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Soil mineralogy and chemistry on Mars: Possible clues from salts and clays in SNC meteorites
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“All subgroups of the shergottites, nakhlites, and chassignites contain traces of salts, including carbonates and sulfates, that have been interpreted as minerals precipitated from water [Gooding, 1992] to precipitate minerals in tiny fractures [ Warren, 1998].”
From A chemical model for evaporites on early Mars: Possible sedimentary tracers of the early climate and implications for exploration (1999) · cites this paper as Gooding, 1992
Citations
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McKay, D. S., Gibson, E. K., Thomas-Keprta, K. L., Vali, H., Romanek, C. S., Clemett, S. J., Chillier, X. D. F., Maechling, C. R., & Zare, R. N. (1996) · Science · doi:10.1126/science.273.5277.924 · Cited by 1,883
What we have learned about Mars from SNC meteorites
McSween, H. Y. (1994) · Meteoritics · doi:10.1111/j.1945-5100.1994.tb01092.x · Cited by 519
Marchant, D. R., & Head, J. W., III (2007) · Icarus · doi:10.1016/j.icarus.2007.06.018 · Cited by 419
“…processes, such as the introduction of salts in the form of Mg and Ca sulfates and chlorides, by leaching or addition of volcanic gases, might account for the measurements (e.g., Toulmin et al., 1977; Clark and Baird, 1979; Settle, 1979; Clark and Van Hart, 1981; Clark et al., 1982; Gooding, 1992).”
Spectroscopic Identification of Carbonate Minerals in the Martian Dust
Bandfield, J. L., Glotch, T. D., & Christensen, P. R. (2003) · Science · doi:10.1126/science.1088054 · Cited by 385
Mineralogy of meteorite groups
Rubin, A. (1997) · Meteoritics and Planetary Science · doi:10.1111/j.1945-5100.1997.tb01262.x · Cited by 368
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Bell, J. F., III, McSWEEN, H. Y., Jr., Crisp, J. A., Morris, R. V., Murchie, S. L., Bridges, N. T., Johnson, J. R., Britt, D. T., Golombek, M. P., Moore, H. J., et al. (2000) · Journal of Geophysical Research Atmospheres · doi:10.1029/1999je001060 · Cited by 350
Morris, R., Golden, D., Bell, J., Shelfer, T., Scheinost, A. C., Hinman, N., Furniss, G., Mertzman, S., Bishop, J., Ming, D., et al. (2000) · Journal of Geophysical Research Atmospheres · doi:10.1029/1999je001059 · Cited by 323
Thomas-Keprta, K., Bazylinski, D., Kirschvink, J., Clemett, S., Mckay, D., Wentworth, S., Vali, H., Gibson, E. K., & Romanek, C. (2000) · Geochimica et Cosmochimica Acta · doi:10.1016/s0016-7037(00)00481-6 · Cited by 285
“We use these criteria to evaluate the origins of magnetites extracted from ALH84001 carbonate globules.”
BackgroundMethodHave olivine, will gas: Serpentinization and the abiogenic production of methane on Mars
Oze, C., & Sharma, M. (2005) · Geophysical Research Letters · doi:10.1029/2005gl022691 · Cited by 300
“nH2O) [Gooding, 1992]; the latter contains anomalous (17)O and is likely produced from low-T aqueous alteration of sulfides [Thiemens et al.”
