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Science 5 June 1998: Vol. 280. no. 5369, pp. 1580 - 1582 DOI: 10.1126/science.280.5369.1580
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Reports
Atmosphere-Surface Interactions on Mars: 17O Measurements of Carbonate from ALH 84001
James Farquhar,
Mark H. Thiemens,
Teresa Jackson
Oxygen isotope measurements of carbonate from martian meteorite ALH
84001 ( 18O = 18.3 ± 0.4 per mil,
17O = 10.3 ± 0.2 per mil, and
17O = 0.8 ± 0.05 per mil) are fractionated
with respect to those of silicate minerals. These measurements support
the existence of two oxygen isotope reservoirs (the atmosphere and the
silicate planet) on Mars at the time of carbonate growth. The cause of the atmospheric oxygen isotope anomaly may be exchange between CO2 and O(1D) produced by the
photodecomposition of ozone. Atmospheric oxygen isotope compositions
may be transferred to carbonate minerals by
CO2-H2O exchange and mineral growth. A sink of
17O-depleted oxygen, as required by mass balance, may exist
in the planetary regolith.
Department of Chemistry, University of California San Diego,
92093-0356, USA. E-mail: jfarquha{at}ucsd.edu (J.F.), mht{at}ucsd.edu
(M.H.T.), tjackson{at}ucsd.edu (T.J.)
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THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
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Reviews in Mineralogy and Geochemistry
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- Photochemical Mass-Independent Sulfur Isotopes in Achondritic Meteorites.
- V. K. Rai, T. L. Jackson, and M. H. Thiemens (2005)
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309, 1062-1065
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- Mass-independent fractionation of oxygen isotopes during thermal decomposition of carbonates.
- M. F. Miller, I. A. Franchi, M. H. Thiemens, T. L. Jackson, A. Brack, G. Kurat, and C. T. Pillinger (2002)
PNAS
99, 10988-10993
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- Stable Isotope Variations in Extraterrestrial Materials.
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Reviews in Mineralogy and Geochemistry
43, 279-318
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- Mass-Independent Isotope Effects in Planetary Atmospheres and the Early Solar System.
- M. H. Thiemens (1999)
Science
283, 341-345
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