| Literature DB >> 35382442 |
Chunlai Li1, Hao Hu2, Meng-Fei Yang3, Zhao-Yu Pei2, Qin Zhou1, Xin Ren1, Bin Liu1, Dawei Liu1, Xingguo Zeng1, Guangliang Zhang1, Hongbo Zhang1, Jianjun Liu1, Qiong Wang2, Xiangjin Deng3, Caijin Xiao4, Yonggang Yao4, Dingshuai Xue5, Wei Zuo1, Yan Su1, Weibin Wen1, Ziyuan Ouyang1.
Abstract
Forty-five years after the Apollo and Luna missions returned lunar samples, China's Chang'E-5 (CE-5) mission collected new samples from the mid-latitude region in the northeastern Oceanus Procellarum of the Moon. Our study shows that 95% of CE-5 lunar soil sizes are found to be within the range of 1.40-9.35 μm, while 95% of the soils by mass are within the size range of 4.84-432.27 μm. The bulk density, true density and specific surface area of CE-5 soils are 1.2387 g/cm3, 3.1952 g/cm3 and 0.56 m2/g, respectively. Fragments from the CE-5 regolith are classified into igneous clasts (mostly basalt), agglutinate and glass. A few breccias were also found. The minerals and compositions of CE-5 soils are consistent with mare basalts and can be classified as low-Ti/low-Al/low-K type with lower rare-earth-element contents than materials rich in potassium, rare earth element and phosphorus. CE-5 soils have high FeO and low Mg index, which could represent a new class of basalt.Entities:
Keywords: Chang’E-5; chemistry; lunar soils; mineralogy; petrography; physical properties
Year: 2021 PMID: 35382442 PMCID: PMC8974359 DOI: 10.1093/nsr/nwab188
Source DB: PubMed Journal: Natl Sci Rev ISSN: 2053-714X Impact factor: 17.275