Atmosphere-Surface Interactions on Mars: Δ 17 O Measurements of Carbonate from ALH 84001

Author:

Farquhar James1,Thiemens Mark H.1,Jackson Teresa1

Affiliation:

1. Department of Chemistry, University of California San Diego, 92093–0356, USA.(J.F.), (M.H.T.), (T.J.)

Abstract

Oxygen isotope measurements of carbonate from martian meteorite ALH 84001 (δ 18 O = 18.3 ± 0.4 per mil, δ 17 O = 10.3 ± 0.2 per mil, and Δ 17 O = 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 CO 2 and O( 1 D) produced by the photodecomposition of ozone. Atmospheric oxygen isotope compositions may be transferred to carbonate minerals by CO 2 -H 2 O exchange and mineral growth. A sink of 17 O-depleted oxygen, as required by mass balance, may exist in the planetary regolith.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference34 articles.

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