_6 · Cited by 23
Telling, J. P., Voglesonger, K. M., Sutcliffe, C. N., Lacrampe‐Couloume, G., Edwards, E. A., & Lollar, B. S. (2017) · Geomicrobiology Journal · doi:10.1080/01490451.2017.1333176 · Cited by 23
“Our study at the Thompson Mine suggests that hydrogenotrophic microorganisms are unlikely to be present in similar highly saline brines in the subsurface of Mars unless they base their osmotic regulation around the accumulation of inorganic (e.g., KC) rather than organic osmolytes (Figure 7).”
BackgroundInfluentialSignificance to Astrobiology of Micro-Organisms in Permafrost and Ice
Hoover, R., & Gilichinsky, D. (2001) · doi:10.1007/978-94-010-0684-2_38 · Cited by 22
A New Frontier for Palaeobiology: Earth's Vast Deep Biosphere
McMahon, S., & Ivarsson, M. (2019) · Bioessays · doi:10.1002/bies.201900052 · Cited by 20
Advancing the search for extra-terrestrial genomes
Carr, C. E., Mojarro, A., Tani, J., Bhattaru, S. A., Zuber, M. T., Doebler, R. W., Brown, M. J., Herrington, K., Talbot, R., Fuller, C. W., et al. (2016) · IEEE Aerospace Conference (AERO) · doi:10.1109/aero.2016.7500859 · Cited by 21
“A reasonable place to search for extant Martian life would be in the subsurface of once habitable locations [39, 40].”
BackgroundThe habitability of vesicles in martian basalt
McMahon, S., Parnell, J., Ponicka, J., Hole, M., & Boyce, A. (2013) · Astronomy & Geophysics · doi:10.1093/astrogeo/ats035 · Cited by 20
Peer Reviewed: Detecting Amino Acids on Mars
Bada, J., & Mcdonald, G. (1996) · Analytical Chemistry · doi:10.1021/ac9621231 · Cited by 20
Fungal Spores Viability on the International Space Station
Gomoiu, I., Chatzitheodoridis, E., Vadrucci, S., Walther, I., & Cojoc, R. (2016) · Origins of Life and Evolution of Biospheres · doi:10.1007/s11084-016-9502-5 · Cited by 19
“2008), in which microbial communities possibly could have been found inhabiting niche environments in subsurface rocks (Chatzitheodoridis et al. 2014; Marschall et al. 2012; Boston et al. 1992).”
BackgroundFu, Q., Socki, R. A., & Niles, P. B. (2015) · Geochimica et Cosmochimica Acta · doi:10.1016/j.gca.2015.01.027 · Cited by 21
Eos Chasma, Mars: Regional setting for a potential landing site for astrobiology
Greeley, R., Kuzmin, R. O., Nelson, D. M., & Farmer, J. D. (2003) · Journal of Geophysical Research Atmospheres · doi:10.1029/2002je002014 · Cited by 8
Mars as a time machine to Precambrian Earth
Lapôtre, M. G. A., Bishop, J. L., Ielpi, A., Lowe, D. R., Siebach, K. L., Sleep, N. H., & Tikoo-Schantz, S. M. (2022) · Journal of the Geological Society · doi:10.1144/jgs2022-047 · Cited by 18
“…(e.g. Gault et al. 1968; Osinski et al. 2020), creating new spaces within fracture networks that are shielded from UV and cosmic radiation (e.g. Boston et al. 1992; Osinski et al. 2020), and giving way to conditions conducive to hydrothermal circulation (e.g. Abramov and Kring 2005; Kirsimäe…”
BackgroundPreston, L., Melim, L., Polyak, V., Asmerom, Y., & Southam, G. (2014) · Geomicrobiology Journal · doi:10.1080/01490451.2014.913096 · Cited by 17
“This data will be added to the development of a biosignature suite (Boston et al. 1992, 2001) to identify microbial involvement in carbonate precipitation on the earth and elsewhere.”
MethodCan rapid loss and high variability of Martian methane be explained by surface H2O2?
Gough, R. V., Turley, J., Ferrell, G. R., Cordova, K. E., Wood, S. E., DeHaan, D. O., McKay, C. P., Toon, O. B., & Tolbert, M. A. (2010) · Planetary and Space Science · doi:10.1016/j.pss.2010.09.018 · Cited by 19
Geology, Life, and Habitability
Southam, G., Westall, F., & Spohn, T. (2015) · Elsevier eBooks · doi:10.1016/b978-0-444-53802-4.00175-5 · Cited by 21
Astrobiological Benefits of Human Space Exploration
Crawford, I. A. (2010) · Astrobiology · doi:10.1089/ast.2010.0476 · Cited by 16
“The harsh conditions of the martian surface have led many to suggest that, if life does exist on Mars today, it is most likely to be found below the surface ( e.g., Boston et al., 1992).”