BackgroundJarosite as an indicator of water-limited chemical weathering on Mars
Madden, M. E. E., Bodnar, R. J., & Rimstidt, J. D. (2004) · Nature · doi:10.1038/nature02971 · Cited by 295
“The occurrence of sulphate alteration phases in martian meteorite”
BackgroundWater alteration of rocks and soils on Mars at the Spirit rover site in Gusev crater
HASKIN, L. A., Wang, A., Jolliff, B. L., McSWEEN, H. Y., Jr., Clark, B. C., Marais, D. J. D., McLennan, S. M., Tosca, N. J., Hurowitz, J. A., Farmer, J. D., et al. (2005) · Nature · doi:10.1038/nature03640 · Cited by 266
McSWEEN, H. Y., Jr., Murchie, S. L., Crisp, J. A., Bridges, N. T., Anderson, R. C., Bell, J. F., III, Britt, D. T., Brückner, J., DREIBUS, G., Economou, T. E., et al. (1999) · Journal of Geophysical Research Atmospheres · doi:10.1029/98je02551 · Cited by 248
Acid‐sulfate weathering of synthetic Martian basalt: The acid fog model revisited
Tosca, N. J., McLennan, S. M., LINDSLEY, D. H., & Schoonen, M. A. A. (2004) · Journal of Geophysical Research Atmospheres · doi:10.1029/2003je002218 · Cited by 257
The SNC meteorites are from Mars
Treiman, A., Gleason, J., & Bogard, D. (2000) · Planetary and Space Science · doi:10.1016/s0032-0633(00)00105-7 · Cited by 185
Kounaves, S. P., Carrier, B. L., O’Neil, G. D., Stroble, S. T., & Claire, M. W. (2013) · Icarus · doi:10.1016/j.icarus.2013.11.012 · Cited by 193
Rates and mechanisms of chemical weathering of ferromagnesian silicate minerals on Mars
Burns, R. G. (1993) · Geochimica et Cosmochimica Acta · doi:10.1016/0016-7037(93)90182-v · Cited by 185
McKay, C. P. (1997) · PubMed · Cited by 178
Acidic volatiles and the Mars soil
Banin, A., Han, F. X., Kan, I., & Cicelsky, A. (1997) · Journal of Geophysical Research Atmospheres · doi:10.1029/97je01160 · Cited by 177
Hydrogen isotope geochemistry of SNC meteorites
Leshin, L. A., Epstein, S., & Stolper, E. M. (1996) · Geochimica et Cosmochimica Acta · doi:10.1016/0016-7037(96)00122-6 · Cited by 170
A petrographic history of martian meteorite ALH84001: Two shocks and an ancient age
Treiman, A. H. (1995) · Meteoritics · doi:10.1111/j.1945-5100.1995.tb01127.x · Cited by 156
“In addition, ALH84001 contains preterrestrial alteration materials of magnesite-siderite-ankerite carbonates and pyrite, an assemblage not identified in other martian meteorites (Gooding, 1992).”
Ehlmann, B. L., Mustard, J. F., Clark, R. N., Swayze, G. A., & Murchie, S. L. (2011) · Clays and Clay Minerals · doi:10.1346/ccmn.2011.0590402 · Cited by 155
Catling, D. C. (1999) · Journal of Geophysical Research: Planets · doi:10.1029/1998je001020 · Cited by 148
Final chemical results from the Mars Pathfinder alpha proton X‐ray spectrometer
Foley, C. N., Economou, T., & Clayton, R. N. (2003) · Journal of Geophysical Research: Planets · doi:10.1029/2002je002019 · Cited by 148
McKay, C. P. (1997) · Origins of Life and Evolution of Biospheres · doi:10.1023/a:1006500116990 · Cited by 209
“The S, N, and C meteorites are relatively young, having formed on Mars between orig749.tex; 10/06/1997; 16:49; v.7; p.13 200 and 1300 Myr ago (e.g. Gooding, 1992).”
BackgroundGeochemical Consequences of Widespread Clay Mineral Formation in Mars’ Ancient Crust
Ehlmann, B. L., Berger, G., Mangold, N., Michalski, J. R., Catling, D. C., Ruff, S. W., Chassefière, É., Niles, P. B., Chevrier, V. F., & Poulet, F. (2012) · Space Science Reviews · doi:10.1007/s11214-012-9930-0 · Cited by 154
“Fe-poor, Al-rich illite clay minerals may also be present in EETA79001 (Gooding 1992), a shergottite meteorite with a crystallization age typically accepted as 173 Myr (Nyquist et al.”
InfluentialQuantifying absolute water content of minerals using near‐infrared reflectance spectroscopy
Milliken, R. E., & Mustard, J. F. (2005) · Journal of Geophysical Research Atmospheres · doi:10.1029/2005je002534 · Cited by 148
“…Emission Spectrometer (TES) observations [Kuzmin et al., 2004], the presence of hydrated minerals in the SNC meteorites [Bridges et al., 2001; Gooding, 1992], H+ abundance as measured by the Mars Odyssey GRS instruments [Boynton et al., 2002; Feldman et al., 2002; Mitrofanov et al., 2002],…”
MethodMeteoritic minerals and their origins
Rubin, A. E., & Ma, C. (2017) · Geochemistry · doi:10.1016/j.chemer.2017.01.005 · Cited by 139
Magnetofossils from Ancient Mars: a Robust Biosignature in the Martian Meteorite ALH84001
Thomas-Keprta, K., Clemett, S., Bazylinski, D., Kirschvink, J., Mckay, D., Wentworth, S., Vali, H., Gibson, E., & Romanek, C. (2002) · Applied and Environmental Microbiology · doi:10.1128/aem.68.8.3663-3672.2002 · Cited by 116
“The nearsurface environment on the ice fields of Antarctica is oxidizing, and nearly all Antarctic meteorites show evidence of rust on their outer surfaces (29).”
