Mare volcanics on the Moon are the key record of thermo-chemical evolution throughout most of lunar history,–. Young mare basalts—mainly distributed in a region rich in …
Just as the use of new tools revolutionized lunar science in 1610 (Galileo's telescope), 1840 (photography), and 1960s–1970s and 1990s (over 45 robotic and human missions to the …
The Chang'E-5 (CE5) mission has demonstrated that lunar volcanism was still active until two billion years ago, much younger than the previous isotopically dated lunar basalts. How …
We utilize a theoretical analysis of the generation, ascent, intrusion and eruption of basaltic magma on the Moon to develop new insights into magma source depths, supply processes …
Abstract The visible (400–700 nm) and near-infrared (700–2800 nm) reflectance of the lunar regolith is dominantly controlled by variations in the abundance of plagioclase, iron-bearing …
N Zhang, M Ding, MH Zhu, H Li, H Li, Z Yue - Nature Geoscience, 2022 - nature.com
The spatial distribution of mare basalts, titanium and KREEP (potassium, rare earth elements and phosphorus) on the Moon is asymmetrical between the nearside and farside …
The lunar basalt samples returned by the Chang'e-5 mission erupted about 2.0 billion years ago during the late period of the Moon's secular cooling. The conditions of mantle melting in …
D Zhang, B Su, Y Chen, W Yang, Q Mao, LH Jia - Lithos, 2022 - Elsevier
Abstract China's Chang'E-5 mission returned new samples from the Moon and has extended the eruption ages of lunar volcanism ca. 800 million years younger than previous …
The recent discoveries of hydrogen (H) bearing species on the lunar surface and in samples derived from the lunar interior have necessitated a paradigm shift in our understanding of …