Cited by 1,883Planetary Science and ExplorationAstro and Planetary ScienceSpace Science and Extraterrestrial Life

Search for Past Life on Mars: Possible Relic Biogenic Activity in Martian Meteorite ALH84001

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McKay, David S., Gibson, Everett K., Thomas-Keprta, Kathie L., Vali, Hojatollah, Romanek, Christopher S., Clemett, Simon J., Chillier, Xavier D. F., Maechling, Claude R. +1 more·1996·Science

Abstract

Fresh fracture surfaces of the martian meteorite ALH84001 contain abundant polycyclic aromatic hydrocarbons (PAHs). These fresh fracture surfaces also display carbonate globules. Contamination studies suggest that the PAHs are indigenous to the meteorite. High-resolution scanning and transmission electron microscopy study of surface textures and internal structures of selected carbonate globules show that the globules contain fine-grained, secondary phases of single-domain magnetite and Fe-sulfides. The carbonate globules are similar in texture and size to some terrestrial bacterially induced carbonate precipitates. Although inorganic formation is possible, formation of the globules by biogenic processes could explain many of the observed features, including the PAHs. The PAHs, the carbonate globules, and their associated secondary mineral phases and textures could thus be fossil remains of a past martian biota.

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Crossref · 10.1126/science.273.5277.924

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  • Most ALH 84001 globules had only a single magnetite rim, whereas some contained a white magnesite zone between two outer rims of magnetite.

    “Whereas some globules contained a white magnesite zone between two outer rims of magnetite-as identified from previous observations (McKay et al. 1996) and during Raman mapping-most had only a single magnetite rim”
  • Hematite may not have been detected previously in ALH 84001 globules because the primary analytical tools were optical and electron microscopy and elemental mapping, with the mineralogy of the carbonate composition being inferred from assessments based on the amounts of Fe, Ca, Mg, Mn, C, and O present.

    “Hematite may not have been detected previously in ALH 84001 globules because the primary analytical tools were optical and electron microscopy and elemental mapping (electron microprobe, energy dispersive X-ray analysis), with the mineralogy of the carbonate composition being inferred from assessments based on the amounts of Fe, Ca, Mg, Mn, C, and O present (McKay et al. 1996;Mittlefehldt 1994aM”
  • Two types of carbonate globules have previously been described in ALH 84001: dark brown globules containing a single magnetite rim, and lighter orange-colored globules with a second magnetite outer rim bounded by an area of magnesite.

    “Two types of carbonate globules (Fig. 1) have previously been described in ALH 84001: dark brown globules containing a single magnetite rim, and lighter orange-colored globules with a second magnetite outer rim bounded by an area of magnesite (e.g., Figs.1a and 1d) (McKay et al. 1996;Treiman et al. 2003).”
  • Iron- and magnesium-rich carbonate globules (with calcium-rich areas) are the host minerals of the microscopic structures in question within the meteorite ALH84001.

    “Particular interest has focused on the ability to identify carbonate minerals on Mars' surface because iron- and magnesium-rich carbonate globules (with calcium-rich areas) are the host minerals of the microscopic structures in question within the meteorite.”

    From Thermal infrared emission spectroscopy of anhydrous carbonates (1997) · cites this paper as McKay et al., 1996

  • Carbonate has been identified in the Martian meteorite ALH84001.

    “Not only has carbonate been identified in the Martian meteorite ALH84001 [McKay et al., 1996]”

    From Thermal infrared emission spectroscopy of anhydrous carbonates (1997) · cites this paper as McKay et al., 1996

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References 61 · Cited by 1,883

Authors
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.
Affiliations
  • National Aeronautics and Space Administration (US)
  • Johnson Space Center (US)
  • Lockheed Martin (United States) (US)
  • McGill University (CA)
  • University of Georgia (US)
  • Stanford University (US)
Venue
Science
Published
1996-08-16
Volume
273
Issue
5277
Pages
924-930
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W1968713120
Cited by
1,883
References
61
Citations by year
2026: 34 · 2025: 35 · 2024: 37 · 2023: 51 · 2022: 45 · 2021: 78 · 2020: 48 · 2019: 70 · 2018: 91 · 2017: 33 · 2016: 45 · 2015: 46 · 2014: 43 · 2013: 56 · 2012: 68
FWCI
95.99
Type
journal article
Language
en
Open access
Licence
cc-by
Locations
  • Science (publishedVersion)
  • PubMed (publishedVersion)
  • Archive ouverte UNIGE (University of Geneva) (submittedVersion, cc-by)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Planetary Science and Exploration
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astro and Planetary Science
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Space Science and Extraterrestrial Life
Keywords
ALH84001, Martian meteorites, polycyclic aromatic hydrocarbons, carbonate globules, magnetite, iron sulfide, bacterial carbonate precipitation, fracture morphology
MeSH terms
Antarctic Regions, Bacteria, Carbonates, Extraterrestrial Environment, Ferrous Compounds, Fossils, Hydrogen-Ion Concentration, Iron, Microscopy, Electron, Microscopy, Electron, Scanning, Oxides, Polycyclic Aromatic Hydrocarbons, Mars, Exobiology, Meteoroids, Ferrosoferric Oxide

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