Goodwin, A., & Papineau, D. (2021) · Astrobiology · doi:10.1089/ast.2021.0010 · Cited by 17
“There is significant evidence for past liquid water preserved in the martian geological record (Boston et al. , 1992), and it has been hypothesized that microbial mats could have thrived on a wet martian surface * 3.8–3.1 Ga (Ellery et al. , 2004).”
InfluentialRichardson, C. D., Hinman, N. W., McHenry, L. J., Kotler, J. M., Knipe, D., & Scott, J. R. (2012) · Planetary and Space Science · doi:10.1016/j.pss.2012.02.002 · Cited by 17
Hydrogen symbioses in evolution and disease
Williams, A. C., & Ramsden, D. B. (2007) · QJM · doi:10.1093/qjmed/hcm045 · Cited by 14
A Mobile Robot System for Remote Measurements of Ammonia Vapor in the Atmosphere
Anderson, G., Sheesley, C., Tolson, J., Wilson, E., & Tunstel, E. (2006) · IEEE International Conference on Systems, Man and Cybernetics · doi:10.1109/icsmc.2006.384389 · Cited by 16
An Overview Of The Origin Of Life: The Case For Biological Prospecting On Mars
Hiscox, J. A. (1999) · Earth Moon and Planets · doi:10.1023/a:1013143024842 · Cited by 17
“Extant (living organisms) such as chemolithotrophs might still be located below the martian surface, provided liquid water was stable (Boston et al., 1992).”
BackgroundStable carbon isotope fractionation by methanogens growing on different Mars regolith analogs
Sinha, N., & Kral, T. A. (2015) · Planetary and Space Science · doi:10.1016/j.pss.2015.04.011 · Cited by 15
Pontefract, A., Osinski, G. R., Lindgren, P., Parnell, J., Cockell, C. S., & Southam, G. (2012) · doi:10.1111/maps.12004 · Cited by 15
Mars Atmospheric Oxidant Sensor (MAOS): An In-Situ Heterogeneous Chemistry Analysis
Zent, A., Quinn, R., Grunthaner, F., Hecht, M., Buehler, M., Mckay, C., & Ricco, A. (2002) · Planetary and Space Science · doi:10.1016/s0032-0633(02)00204-0 · Cited by 15
Nagy, B., Kovács, J., Ignéczi, Á., Beleznai, S., Mari, L., Keresztúri, Á., & Szalai, Z. (2020) · Astrobiology · doi:10.1089/ast.2018.2021 · Cited by 16
“…evolution and melting of the permafrost in the vicinity of the Ojos del Salado could provide insights into the potential habitability of such dry regions with shallow sub-surface ice occurrence (Boston et al. , 1992; Gilichinsky, 2011; Dogamal-Goldmann et al. , 2016; Kereszturi and Noack, 2016).”
Barometric Pumping Through Fractured Rock: A Mechanism for Venting Deep Methane to Mars' Atmosphere
Ortiz, J., Rajaram, H., Stauffer, P., Harp, D., Wiens, R., & Lewis, K. (2022) · Geophysical Research Letters · doi:10.1029/2022gl098946 · Cited by 13
Mars-Analog Calcium Sulfate Veins Record Evidence of Ancient Subsurface Life
McMahon, S., Parnell, J., & Philippe, R. (2020) · Astrobiology · doi:10.1089/ast.2019.2172 · Cited by 15
“…in Earth’s deep biosphere and its fossil record have inspired widespread speculation that life on Mars could also have colonized the subsurface, perhaps surviving there for billions of years after the surface became inhospitable ( e.g., Boston et al., 1992; Fisk and Giovannoni 1999; Cockell, 2014).”
