4.7 Article

The Geological History of the Chang'e-5 Sample Return Region

Journal

REMOTE SENSING
Volume 13, Issue 22, Pages -

Publisher

MDPI
DOI: 10.3390/rs13224679

Keywords

Moon; CE-5; geological features; volcanism; tectonism

Funding

  1. B-type Strategic Priority Program of the Chinese Academy of Sciences [XDB41000000]
  2. National Natural Science Foundation of China [42130110, 41571388]
  3. Key projects of national basic work of science and technology [2015FY210500]

Ask authors/readers for more resources

Researchers analyzed the topographic characteristics, mineral composition, and chronology of the landing site region of Chang'e-5 through satellite data, revealing a history of multi-stage magmatic activities forming multiple mare units with different chemical and mineral compositions.
Chang'e-5 (CE-5), China's first sample-return mission, has successfully landed in Oceanus Procellarum near Mons Rumker. It is important to have a detailed study of the geological evolution of the CE-5 sample return region. This work aims to study the geological background, topography, geomorphology, major chemical composition, mineralogy, and chronology of the landing site region. First, we used the map of topography obtained by the Kaguya TC merged Digital Terrain Model (DTM) to analyze the topographic characteristics. Then, we used the Kaguya Multiband Imager (MI) reflectance data to derive FeO and TiO2 abundance and the hyperspectral data of the Moon Mineralogy Mapper (M-3) onboard the Chandrayaan-1 spacecraft to study the mineralogy of the landing site region. Later, we defined and dated the geological units of the landing area using the crater size-frequency distribution (CSFD) method. Finally, we conducted a detailed analysis of the volcanism and tectonism that occurred in the CE-5 landing area. The study region has experienced multi-stage magmatic activities (~3.36 Ga to ~1.22 Ga) and formed multiple mare units with different chemical and mineral compositions. The relationship between the wrinkle ridges cut by small impact craters suggests that the U7/Em5 has experienced Copernican aged tectonism recently ~320 Ma. The U7/Em5 unit where the Chang'e-5 sample return mission landed is dominantly composed of mature pyroxene and the basalts are mainly high-iron and mid-titanium basalts. Additionally, the analysis of pure basalt in the U7/Em5 suggests that the samples returned by the CE-5 mission may contain the ejecta and ray materials of young craters, including sharp B, Harding, Copernicus, and Aristarchus.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.7
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available