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Isotopic Evidence for a Terrestrial Source of Organic Compounds Found in Martian Meteorites Allan Hills 84001 and Elephant Moraine 79001
Abstract
Stepped-heating experiments on martian meteorites Allan Hills 84001 (ALH84001) and Elephant Moraine 79001 (EETA79001) revealed low-temperature (200 to 430 degrees Celsius) fractions with a carbon isotopic composition delta13C between -22 and -33 per mil and a carbon-14 content that is 40 to 60 percent of that of modern terrestrial carbon, consistent with a terrestrial origin for most of the organic material. Intermediate-temperature (400 to 600 degrees Celsius) carbonate-rich fractions of ALH84001 have delta13C of +32 to +40 per mil with a low carbon-14 content, consistent with an extraterrestrial origin, whereas some of the carbonate fraction of EETA79001 is terrestrial. In addition, ALH84001 contains a small preterrestrial carbon component of unknown origin that combusts at intermediate temperatures. This component is likely a residual acid-insoluble carbonate or a more refractory organic phase.
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“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 Jull et al. 1998
In the citing paper
“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 Jull et al. 1998
Citations
Cites
Search for Past Life on Mars: Possible Relic Biogenic Activity in Martian Meteorite ALH84001
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
A Search for Endogenous Amino Acids in Martian Meteorite ALH84001
Bada, J. L., Glavin, D. P., McDonald, G. D., & Becker, L. (1998) · Science · doi:10.1126/science.279.5349.362 · Cited by 179
Calcium carbonate and sulfate of possible extraterrestrial origin in the EETA 79001 meteorite
Gooding, J. L., Wentworth, S. J., & Zolensky, M. E. (1988) · Geochimica et Cosmochimica Acta · doi:10.1016/0016-7037(88)90361-4 · Cited by 149
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- A negligible amount of 14 C could have been produced by spallation reactions in the organic components of these meteorites. The amount produced by spallation would not produce a significant 14 C/ 12 C ratio. No appreciable 14 C should have been produced while in space in the organic phases through the action of cosmic-ray–generated secondary thermal neutrons on 14 N or through thermal neutron capture on 13 C. The reason is that secondary cosmic-ray neutrons can only become thermalized inside a large parent meteoroid or in a smaller body with significant water content. Given that all of the martian meteorites so far recovered were irradiated as small objects in space with little water content very few cosmic-ray–generated neutrons can have been thermalized. M. S. Spergel et al. [ Proc. Lunar Planet. Sci. Conf. 16 J. Geophys. Res. 91 483 (1986)] have shown that for objects of pre-atmospheric radius less than ∼50 g/cm 2 (or approximately 19 kg in mass) that the cosmic-ray–induced thermal neutron flux is extremely small and neutron products are not detectable. ALH84001 and EETA79001 were much smaller than this size (recovered masses of 2.1 and 7.9 kg respectively) and thus the thermal neutron flux would be even lower and we can rule out any significant thermal neutron production of 14 C in the organic components of these martian meteorites. Consequently organic material indigenous to ALH84001 or EETA79001 would be expected to have very low 14 C abundance resulting from irradiation in space.
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Cited by
Sorted by citations
Ages and Geologic Histories of Martian Meteorites
Nyquist, L., Bogard, D., Shih, C., Greshake, A., Stöffler, D., & Eugster, O. (2001) · Space sciences series of ISSI · doi:10.1007/978-94-017-1035-0_5 · Cited by 693
“The high concentrations of PAHs, present in all textural units of ALH84001 (Stephan et al., 1998, 1999), could also be due to terrestrial contamination (Becker et al., 1997; Jull et al., 1998).”
BackgroundThe Sample Analysis at Mars Investigation and Instrument Suite
Mahaffy, P. R., Webster, C. R., Cabane, M., Conrad, P. G., Coll, P., Atreya, S. K., Arvey, R., Barciniak, M., Benna, M., Bleacher, L. V., et al. (2012) · Space Science Reviews · doi:10.1007/s11214-012-9879-z · Cited by 596
“Measurements of the 13C/12C ratio in organic macromolecular material in martian meteorites (Jull et al. 1998a, 1998b; Grady et al. 2004) overlap with ranges common of terrestrial biogenic carbon and certainly no single carbon isotope signature can establish biogenicity.”
BackgroundGlavin, D., Freissinet, C., Miller, K., Eigenbrode, J., Brunner, A., Buch, A., Sutter, B., Archer, P. D., Atreya, S., Brinckerhoff, W., et al. (2013) · Journal of Geophysical Research Planets · doi:10.1002/jgre.20144 · Cited by 448
A Reduced Organic Carbon Component in Martian Basalts
Steele, A., Mccubbin, F. M., Fries, M. D., Kater, L., Boctor, N. Z., Fogel, M. L., Conrad, P. G., Glamoclija, M., Spencer, M. K., Morrow, A. L., et al. (2012) · Science · doi:10.1126/science.1220715 · Cited by 251
Self-citationEhrenfreund, P., & Charnley, S. B. (2000) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.38.1.427 · Cited by 1,061
Metadata
- Authors
- Jull, A. J. T., Courtney, C., Jeffrey, D. A., & Beck, J. W.
- Affiliations
- U.S. National Science Foundation (US)
- ORCID
- Beck, J. W.
- Venue
- Science
- Published
- 1998-01-16
- Volume
- 279
- Issue
- 5349
- Pages
- 366-369
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W1991009883
- Cited by
- 159
- References
- 0
- Citations by year
- 2026: 1 · 2025: 3 · 2024: 2 · 2023: 4 · 2022: 3 · 2021: 4 · 2020: 1 · 2019: 1 · 2018: 4 · 2016: 3 · 2015: 4 · 2014: 5 · 2013: 5 · 2012: 7
- FWCI
- 10.86
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Science (publishedVersion)
- PubMed (publishedVersion)
- 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 › Paleontology › Paleontology and Stratigraphy of Fossils
- Keywords
- Martian meteorites, ALH84001, organic compounds, terrestrial contamination, carbon isotopes, carbon-14, carbonates
- MeSH terms
- Carbon, Carbon Dioxide, Carbon Isotopes, Carbon Radioisotopes, Carbonates, Hot Temperature, Organic Chemicals, Silicates, Mars, Meteoroids
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