BackgroundThe Origin of Life in the Solar System: Current Issues
Chyba, C. F., & McDonald, G. D. (1995) · Annual Review of Earth and Planetary Sciences · doi:10.1146/annurev.ea.23.050195.001243 · Cited by 132
Halococcus dombrowskii sp. nov., an archaeal isolate from a Permian alpine salt deposit.
Stan‐Lotter, H., Dornmayr‐Pfaffenhuemer, M., Legat, A., Busse, H., Radax, C., & Gruber, C. (2002) · INTERNATIONAL JOURNAL OF SYSTEMATIC AND EVOLUTIONARY MICROBIOLOGY · doi:10.1099/00207713-52-5-1807 · Cited by 131
“may be interesting candidates to be considered when targeting the search for extraterrestrial forms of life, particularly since halite has been detected in outer space (Gooding, 1992; McCord et al., 1998; Zolensky et al., 1999; Whitby et al., 2000).”
BackgroundSources of nutrients and energy for a deep biosphere on Mars
Fisk, M., & Giovannoni, S. (1999) · Journal of Geophysical Research Atmospheres · doi:10.1029/1999je900010 · Cited by 139
Extremely halophilic archaea and the issue of long-term microbial survival
Fendrihan, S., Legat, A., Dornmayr‐Pfaffenhuemer, M., Gruber, C., Weidler, G. W., Gerbl, F. W., & Stan‐Lotter, H. (2006) · Reviews in Environmental Science and Bio/Technology · doi:10.1007/s11157-006-0007-y · Cited by 127
“Evidence for halite was found in the SNC meteorites (Gooding 1992); their Martian origin has been confirmed independently by several groups (Treiman et al. 2000; Rieder et al. 2004).”
BackgroundBecker, L., GLAVIN, D. P., & Bada, J. L. (1997) · Geochimica et Cosmochimica Acta · doi:10.1016/s0016-7037(96)00400-0 · Cited by 125
Paleomagnetic Evidence of a Low-Temperature Origin of Carbonate in the Martian Meteorite ALH84001
Kirschvink, J., Maine, A., & Vali, H. (1997) · Science · doi:10.1126/science.275.5306.1629 · Cited by 125
Dyar, M. D., Tucker, J., Humphries, S. D., Clegg, S. M., Wiens, R. C., & Lane, M. D. (2010) · Spectrochimica Acta Part B Atomic Spectroscopy · doi:10.1016/j.sab.2010.11.016 · Cited by 129
Multiple emission angle surface–atmosphere separations of thermal emission spectrometer data
Bandfield, J. L., & Smith, M. D. (2003) · Icarus · doi:10.1016/s0019-1035(02)00025-8 · Cited by 119
“Toulmin et al. (1977), Gooding (1992), and Bell et al. (2000), have attempted to recast the elemental abundances in terms of normative mineralogy.”
Hagerty, J. J., & NEWSOM, H. E. (2003) · Meteoritics and Planetary Science · doi:10.1111/j.1945-5100.2003.tb00272.x · Cited by 113
“Baird et al. (1976, 1977), Toulmin et al. (1977), and Gooding (1992) found that the composition of the Viking soils could be matched with multicomponent models including hydrous alteration phases, such as smectites.”
BackgroundGeochemical components in Martian soil
Clark, B. C. (1993) · Geochimica et Cosmochimica Acta · doi:10.1016/0016-7037(93)90183-w · Cited by 110
Geological and geochemical legacy of a cold early Mars
Gaidos, E. J., & Marion, G. M. (2003) · Journal of Geophysical Research Atmospheres · doi:10.1029/2002je002000 · Cited by 101
“Moreover, the secondary minerals appear to post-date crystallization of the igneous parent rock by several hundreds Myr, including an Amazonian age of 680 Myr in the Lafayette meteorite [Gooding, 1992; Bridges and Grady, 2000; Bridges et al., 2001].”
