First direct detection of ions originating from the Moon by MAP-PACE IMA onboard SELENE (KAGUYA)

Shoichiro Yokota, Yoshifumi Saito, Kazushi Asamura, Takaaki Tanaka, Masaki N. Nishino, Hideo Tsunakawa, Hidetoshi Shibuya, Masaki Matsushima, Hisayoshi Shimizu, Futoshi Takahashi, Masaki Fujimoto, Toshifumi Mukai, Toshio Terasawa

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Abstract

The Moon has no global intrinsic magnetic field and only has a very thin atmosphere. Ion measurements made from lunar orbit provide us with information regarding interactions between the solar wind and planetary surface, the surface composition through secondary ion mass spectrometry and the source and loss mechanisms of planetary tenuous atmosphere. An ion energy mass spectrometer MAP-PACE IMA onboard a lunar orbiter SELENE (KAGUYA) has detected low-energy ions at 100-km altitude. The MAP-PACE measurements have elucidated that the ions originate from the lunar surface and exosphere and that the ions are at least composed of He+, C+, O+, Na+ and K+. Following the discovery of the lunar Na and K exospheres by the ground-based observation, MAP-PACE IMA have found the He, C and 0 exospheres around the Moon.

Original languageEnglish
Article numberL11201
JournalGeophysical Research Letters
Volume36
Issue number11
DOIs
Publication statusPublished - Jun 16 2009
Externally publishedYes

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All Science Journal Classification (ASJC) codes

  • Geophysics
  • Earth and Planetary Sciences(all)

Cite this

Yokota, S., Saito, Y., Asamura, K., Tanaka, T., Nishino, M. N., Tsunakawa, H., ... Terasawa, T. (2009). First direct detection of ions originating from the Moon by MAP-PACE IMA onboard SELENE (KAGUYA). Geophysical Research Letters, 36(11), [L11201]. https://doi.org/10.1029/2009GL038185