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Cited by 168

The DOI matches its Crossref record; 1 of the 1 references it cites were found in a registry or an index.

Water in SNC Meteorites: Evidence for a Martian Hydrosphere

Karlsson, Haraldur R., Clayton, Robert N., Gibson, Everett K., Mayeda, Toshiko K.·1992·Science

Abstract

The Shergotty-Nakhla-Chassigny (SNC) meteorites, purportedly of martian origin, contain 0.04 to 0.4 percent water by weight. Oxygen isotopic analysis can be used to determine whether this water is extraterrestrial or terrestrial. Such analysis reveals that a portion of the water is extraterrestrial and furthermore was not in oxygen isotopic equilibrium with the host rock. Lack of equilibrium between water and host rock implies that the lithosphere and hydrosphere of the SNC parent body formed two distinct oxygen isotopic reservoirs. If Mars was the parent body, the maintenance of two distinct reservoirs may result from the absence of plate tectonics on the planet.

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Crossref · 10.1126/science.11537889

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Metadata

Authors
Karlsson, H. R., Clayton, R. N., Gibson, E. K., & Mayeda, T. K.
Venue
Science
Published
1992-03-13
Volume
255
Issue
5050
Pages
1409-1411
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W1971105678
Cited by
168
References
1
FWCI
13.76
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Water in SNC Meteorites: Evidence for a Martian Hydrosphere. https://app.cochat.ai/papers/10.1126/science.11537889
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Karlsson, H. R., Clayton, R. N., Gibson, E. K., & Mayeda, T. K. (1992). Water in SNC Meteorites: Evidence for a Martian Hydrosphere. Science. https://doi.org/10.1126/science.11537889

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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