BackgroundMagnetic Properties Experiments on the Mars Pathfinder Lander: Preliminary Results
Hviid, S. F., Madsen, M. B., Gunnlaugsson, H. P., Goetz, W., Knudsen, J. M., Hargraves, R. B., Smith, P., Britt, D., Dinesen, A. R., Mogensen, C. T., et al. (1997) · Science · doi:10.1126/science.278.5344.1768 · Cited by 113
Determining the modal mineralogy of Martian soils
McSWEEN, H. Y., Jr., McGlynn, I. O., & Rogers, A. D. (2010) · Journal of Geophysical Research Atmospheres · doi:10.1029/2010je003582 · Cited by 97
“[23] Both models indicate that igneous minerals dominate the soils at each site (Figure 2). Previous soil mineralogy estimates prior to the MER mission [Baird et al., 1976; Gooding, 1992; Bell et al., 2000], based on the assumption that soils were extensively chemically altered, are clearly incorrect.”
BackgroundMethodInfluentialEdwards, H. G. M., Villar, S. E. J., Parnell, J., Cockell, C. S., & Lee, P. (2005) · The Analyst · doi:10.1039/b503533c · Cited by 95
Modeling aqueous ferrous iron chemistry at low temperatures with application to Mars
Marion, G. M., Catling, D. C., & Kargel, J. S. (2003) · Geochimica et Cosmochimica Acta · doi:10.1016/s0016-7037(03)00372-7 · Cited by 95
“This may account for the minor amounts of carbonate found on the surface of Mars (Blaney and McCord, 1989; Pollack et al., 1990; Gooding, 1992; Calvin et al., 1994; Griffith and Shock, 1995; Christensen et al., 1998, 2000b).”
BackgroundResultInfluentialWentworth, S. J., & Gooding, J. L. (1994) · Meteoritics · doi:10.1111/j.1945-5100.1994.tb01100.x · Cited by 93
Self-citationNew Composite Spectra of Mars, 0.4–5.7 μm
Érard, S., & Calvin, W. M. (1997) · Icarus · doi:10.1006/icar.1997.5830 · Cited by 91
“In the range of possible temperatures, all spectra present Banin and Margulies 1983), and with SNC analyses (e.g., Gooding 1992).”
MethodOxygen Isotopic Constraints on the Genesis of Carbonates from Martian Meteorite ALH84001
Leshin, L. A., McKeegan, K. D., Carpenter, P. K., & Harvey, R. P. (1998) · Geochimica et Cosmochimica Acta · doi:10.1016/s0016-7037(97)00331-1 · Cited by 103
McAdam, A. C., Franz, H. B., Sutter, B., Archer, P. D., Freissinet, C., Eigenbrode, J. L., Ming, D. W., Atreya, S. K., Bish, D. L., Blake, D. F., et al. (2014) · Journal of Geophysical Research Planets · doi:10.1002/2013je004518 · Cited by 86
Mineralogy of Martian atmospheric dust inferred from thermal infrared spectra of aerosols
Hamilton, V. E., McSWEEN, H. Y., Jr., & Hapke, B. W. (2005) · Journal of Geophysical Research Atmospheres · doi:10.1029/2005je002501 · Cited by 85
“Sulfates in soils on Mars have been predicted, based on thermodynamic stability considerations [Clark and Van Hart, 1981; Catling, 1999] and their occurrence as alteration products in Martian meteorites [ Gooding, 1992 ].”
BackgroundMethodInfluentialElectrically conducting, Ca‐rich brines, rather than water, expected in the Martian subsurface
Burt, D. M., & Knauth, L. P. (2003) · Journal of Geophysical Research Atmospheres · doi:10.1029/2002je001862 · Cited by 81
Thick and thin models of the evolution of carbon dioxide on Mars
MANNING, C., McKay, C. P., & Zahnle, K. J. (2005) · Icarus · doi:10.1016/j.icarus.2005.08.014 · Cited by 78
Horneck, G. (1995) · Planetary and Space Science · doi:10.1016/0032-0633(94)00190-3 · Cited by 78
Wang, A., Korotev, R. L., Jolliff, B. L., HASKIN, L. A., Crumpler, L. S., Farrand, W. H., Herkenhoff, K. E., Júnior, P. A. D. S., Kusack, A., Hurowitz, J. A., et al. (2006) · Journal of Geophysical Research Atmospheres · doi:10.1029/2005je002516 · Cited by 76
On Water Detection in the Martian Subsurface Using Sounding Radar
Heggy, E. (2001) · Icarus · doi:10.1006/icar.2001.6717 · Cited by 76
“Mineralogical analysis shows that all subgroups of the SNC contain traces of water-precipitated minerals such as smectite, illite and gypsum, with a minor amount of halite, calcite and hematite ( Gooding, 1992 ).”
