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Formation age of lunar Lalande crater and its implications for the source region of the KREEP-rich meteorite Sayh al Uhaymir 169

  • Published:2022-11 Issue: Volume:386 Page:115166
  • ISSN:0019-1035
  • Container-title:Icarus
  • language:en
  • Short-container-title:Icarus

Author:

Xu Luyuan,Qiao Le,Xie Minggang,Wu Yunhua

Funder

National Aeronautics and Space Administration

State Key Laboratory of Lunar and Planetary Sciences

Shandong University

Malawi University of Science and Technology

Shanghai Science and Technology Development Foundation

China National Space Administration

Anhui University of Science and Technology

National Natural Science Foundation of China

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference78 articles.

1. The regolith portion of the lunar meteorite Sayh al Uhaymir 169;Al-Kathiri;Meteorit. Planet. Sci.,2007

2. Relative and absolute ages of individual craters and the rate of infalls on the moon in the post-Imbrium period;Baldwin;Icarus,1985

3. Lunar surface rock abundance and regolith fines temperatures derived from LRO diviner radiometer data;Bandfield;J. Geophys. Res. Planets,2011

4. A new lunar digital elevation model from the lunar orbiter laser altimeter and SELENE terrain camera;Barker;Icarus,2016

5. Standard techniques for presentation and analysis of crater size-frequency data;Crater Analysis Techniques Working Group;Icarus,1979

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