The origin of organic matter in the Martian meteorite ALH84001
Abstract
Stable carbon isotope measurements of the organic matter associated with the carbonate globules and the bulk matrix material in the ALH84001 Martian meteorite indicate that two distinct sources are present in the sample. The delta 13C values for the organic matter associated with the carbonate globules averaged -26% and is attributed to terrestrial contamination. In contrast, the delta 13C values for the organic matter associated with the bulk matrix material yielded a value of -15%. The only common sources of carbon on the Earth that yield similar delta 13C values, other then some diagenetically altered marine carbonates, are C4 plants. A delta 13C value of -15%, on the other hand, is consistent with a kerogen-like component, the most ubiquitous form of organic matter found in carbonaceous chondrites such as the Murchison meteorite. Examination of the carbonate globules and bulk matrix material using laser desorption mass spectrometry (LDMS) indicates the presence of a high molecular weight organic component which appears to be extraterrestrial in origin, possibly derived from the exogenous delivery, of meteoritic or cometary debris to the surface of Mars.
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Indigenous MMC, which may include PAHs, has been found within ALH 84001.
“Indigenous MMC, which may include PAHs, has been found within ALH 84001 (Becker et al. 1999;Clemett et al. 1998;Jull et al. 1998;McKay et al. 1996).”
From Comprehensive imaging and Raman spectroscopy of carbonate globules from Martian meteorite ALH 84001 and a terrestrial analogue from Svalbard (2007) · cites this paper as Becker et al. 1999
Becker et al. (1999) demonstrated the presence of MMC in the matrix of ALH 84001.
“Becker et al. (1999) demonstrated the presence of MMC in the matrix of ALH 84001.”
From Comprehensive imaging and Raman spectroscopy of carbonate globules from Martian meteorite ALH 84001 and a terrestrial analogue from Svalbard (2007) · cites this paper as Becker et al. 1999
A significant portion of the organic carbon in ALH 84001 probably exists as a macromolecular phase.
“Therefore, a significant portion of the organic carbon in ALH 84001 probably exists as a macromolecular phase”
From Comprehensive imaging and Raman spectroscopy of carbonate globules from Martian meteorite ALH 84001 and a terrestrial analogue from Svalbard (2007) · cites this paper as Becker et al. 1999
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References 26 · Cited by 68
- Authors
- Becker, L., Popp, B., Rust, T., & Bada, J. L.
- Affiliations
- University of Hawaiʻi at Mānoa (US)
- Scripps Institution of Oceanography (US)
- Corresponding author
- Becker, Luann
- Venue
- Earth and Planetary Science Letters
- Publisher
- Elsevier BV
- Published
- 1999-03
- Volume
- 167
- Issue
- 1-2
- Pages
- 71-79
- ISSN
- 0012-821X (ISSN-L)
- OpenAlex
- W2125419520
- Cited by
- 68
- References
- 26
- Citations by year
- 2026: 2 · 2025: 1 · 2024: 2 · 2023: 1 · 2022: 1 · 2021: 1 · 2018: 3 · 2016: 4 · 2015: 2 · 2014: 1 · 2013: 3 · 2012: 8
- FWCI
- 3.27
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Earth and Planetary Science Letters (publishedVersion)
- PubMed (publishedVersion)
- Funders
- National Science Foundation
- Smithsonian Institution
- Johnson Space Center
- 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 › Earth and Planetary Sciences › Paleontology › Paleontology and Stratigraphy of Fossils
- Keywords
- ALH84001, Martian meteorites, organic matter, stable carbon isotopes, terrestrial contamination, carbonate globules, kerogen, C4 plants, carbonaceous chondrites, extraterrestrial organic matter, Mars
- MeSH terms
- Antarctic Regions, Carbon Isotopes, Carbonates, Extraterrestrial Environment, Lasers, Polycyclic Aromatic Hydrocarbons, Mass Spectrometry, Mars, Exobiology, Meteoroids
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