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Cited by 209

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

The oxygen‐isotopic composition of Earth and Mars

FRANCHI, I. A., WRIGHT, I. P., SEXTON, A. S., PILLINGER, C. T.·1999·Meteoritics & Planetary Science

Abstract

Abstract— The small difference between the O‐isotopic mass fractionation lines of the Earth and Mars has been measured precisely using a laser fluorination system. The precision achieved from the two sample sets is better than ±0.014‰, with the offset (Δ 17 O) between Mars and Earth measured as +0.321‰. This result shows that all the Shergotty—Nakhla—Chassigny (SNC) meteorites define a high level of isotopic homogeneity, comparable to that of crustal material on the Earth, indicating that these meteorites originate, unequivocally, from a single, common parent body (Mars). Allan Hills 84001, with its ancient age (4.56 Ga), shows that any initial heterogeneity imparted into Mars from the nebula was homogenised very early in the formation history of the planet.

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Crossref · 10.1111/j.1945-5100.1999.tb01371.x

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Metadata

Authors
FRANCHI, I. A., WRIGHT, I. P., SEXTON, A. S., & PILLINGER, C. T.
Venue
Meteoritics & Planetary Science
Publisher
Wiley
Published
1999-07
Volume
34
Issue
4
Pages
657-661
ISSN
  • 1086-9379 (ISSN-L)
  • 1945-5100
OpenAlex
W2027855284
Cited by
209
References
1
FWCI
6.34
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: The oxygen‐isotopic composition of Earth and Mars. https://app.cochat.ai/papers/10.1111/j.1945-5100.1999.tb01371.x
The paper
FRANCHI, I. A., WRIGHT, I. P., SEXTON, A. S., & PILLINGER, C. T. (1999). The oxygen‐isotopic composition of Earth and Mars. Meteoritics & Planetary Science. https://doi.org/10.1111/j.1945-5100.1999.tb01371.x

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