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AGU: Geophysical Research Letters

 

Keywords

  • Moon
  • energetic neutral atom
  • solar wind interaction

Index Terms

  • Interplanetary Physics: Neutral particles
  • Interplanetary Physics: Pickup ions
  • Interplanetary Physics: Solar wind plasma
  • Planetary Sciences: Solid Surface Planets: Erosion and weathering
  • Planetary Sciences: Solar System Objects: Moon

Abstract

GEOPHYSICAL RESEARCH LETTERS, VOL. 36, L12104, 4 PP., 2009
doi:10.1029/2009GL038794

Lunar backscatter and neutralization of the solar wind: First observations of neutral atoms from the Moon

D. J. McComas

Southwest Research Institute, San Antonio, Texas, USA

F. Allegrini

Southwest Research Institute, San Antonio, Texas, USA

P. Bochsler

Space Science Center, University of New Hampshire, Durham, New Hampshire, USA

P. Frisch

Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois, USA

H. O. Funsten

Los Alamos National Laboratory, Los Alamos, New Mexico, USA

M. Gruntman

Astronautics and Space Technology Division, University of Southern California, Los Angeles, California, USA

P. H. Janzen

Department of Physics and Astronomy, University of Montana, Missoula, Montana, USA

H. Kucharek

Space Science Center, University of New Hampshire, Durham, New Hampshire, USA

E. Möbius

Space Science Center, University of New Hampshire, Durham, New Hampshire, USA

D. B. Reisenfeld

Department of Physics and Astronomy, University of Montana, Missoula, Montana, USA

N. A. Schwadron

Department of Astronomy, Boston University, Boston, Massachusetts, USA

The solar wind continuously flows out from the Sun, filling interplanetary space and impinging directly on the lunar regolith. While most solar wind ions are implanted into the lunar dust, a significant fraction is expected to scatter back and be emitted as energetic neutral atoms (ENAs). However, this population has never been observed, let alone characterized. Here we show the first observations of backscattered neutral atoms from the Moon and determine that the efficiency for this process, the lunar ENA albedo, is ∼10%. This indicates that the Moon emits ∼150 metric tons of hydrogen per year. Our observations are important for understanding the universal processes of backscattering and neutralization from complex surfaces, which occur wherever space plasmas interact with dust and other small bodies throughout our solar system as well as in exoplanetary systems throughout the galaxy and beyond.

Received 20 April 2009; accepted 22 May 2009; published 18 June 2009.

Citation: McComas, D. J., et al. (2009), Lunar backscatter and neutralization of the solar wind: First observations of neutral atoms from the Moon, Geophys. Res. Lett., 36, L12104, doi:10.1029/2009GL038794.

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