Valences of Ti, Cr, and V in Apollo 17 high‐Ti and very low‐Ti basalts and implications for their formation-Reference-Cited by-同舟云学术

Valences of Ti, Cr, and V in Apollo 17 high‐Ti and very low‐Ti basalts and implications for their formation

Published:2018-06-04 Issue:10 Volume:53 Page:2138-2154
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:Meteorit Planet Sci

Author:

Simon Steven B.¹²³^ORCID,Sutton Stephen R.¹⁴

Affiliation:

1. Department of the Geophysical Sciences University of Chicago 5734 S. Ellis Ave Chicago Illinois 60637 USA

2. The Field Museum of Natural History 1400 South Lake Shore Drive Chicago Illinois 60605 USA

3. Institute of Meteoritics University of New Mexico Albuquerque New Mexico 87131 USA

4. Center for Advanced Radiation Sources (CARS) The University of Chicago 5640 S. Ellis Ave Chicago Illinois 60637 USA

Funder

National Aeronautics and Space Administration

National Science Foundation

U.S. Department of Energy

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.13123

Reference46 articles.

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3. Intrinsic oxygen fugacity measurements on seven chondrites, a pallasite, and a tektite and the redox state of meteorite parent bodies

4. BrownG. M. PeckettA. EmeleusC. H. PhillipsR. andPinsentR. H.1975.Petrology and mineralogy of Apollo 17 mare basalts. Proceedings 6th Lunar Science Conference. pp.1–13.

5. BurnsR. G. VaughanD. J. Abu‐EidR. M. WitnerM. andMorawskiA.1973.Spectral evidence for Cr3+ Ti3+ and Fe2+rather than Cr2+and Fe3+in lunar ferromagnesian silicates. Proceedings 4th Lunar Science Conference. pp.983–994.

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