BackgroundFendrihan, S., Bérces, A., Lammer, H., Musso, M. E., Rontó, G., Polacsek, T. K., Holzinger, A., Kolb, C., & Stan‐Lotter, H. (2009) · Astrobiology · doi:10.1089/ast.2007.0234 · Cited by 75
“Halite has been detected in meteorites, some of which stem from Mars (Gooding, 1992; Zolensky et al., 1999; Treiman et al., 2000).”
Implications from sulfur isotopes of the Nakhla meteorite for the origin of sulfate on Mars
Farquhar, J. D., Kim, S., & Masterson, A. L. (2007) · Earth and Planetary Science Letters · doi:10.1016/j.epsl.2007.08.006 · Cited by 75
Mechanisms for incorporation of hydrogen in and on terrestrial planetary surfaces
Dyar, M. D., Hibbitts, C. A., & Orlando, T. M. (2010) · Icarus · doi:10.1016/j.icarus.2010.02.014 · Cited by 73
Mid-infrared (5–100 μm) reflectance spectra and optical constants of ten phyllosilicate minerals
Glotch, T. D., Rossman, G. R., & Aharonson, O. (2007) · Icarus · doi:10.1016/j.icarus.2007.07.002 · Cited by 69
“…et al. (1993) identified iddingsite (a mixture of ferrihydrite and smectite clay) in the Lafayette meteorite, while Gooding and Meunow (1986), Gooding et al. (1991), and Gooding (1992) discussed the possible identification of illite/smectite mixed layer clays in the EETA79001 and Nahkla meteorites.”
BackgroundThermal Infrared Emission Spectroscopy of Salt Minerals Predicted for Mars
Lane, M. D., & Christensen, P. R. (1998) · Icarus · doi:10.1006/icar.1998.5998 · Cited by 67
Report of the COSPAR mars special regions colloquium
Kminek, G., Rummel, J. D., Cockell, C. S., Atlas, R. M., Barlow, N. G., Beaty, D., Boynton, W. V., Carr, M. H., Clifford, S. M., Conley, C. A., et al. (2010) · Advances in Space Research · doi:10.1016/j.asr.2010.04.039 · Cited by 65
“(Gooding, 1992) and crater ages on volcanic surfaces as young as a few million years (Neukum et al.”
BackgroundBarbieri, R., Stivaletta, N., Marinangeli, L., & Ori, G. G. (2006) · Planetary and Space Science · doi:10.1016/j.pss.2006.04.003 · Cited by 65
“Evaporite minerals have also been recognized in extraterrestrial material, such as in carbonaceous chondrites (Gooding, 1999; Zolensky et al., 1999; Keller et al., 2001).”
BackgroundHydrothermal Systems on Mars: An Assessment of Present Evidence
Farmer, J. D. (2007) · Novartis Foundation symposium · doi:10.1002/9780470514986.ch15 · Cited by 65
Heggy, E., Clifford, S. M., Grimm, R. E., Dinwiddie, C. L., Wyrick, D. Y., & Hill, B. E. (2006) · Journal of Geophysical Research Atmospheres · doi:10.1029/2005je002589 · Cited by 63
Sutter, B., Boynton, W. V., Ming, D. W., Niles, P. B., Morris, R. V., Golden, D. C., Lauer, H. V., Fellows, C., Hamara, D., & Mertzman, S. A. (2011) · Icarus · doi:10.1016/j.icarus.2011.12.002 · Cited by 64
Fendrihan, S., Musso, M. E., & Stan‐Lotter, H. (2009) · Journal of Raman Spectroscopy · doi:10.1002/jrs.2357 · Cited by 63
Swindle, T. D., Grier, J. A., & Burkland, M. K. (1995) · Geochimica et Cosmochimica Acta · doi:10.1016/0016-7037(94)00359-t · Cited by 63
On the thickness of the oxidized layer of the Martian regolith
Zent, A. P. (1998) · Journal of Geophysical Research Atmospheres · doi:10.1029/98je01895 · Cited by 60
Can drying and re-wetting of magnesium sulfate salts lead to damage of stone?