Melchiorre, E. B., Bottrill, R. S., Huss, G. R., & Lopez, A. M. (2016) · Geochimica et Cosmochimica Acta · doi:10.1016/j.gca.2016.10.020 · Cited by 12
French, J. E., & Blake, D. (2016) · International Journal of Geophysics · doi:10.1155/2016/2410573 · Cited by 13
“Accordingly, a flurry of recent studies have focussed on understanding terrestrial examples of life-harbouring extreme environments/ paleoenvironments that could have analogs on Mars, including evaporite deposits [7], thermal spring deposits [8], Antarctic paleolake deposits [9], deep sea hydrothermal vent systems and…”
BackgroundMartellato, E., Foing, B., & Benkhoff, J. (2013) · doi:10.1016/j.pss.2013.06.010 · Cited by 13
Marcano, V., Benítez, P., & Palacios‐Prü, E. (2002) · Planetary and Space Science · doi:10.1016/s0032-0633(02)00069-7 · Cited by 15
Stinnesbeck, W., Frey, E. D., Zell, P., Olguín, J. A., Hering, F., Frank, N., Arps, J., Geenen, A., Gescher, J., Isenbeck‐Schröter, M., et al. (2017) · Palaeogeography Palaeoclimatology Palaeoecology · doi:10.1016/j.palaeo.2017.10.012 · Cited by 17
Hydrocarbon System Analysis for Methane Hydrate Exploration on Mars
Max, M., Clifford, S., & Johnson, A. H. (2013) · American Association of Petroleum Geologists eBooks · doi:10.1306/13361573m1013546 · Cited by 13
The Habitability of Mars: Past and Present
McCollom, T. M. (2006) · Springer eBooks · doi:10.1007/3-540-37683-6_6 · Cited by 11
Chen, P. (2015) · Journal of Astrobiology & Outreach · doi:10.4172/2332-2519.1000125 · Cited by 6
“Some methanogens are able to utilize inorganic compounds (H2 and CO2) as their only source of energy through the following methane-generating redox reaction [4,22]:”
BackgroundMicrobial life detection with minimal assumptions
Kounaves, S., Noll, R. A., Buehler, M., Hecht, M., Lankford, K., & West, S. (2002) · SPIE Optics + Photonics · doi:10.1117/12.454772 · Cited by 12
“Even though such constraints may have limited the ecological and evolutionary niches where life may have developed and still flourish, there have been numerous attempts at defining these niches, their chemistry, and the possible martian life-forms that may inhabit them.(13-20)”
BackgroundSite selection for Mars exobiology
Farmer, J. D., Marais, D. D., Greeley, R., Landheim, R., & Klein, H. (1995) · Advances in Space Research · doi:10.1016/s0273-1177(99)80078-7 · Cited by 12
Life in Earth’s Lava Caves: Implications for Life Detection on Other Planets
Northup, D. E., Hathaway, J. J. M., Snider, J. R., Balasch, M. M., Garcia, M. G., Dapkevicius, M. D. L. E., Gabriel, C. R., Stone, F. D., Spilde, M., & Boston, P. J. (2012) · Cellular origin and life in extreme habitats · doi:10.1007/978-94-007-4966-5_26 · Cited by 8
Self-citationSubsurface Geomicrobiology of the Iberian Pyritic Belt
the MARTE Team, Amils, R., Fernández‐Remolar, D. C., Gómez, F., González‐Toril, E., Rodríguez, N., Briones, C., Prieto‐Ballesteros, O., Sanz, J. L., Díaz, E., et al. (2007) · Soil biology · doi:10.1007/978-3-540-74231-9_10 · Cited by 15
“Subsurface ecosystems are also intriguing exobiological models , useful for the re-creation of life on early Earth (Widdel et al. 1993) or the representation of life as it would occur in other planetary bodies ( Boston et al. 1992 ).”
BackgroundVolcanic Features of New Mexico Analogous to Volcanic Features on Mars
Crumpler, L., Aubele, J., & Zimbelman, J. (2007) · Cambridge University Press eBooks · doi:10.1017/cbo9780511536014.005 · Cited by 12
Potential for Liquid Water Biochemistry Deep under the Surfaces of the Moon, Mars, and beyond
Lingam, M., & Loeb, A. (2020) · Astrophysical Journal · doi:10.3847/2041-8213/abb608 · Cited by 11
“Hence, it is not surprising that a number of studies have inves- Corresponding author: Manasvi Lingam mlingam@fit.edu tigated Martian subsurface habitability (Boston et al. 1992; Cockell 2014; Michalski et al. 2018; Sholes et al. 2019; Carrier et al. 2020).”
BackgroundThe Characterization of Biosignatures in Caves Using an Instrument Suite
Uckert, K., Chanover, N. J., Getty, S., Voelz, D., Brinckerhoff, W. B., McMillan, N. J., Xiao, X., Boston, P. J., Li, X., McAdam, A. C., et al. (2017) · Astrobiology · doi:10.1089/ast.2016.1568 · Cited by 14
“…offered by the terrestrial subsurface could have been exploited by primitive microorganisms early on in the history of life on Earth, and at present, these same subsurface attributes provide habitable environments for a vast variety of microorganisms (Kaiser and Bollag, 1990; Boston et al., 1992).”
