Valence of Ti, V, and Cr in Apollo 14 aluminous basalts 14053 and 14072-Reference-Cited by-同舟云学术

Valence of Ti, V, and Cr in Apollo 14 aluminous basalts 14053 and 14072

Published:2017-07-02 Issue:9 Volume:52 Page:2051-2066
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 The 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

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.12908

Reference50 articles.

1. BenceA. E.andPapikeJ. J.1972.Pyroxenes as recorders of lunar basalt petrogenesis: Chemical trends due to crystal‐liquid interaction. Proceedings 3rd Lunar Science Conference. pp. 431‐469.

2. A XANES determination of the oxidation state of chromium in silicate glasses

3. Titanium substitution mechanisms in forsterite

4. BrownG. M. EmeleusC. H. HollandJ. G. PeckettA. andPhillipsR.1972.Mineral‐chemical variations in Apollo 14 and Apollo 15 basalts and granitic fractions. Proceedings3rd Lunar Science Conference141–157

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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