Balboni, E., Espinosa-Marzal, R. M., Doehne, E., & Scherer, G. W. (2010) · Environmental Earth Sciences · doi:10.1007/s12665-010-0774-1 · Cited by 59
“sulfate is also commonly related to weathering processes on Earth (Evans 1969) and on Mars (Gooding 1992; Clark and Van Hart 1981).”
BackgroundThiemens, M. H., Savarino, J., Farquhar, J. D., & Bao, H. (2001) · Accounts of Chemical Research · doi:10.1021/ar960224f · Cited by 56
Mossbauer parameters of iron in phosphate minerals: Implications for interpretation of martian data
Dyar, M. D., Jawin, E. R., Breves, E. A., Marchand, G., Nelms, M., Lane, M. D., Mertzman, S. A., Bish, D. L., & Bishop, J. L. (2014) · American Mineralogist · doi:10.2138/am.2014.4701 · Cited by 55
“The phosphates in the martian meteorites are generally thought to be primary, late crystallization, igneous minerals, with few exceptions (Gooding and Wentworth 1991; Mojzsis and Arrhenius 1998).”
BackgroundAqueous Alteration in Martian Meteorites
Velbel, M. A. (2012) · SEPM (Society for Sedimentary Geology) eBooks · doi:10.2110/pec.12.102.0097 · Cited by 54
Water soluble ions in the Nakhla martian meteorite
Sawyer, D. J., McGehee, M. D., Canepa, J., & Moore, C. (2000) · Meteoritics and Planetary Science · doi:10.1111/j.1945-5100.2000.tb01458.x · Cited by 56
Harner, P. L., & Gilmore, M. S. (2014) · Icarus · doi:10.1016/j.icarus.2014.11.037 · Cited by 52
Preston, L. J., Benedix, G. K., GENGE, M. J., & Sephton, M. A. (2008) · Icarus · doi:10.1016/j.icarus.2008.08.006 · Cited by 49
“Hydrous mineral assemblages (Gooding, 1992), the D/H ratios of water extracted from SNC meteorites (Watson et al.”
BackgroundS ≠ NC: Multiple source areas for Martian meteorites
Treiman, A. H. (1995) · Journal of Geophysical Research Atmospheres · doi:10.1029/94je02184 · Cited by 48
Laboratory simulations of Mars aqueous geochemistry
Bullock, M. A., Moore, J. M., & Mellon, M. T. (2004) · Icarus · doi:10.1016/j.icarus.2004.03.016 · Cited by 46
“However, salt minerals and clays have been observe rectly in SNCs, and are thought to be due to either hydrot mal processes or to weathering(Gooding, 1992).”
BackgroundOxygenic photosynthesis and the oxidation state of Mars
Hartman, H., & McKay, C. P. (1995) · Planetary and Space Science · doi:10.1016/0032-0633(94)00223-e · Cited by 47
“These meteorites date back from 200 to 1300 million years suggesting oxidizing conditions on the near surface of Mars at least that long ago (Gooding, 1992).”
BackgroundAnderson, S., & Grimm, R. E. (1998) · Journal of Geophysical Research Atmospheres · doi:10.1029/98je00740 · Cited by 47
Rubin, A. E., & Ma, C. (2021) · Cambridge University Press eBooks · doi:10.1017/9781108613767 · Cited by 46
Evidence of honeycomb weathering on Mars
Rodriguez-Navarro, C. M. (1998) · Geophysical Research Letters · doi:10.1029/98gl02569 · Cited by 44
Oxygen isotopic record of silicate alteration in the Shergotty—Nakhla—Chassigny meteorite Lafayette
Romanek, C. S., Perry, E. C., Treiman, A. H., Socki, R. A., JONES, J. H., & Gibson, E. K. (1998) · Meteoritics and Planetary Science · doi:10.1111/j.1945-5100.1998.tb01683.x · Cited by 45
Resolution of Lava Tubes With Ground Penetrating Radar: The TubeX Project
Esmaeili, S., Kruse, S., Jazayeri, S., Whelley, P., Bell, E., Richardson, J. A., Garry, W. B., & Young, K. E. (2020) · Journal of Geophysical Research Planets · doi:10.1029/2019je006138 · Cited by 44
“…characteristics of lunar or Martian soil include, for example, temperature, UV exposure, triboelectric effects due to local dust storms, and the probable presence of evaporites and clays in the Martian soil (Gooding, 1992; Heggy et al., 2006; Olhoeft, 1991; Stillman & Olhoeft, 2005).”