Self-citationCave Geomicrobiology in India: Status and Prospects
Baskar, S., Baskar, R., Tewari, V. C., Thorseth, I., Øvreås, L., Lee, N. M., & Routh, J. (2011) · Cellular origin and life in extreme habitats · doi:10.1007/978-94-007-0397-1_24 · Cited by 11
Planetary protection issues and the future exploration of Mars
Devincenzi, D. (1992) · doi:10.1016/0273-1177(92)90165-t · Cited by 11
Large‐scale fluid‐deposited mineralization in Margaritifer Terra, Mars
Thomas, R. J., Potter‐McIntyre, S. L., & Hynek, B. M. (2017) · Geophysical Research Letters · doi:10.1002/2017gl073388 · Cited by 11
“…on Mars comes from a zone that is shielded from inhospitable surface conditions, retains porosity, is minimally altered, and features the elemental nutrients and redox reactions necessary for metabolically available energy [Boston et al., 1992; Michalski et al., 2013; Parnell and McMahon, 2016].”
BackgroundMcKay, C. P., Mykytczuk, N., & Whyte, L. G. (2014) · ASM Press eBooks · doi:10.1128/9781555817183.ch14 · Cited by 8
Potential Habitability of Present-Day Martian Subsurface for Earth-Like Methanogens
Butturini, A., Benaiges-Fernández, R., Fors, O., & García‐Castellanos, D. (2025) · Astrobiology · doi:10.1089/ast.2024.0100 · Cited by 9
“Based on this, the methanogenic hydrogenotrophs have emerged as a candidate “ model organism ” for studying survival on Mars (Boston et al., 1992; Kral et al., 2010; Mickol et al., 2014) because they feed on simple inorganic molecules ( i.e. , H 2 and CO 2 ) that are expected to be available on the…”
Strategies for Deploying a Sensor Network to Explore Planetary Lava Tubes
Kalita, H., & Thangavelautham, J. (2021) · Italian National Conference on Sensors · doi:10.3390/s21186203 · Cited by 9
“Here, living organisms could have been sheltered from dangerous ultraviolet radiation, while volcanic minerals might have provided a rich source of nutrients for chemosynthesis (similar to living colonies near Earth-based volcanic vents) [18].”
BackgroundPaleo-Critical Zones, windows into the changing life and landscapes during the Quaternary Period
Ashley, G. M. (2020) · Quaternary Research · doi:10.1017/qua.2020.49 · Cited by 8
“If Mars was ever habitable (Boston et al., 1992), Martian PCZ’s are more likely to reveal the transition from proto-CZ (abiotic) to biotic CZ than on Earth (Fig.”
BackgroundTelling, J. P., Lacrampe‐Couloume, G., & Lollar, B. S. (2013) · Astrobiology · doi:10.1089/ast.2012.0915 · Cited by 9
“…insight into the chemistry of organic synthesis before life evolved on Earth and define parameters for the search for life on future exobiology missions (Boston et al., 1992; McCollom, 1999; Fortes, 2000; Formisano et al., 2004; Krasnopolsky et al., 2004; Sleep et al., 2004; Niemann et al., 2005).”
Lavoie, K. H., Northup, D. E., & Barton, H. A. (2010) · Science Publishers eBooks · doi:10.1201/b10193-2 · Cited by 10
Chanda, P., Amenábar, M. J., Boyd, E. S., Beard, B. L., & Johnson, C. M. (2020) · Geochimica et Cosmochimica Acta · doi:10.1016/j.gca.2020.09.025 · Cited by 10
Hard rock dark biosphere and habitability
Escudero, C., & Amils, R. (2023) · Frontiers in Astronomy and Space Sciences · doi:10.3389/fspas.2023.1203845 · Cited by 10
Metadata
- Authors
- Boston, P. J., Ivanov, M. V., & P. McKay, C.
- Affiliations
- Academy of Sciences of the Soviet Union (RU)
- Venue
- Icarus
- Publisher
- Elsevier BV
- Published
- 1992-02
- Volume
- 95
- Issue
- 2
- Pages
- 300-308
- ISSN
- 0019-1035 (ISSN-L)
- OpenAlex
- W2039172699
- Cited by
- 325
- References
- 0
- Citations by year
- 2026: 6 · 2025: 7 · 2024: 6 · 2023: 6 · 2022: 8 · 2021: 6 · 2020: 11 · 2019: 10 · 2018: 11 · 2017: 15 · 2016: 15 · 2015: 9 · 2014: 11 · 2013: 10 · 2012: 12
- FWCI
- 5.27
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Icarus (publishedVersion)
- PubMed (publishedVersion)
- Funders
- National Aeronautics and Space Administration
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Planetary Science and Exploration
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Keywords
- chemosynthetic ecosystems, subsurface microbial life, Mars, hydrothermal activity, Martian meteorites, permafrost, geothermal activity, chemolithoautotrophy, methanogenic archaea, acetogenic bacteria, hydrothermal vent communities
- MeSH terms
- Carbon Dioxide, Environmental Microbiology, Extraterrestrial Environment, Geology, Temperature, Solar System, Ecosystem, Mars, Exobiology, Volcanic Eruptions, Geological Phenomena
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review