| Literature DB >> 18988811 |
Junichi Haruyama1, Makiko Ohtake, Tsuneo Matsunaga, Tomokatsu Morota, Chikatoshi Honda, Yasuhiro Yokota, Masanao Abe, Yoshiko Ogawa, Hideaki Miyamoto, Akira Iwasaki, Carle M Pieters, Noriaki Asada, Hirohide Demura, Naru Hirata, Junya Terazono, Sho Sasaki, Kazuto Saiki, Atsushi Yamaji, Masaya Torii, Jean-Luc Josset.
Abstract
We determined model ages of mare deposits on the farside of the Moon on the basis of the crater frequency distributions in 10-meter-resolution images obtained by the Terrain Camera on SELENE (Selenological and Engineering Explorer) (Kaguya). Most mare volcanism that formed mare deposits on the lunar farside ceased at approximately 3.0 billion years ago, suggesting that mare volcanism on the Moon was markedly reduced globally during this period. However, several mare deposits at various locations on the lunar farside also show a much younger age, clustering at approximately 2.5 billion years ago. These young ages indicate that mare volcanism on the lunar farside lasted longer than was previously considered and may have occurred episodically.Entities:
Year: 2008 PMID: 18988811 DOI: 10.1126/science.1163382
Source DB: PubMed Journal: Science ISSN: 0036-8075 Impact factor: 47.728