BackgroundAstrobiology with haloarchaea from Permo-Triassic rock salt
Stan‐Lotter, H., Radax, C., Gruber, C., Legat, A., Pfaffenhuemer, M., Wieland, H., Leuko, S., Weidler, G. W., Kömle, N. I., & Kargl, G. (2002) · International Journal of Astrobiology · doi:10.1017/s1473550403001307 · Cited by 44
“Halite has been detected in meteorites, some of which stem from Mars (Gooding 1992; Treiman et al. 2000); in addition, a salty ocean is thought to exist under the surface ice cover of the Jovian moon Europa (McCord et al. 1998).”
BackgroundTrace element geochemistry of Martian iddingsite in the Lafayette meteorite
Treiman, A. H., & Lindstrom, D. J. (1997) · Journal of Geophysical Research Atmospheres · doi:10.1029/96je03884 · Cited by 44
Origin of carbonate‐magnetite‐sulfide assemblages in Martian meteorite ALH84001
Scott, E. R. D. (1999) · Journal of Geophysical Research: Planets · doi:10.1029/1998je900034 · Cited by 44
TREIMAN, A. H., & ROMANEK, C. S. (1998) · Meteoritics & Planetary Science · doi:10.1111/j.1945-5100.1998.tb01679.x · Cited by 47
Sulfate Minerals: A Problem for the Detection of Organic Compounds on Mars?
Lewis, J. M. T., Watson, J. S., Najorka, J., Luong, D., & Sephton, M. A. (2015) · Astrobiology · doi:10.1089/ast.2014.1160 · Cited by 42
“Oxidized sulfur species are widespread in martian meteorites, with calcium and magnesium sulfates being the most common forms (Burgess et al., 1989; Gooding, 1992).”
BackgroundSeckbach, J., & Walsh, M. M. (2008) · Cellular origin and life in extreme habitats · doi:10.1007/978-1-4020-8837-7 · Cited by 42
Chatzitheodoridis, E., Haigh, S. J., & Lyon, I. C. (2014) · Astrobiology · doi:10.1089/ast.2013.1069 · Cited by 41
“The palagonitization of basaltic glass is considered to be a viable process on Mars (Toulmin et al., 1977; Allen et al., 1981; Gooding, 1992).”
BackgroundExobiological implications of potential sedimentary deposits on Mars
Komatsu, G., & Ori, G. (2000) · Planetary and Space Science · doi:10.1016/s0032-0633(00)00078-7 · Cited by 45
Macey, M. C., Fox‐Powell, M. G., Ramkissoon, N. K., Stephens, B. P., Barton, T., Schwenzer, S. P., Pearson, V. K., Cousins, C. R., & Olsson‐Francis, K. (2020) · Scientific Reports · doi:10.1038/s41598-020-67815-8 · Cited by 39
Kunte, H., Trüper, H. G., & Stan‐Lotter, H. (2002) · Springer eBooks · doi:10.1007/978-3-642-59381-9_13 · Cited by 39
The Mars oxidant experiment (MOx) for Mars '96.
McKay, C. P., Grunthaner, F., Lane, A., Herring, M., Bartman, R., Ksendzov, A., Manning, C., Lamb, J. L., Williams, R., Ricco, A., et al. (1998) · Planetary and Space Science · doi:10.1016/s0032-0633(98)00011-7 · Cited by 42
Phosphates and carbon on Mars: Exobiological implications and sample return considerations
Mojzsis, S., & Arrhenius, G. (1998) · Journal of Geophysical Research Atmospheres · doi:10.1029/98je02141 · Cited by 33
Cabane, M., Coll, P., Szopa, C., Israël, G., Raulin, F., Sternberg, R., Mahaffy, P. R., Person, A., Rodier, C. G., Navarro-González, R., et al. (2004) · Advances in Space Research · doi:10.1016/s0273-1177(03)00523-4 · Cited by 38
“Carbonates, as observed in the SNC-Martian meteorites (Gooding, 1992), have not been fully confirmed at the surface of Mars, nevertheless some observations (Pollack et al.”
