Magma source transition of lunar mare volcanism at 2.3 Ga

Author:

Kato Shinsuke1ORCID,Morota Tomokatsu1,Yamaguchi Yasushi1,Watanabe Sei‐ichiro1,Otake Hisashi2,Ohtake Makiko2

Affiliation:

1. Graduate School of Environmental Studies Nagoya University Furo‐cho Chikusa‐ku Nagoya 464–8602 Japan

2. Japan Aerospace Exploration Agency 3‐1‐1 Yoshinodai Sagamihara Kanagawa 229‐8510 Japan

Funder

Japan Society for the Promotion of Science

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Reference90 articles.

Cited by 16 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. A shallow (<100 km) ilmenite-bearing pyroxenitic source for young lunar volcanism;Earth and Planetary Science Letters;2024-08

2. The Lunar Cratering Chronology;Reviews in Mineralogy and Geochemistry;2023-12-01

3. The Evolution of the Lunar Crust;Reviews in Mineralogy and Geochemistry;2023-12-01

4. Magmatic Evolution II: A New View of Post-Differentiation Magmatism;Reviews in Mineralogy and Geochemistry;2023-12-01

5. Long-lived lunar volcanism sustained by precession-driven core-mantle friction;National Science Review;2023-10-31

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