A catalogue of impact craters larger than 200 m and surface age analysis in the Chang'e-5 landing area

•32,277 craters larger than 200 m are mapped in the landing area, near Mons Rümker.•Craters smaller than 1 km are denser in the east and west parts of the area.•The N (D>1 km) of different geologic units in the landing area are calculated.•Radioisotope dating of returned samples can calibrate lun...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Earth and planetary science letters 2020-07, Vol.541, p.116272, Article 116272
Hauptverfasser: Jia, Mengna, Yue, Zongyu, Di, Kaichang, Liu, Bin, Liu, Jianzhong, Michael, Gregory
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
Beschreibung
Zusammenfassung:•32,277 craters larger than 200 m are mapped in the landing area, near Mons Rümker.•Craters smaller than 1 km are denser in the east and west parts of the area.•The N (D>1 km) of different geologic units in the landing area are calculated.•Radioisotope dating of returned samples can calibrate lunar chronology function. Chang'e-5 (CE-5) is the first sample-return mission of China's lunar exploration and will be launched in 2020. The planned landing area is near Mons Rümker in Oceanus Procellarum. It is important to have a detailed geological analysis of the landing area prior to the lunar sample collection. The crater size-frequency distribution curve, combined with radioisotope dating of components of the returned sample by CE-5, may allow a refinement of the lunar chronology function. Based on a digital orthophoto map with a pixel size of 1.5 m generated from more than 700 Lunar Reconnaissance Orbiter Camera Narrow Angle Camera images of the CE-5 landing area, all impact craters larger than 200 m in diameter were extracted. Using the resultant crater catalogue of 32,277 craters, a systematic analysis of the landing area including the crater distribution, morphology characteristics, and geologic model ages is conducted. The results show that craters smaller than 1,000 m are denser in the east and the west parts of the region, while those larger than 1,000 m tend to be more concentrated in the central part, particularly within the range of 61.5°W–64.5°W. Within nine geologic units divided using the spectral characteristics, the geologic unit of Em1 (Eratosthenian-aged mare, Em) near the Mons Rümker is the youngest with a model age of 2.02−0.16+0.16 Ga. The three Rümker plateau (IR) units are the oldest parts of the landing area with the largest model age of 3.49−0.12+0.073 Ga. The crater catalogue and the surface model age analysis results can contribute to the CE-5 mission as well as further scientific research.
ISSN:0012-821X
1385-013X
DOI:10.1016/j.epsl.2020.116272