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Effects of an ICME on the Lunar ExosphereThe lunar exosphere is produced in part by the sputtering of atoms off of the Moon's surface by solar wind ions. We present simulations of He, Na, K, Mg, and Ca in the lunar exosphere under nominal conditions. Next, we examine the resulting exospheric enhancement that occurs during the passage of an Interplanetary Coronal Mass Ejection (ICME). Enhanced sputtering under ICME conditions can increase the mass of the lunar exosphere 10-50 times the nominal value. The increase occurs rapidly within the onset of the ICME. Similarly, after the storm passes the Moon, the return to nominal exospheric density is also rapid. Because sputtered particles are energetic, many escape the Moon. Thus ICMEs induce a mass loss from the Moon. However, the implantation of solar wind into the lunar regolith is also enhanced during an ICME, resulting in mass addition to the Moon. This partially mitigates the mass loss caused by ICME sputtering. We present model estimates of the net lunar mass loss induced by ICMEs
Document ID
20120015962
Document Type
Presentation
Authors
Hurley, Dana M.
Killen, Rosemary M. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Farrell, William M. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 26, 2013
Publication Date
June 18, 2012
Subject Category
Lunar and Planetary Science and Exploration
Report/Patent Number
GSFC.ABS.7444.2012
Meeting Information
Solar Wind 13, Thirteenth International Solar Wind Conference(Kona, HI)
Distribution Limits
Public
Copyright
Public Use Permitted.

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