دورية أكاديمية

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

التفاصيل البيبلوغرافية
العنوان: Lunar Evolution in Light of the Chang'e-5 Returned Samples.
المؤلفون: Wu, Fu-Yuan, Li, Qiu-Li, Chen, Yi, Hu, Sen, Yue, Zong-Yu, Zhou, Qin, Wang, Hao, Yang, Wei, Tian, Heng-Ci, Zhang, Chi, Li, Jin-Hua, Li, Lin-Xi, Hui, He-Jiu, Li, Chun-Lai, Lin, Yang-Ting, Li, Xian-Hua, Delano, John W.
المصدر: Annual Review of Earth & Planetary Sciences; May2024, Vol. 52 Issue 1, p159-194, 35p
مصطلحات موضوعية: RARE earth metals, CHLORINE, LUNAR soil, SIDEROPHILE elements, REGOLITH, VOLCANISM, BASALT, ANORTHOSITE
مستخلص: 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 basalt, impact glass, agglutinates, and mineral fragments. The basalts could be classified as of a low-Ti and highly fractionated type based on their TiO2 content of ∼5.3 wt% and Mg# of ∼28. Independent of petrographic texture, the CE-5 basalts have a uniform eruption age of 2,030 ± 4 Ma, demonstrating that the Moon remained volcanically active until at least ∼2.0 Ga. Although the CE-5 landing site lies within the so-called Procellarum KREEP [potassium (K), rare earth elements (REE), and phosphorus (P)] Terrane, neither the CE-5 basalts nor the mantle source regions of those basalts were enriched in KREEP components, such as incompatible elements, water, sulfur, or chlorine. Therefore, it would be a new and stimulating task in the future to look for the triggering mechanism of the young volcanism on the Moon. The CE-5 spacecraft returned 1,731 grams of lunar regolith in December 2020. It was the first new lunar sample since the last collection in August 1976. CE-5 regolith is basaltic in chemical composition, with only ∼1% highland materials of anorthosite, Mg suite, alkali suite, and KREEP. The CE-5 basalt is low Ti and highly differentiated. It was extruded at ∼2.0 Ga, being the youngest lunar basalt identified so far from the Moon. The triggering mechanism of the ∼2.0 Ga lunar volcanism is not clearly understood because its mantle source was dry and contained low abundances of KREEP elements. [ABSTRACT FROM AUTHOR]
Copyright of Annual Review of Earth & Planetary Sciences is the property of Annual Reviews Inc. and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
قاعدة البيانات: Complementary Index
الوصف
تدمد:00846597
DOI:10.1146/annurev-earth-040722-100453