Lunar Evolution in Light of the Chang'e-5 Returned Samples

FY Wu, QL Li, Y Chen, S Hu, ZY Yue… - Annual Review of …, 2024 - annualreviews.org
The Chinese spacecraft Chang'e-5 (CE-5) landed on the northern Ocean Procellarum and
returned 1,731 grams of regolith. The CE-5 regolith is composed mostly of fragments of …

Non-KREEP origin for Chang'e-5 basalts in the Procellarum KREEP Terrane

HC Tian, H Wang, Y Chen, W Yang, Q Zhou, C Zhang… - Nature, 2021 - nature.com
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 …

Magmatic evolution II: A new view of post-differentiation magmatism

C Shearer, CR Neal, TD Glotch… - … in Mineralogy and …, 2023 - pubs.geoscienceworld.org
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 …

Fusible mantle cumulates trigger young mare volcanism on the Cooling Moon

B Su, J Yuan, Y Chen, W Yang, RN Mitchell, H Hui… - Science …, 2022 - science.org
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 …

Generation, ascent and eruption of magma on the Moon: New insights into source depths, magma supply, intrusions and effusive/explosive eruptions (Part 2 …

JW Head, L Wilson - Icarus, 2017 - Elsevier
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 …

Lunar mare TiO2 abundances estimated from UV/Vis reflectance

H Sato, MS Robinson, SJ Lawrence, BW Denevi… - Icarus, 2017 - Elsevier
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 …

Lunar compositional asymmetry explained by mantle overturn following the South Pole–Aitken impact

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 magmatic architecture and evolution of the Chang'e-5 lunar basalts

B Luo, Z Wang, J Song, Y Qian, Q He, Y Li… - Nature …, 2023 - nature.com
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 …

Titanium in olivine reveals low-Ti origin of the Chang'E-5 lunar basalts

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 …

[HTML][HTML] The origin of water in the primitive Moon as revealed by the lunar highlands samples

JJ Barnes, R Tartèse, M Anand, FM McCubbin… - Earth and Planetary …, 2014 - Elsevier
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 …