Understanding the textures of Apollo 11 high‐Ti mare basalts: A quantitative petrographic approach-Reference-Cited by-同舟云学术

Understanding the textures of Apollo 11 high‐Ti mare basalts: A quantitative petrographic approach

Published:2021-12 Issue:12 Volume:56 Page:2211-2229
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:Meteorit & Planetary Scien

Author:

Xue Zhuqing¹²³^ORCID,Welsh Donald F.³,Neal Clive R.³^ORCID,Xiao Long⁴^ORCID

Affiliation:

1. School of Marine Sciences University of the Chinese Academy of Sciences Beijing 100049 China

2. Center of Deep‐Sea Research Institute of Oceanology Chinese Academy of Sciences Qingdao 266071 China

3. Department of Civil and Environmental Engineering and Earth Sciences University of Notre Dame Notre Dame Indiana 46556 USA

4. School of Earth Sciences China University of Geosciences Wuhan 430074 China

Funder

China Scholarship Council

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.13767

Reference49 articles.

1. Beaty D. W. andAlbee A. L.1978. Comparative Petrology and Possible Genetic Relations Among the Apollo 11 Basalts. Proceedings 9th Lunar and Planetary Science Conference. pp.359–463.

2. Beaty D. W. andAlbee A. L.1980. The Geology and Petrology of the Apollo 11 Landing Site. Proceedings 11th Lunar and Planetary Science Conference. pp.23–35.

3. Beaty D. W. Hill S. M. R. Albee A. L. Ma M. S. andSchmitt R. A.1979. The Petrology and Chemistry of Basaltic Fragments from the Apollo 11 Soil Part 1. Proceedings 10th Lunar and Planetary Science Conference. pp.41–75.

4. Brown G. M. Peckett A. Emeleus C. H. Phillips R. andPinsent R. H.1975.Petrology and Mineralogy of Apollo 17 Mare Basalts. Proceedings 6th Lunar Science Conference 1–13.

5. CHAPTER 10. TEXTURAL CONSTRAINTS ON THE KINETICS OF CRYSTALLIZATION OF IGNEOUS ROCKS

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