BackgroundRemote Detection of Phyllosilicates on Mars and Implications for Climate and Habitability
Bishop, J. L. (2018) · Elsevier eBooks · doi:10.1016/b978-0-12-809935-3.00003-7 · Cited by 38
Dyar, M. D., Carmosino, M., Tucker, J., Brown, E., Clegg, S. M., Wiens, R. C., Barefield, J. E., Delaney, J. S., Ashley, G. M., & Driese, S. G. (2011) · Chemical Geology · doi:10.1016/j.chemgeo.2011.11.019 · Cited by 37
“Studies of martian meteorites (e.g., Gooding et al., 1991; Gooding, 1992), MER rover observations, and geochemical calculations (e.”
Mars remote‐sensing analog studies in the Badwater Basin, Death Valley, California
Baldridge, A. M., Farmer, J. D., & Moersch, J. E. (2004) · Journal of Geophysical Research Atmospheres · doi:10.1029/2004je002315 · Cited by 39
“Such models predict the occurrence of carbonates, sulfates, phosphates and chlorides as major components of Martian evaporite assemblages [Baird et al., 1976; Clark et al., 1976; Gooding, 1978, 1992; Clark and Vanhart, 1981; Treiman and Gooding ,1 991;Wentworth and Gooding, 1994; McKay et al., 1996; Lane and Christens…”
BackgroundDetection and monitoring of H 2 O and CO 2 ice clouds on Mars
Bell, J. F., III, Calvin, W. M., Ockert-Bell, M. E., Crisp, D., Pollack, J. B., & Spencer, J. R. (1996) · Journal of Geophysical Research Atmospheres · doi:10.1029/96je00689 · Cited by 38
Stalport, F., Coll, P., Szopa, C., Person, A., Navarro-González, R., Cabane, M., Ausset, P., & Vaulay, M.-J. (2007) · Geophysical Research Letters · doi:10.1029/2007gl031184 · Cited by 33
“, 2003], the analyses of several Martian meteorites pointed to their presence, suggesting they could be of Martian origin [Gooding, 1992; McKay et al., 1996; Bridges et al., 2001], and some geomorphological structures (such as karsts) of the Mars surface could be attributed to carbonate deposits [Bérczi, 2005].”
BackgroundExperimental studies of Mars‐analog brines
Moore, J. M., & Bullock, M. A. (1999) · Journal of Geophysical Research Atmospheres · doi:10.1029/1999je001040 · Cited by 31
“The weight ratio of CO2/SO2 in our pilot experiment was 5.1, which may be compared to the estimates of ;4 for SNC meteorites [Gooding, 1992].”
BackgroundResultInfluential
Metadata
- Authors
- Gooding, J. L.
- Affiliations
- National Aeronautics and Space Administration (US)
- Corresponding author
- Gooding, James L.
- Venue
- Icarus
- Publisher
- Elsevier BV
- Published
- 1992-09
- Volume
- 99
- Issue
- 1
- Pages
- 28-41
- ISSN
- 0019-1035 (ISSN-L)
- OpenAlex
- W2004018625
- Cited by
- 232
- References
- 92
- Citations by year
- 2026: 2 · 2025: 2 · 2024: 2 · 2023: 1 · 2022: 3 · 2021: 25 · 2020: 8 · 2019: 3 · 2018: 6 · 2017: 7 · 2016: 2 · 2015: 4 · 2014: 7 · 2013: 4 · 2012: 8
- FWCI
- 11.20
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Icarus (publishedVersion)
- Funders
- National Aeronautics and Space Administration
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Planetary Science and Exploration
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Earth and Planetary Sciences › Geochemistry and Petrology › Geochemistry and Elemental Analysis
- Keywords
- Martian meteorites, Mars, shergottites, nakhlites, chassignites, aqueous alteration, clay minerals, carbonates, sulfate, halides, ferric oxide, aluminosilicates, scapolite, smectite, illite, gypsum, clay catalysis, Martian dust
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