論文

査読有り
2017年2月

Biogenic oxygen from Earth transported to the Moon by a wind of magnetospheric ions

NATURE ASTRONOMY
  • Kentaro Terada
  • ,
  • Shoichiro Yokota
  • ,
  • Yoshifumi Saito
  • ,
  • Naritoshi Kitamura
  • ,
  • Kazushi Asamura
  • ,
  • Masaki N. Nishino

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2
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1038/s41550-016-0026
出版者・発行元
NATURE PUBLISHING GROUP

For five days of each lunar orbit, the Moon is shielded from solar wind bombardment by the Earths magnetosphere, which is filled with terrestrial ions. Although the possibility of the presence of terrestrial nitrogen and noble gases in lunar soil has been discussed based on their isotopic composition, complicated oxygen isotope fractionation in lunar metal(2,3) (particularly the provenance of a O-16-poor component) remains an enigma(4,5) . Here, we report observations from the Japanese spacecraft Kaguya of significant numbers of 110 keV O+ ions, seen only when the Moon was in the Earths plasma sheet. Considering the penetration depth into metal of O+ ions with such energy, and the O-16-poor mass-independent fractionation of the Earths upper atmosphere 6 , we conclude that biogenic terrestrial oxygen has been transported to the Moon by the Earth wind (at least 2.6 x104 ions cm(-2) s(-1)) and implanted into the surface of the lunar regolith, at around tens of nanometres in depth (3,4) . We suggest the possibility that the Earths atmosphere of billions of years ago may be preserved on the present-day lunar surface.

リンク情報
DOI
https://doi.org/10.1038/s41550-016-0026
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000406528600002&DestApp=WOS_CPL
ID情報
  • DOI : 10.1038/s41550-016-0026
  • ISSN : 2397-3366
  • Web of Science ID : WOS:000406528600002

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