Abstract
Planetary satellites are an important source of mass for planetary magnetospheres. Meteoroid impact vaporization is a supply mechanism which can potentially compete with charged-particle sputtering. Recent estimates of impact fluxes in the outer solar system vary by several orders of magnitude. For the larger flux values impact vaporization will play a role both at Jupiter and Saturn, although for the most part it will not dominate sputtering. At the small end of the flux range, sputtering dominates magnetospheric mass-loading everywhere.
Original language | English |
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Pages (from-to) | 258-269 |
Number of pages | 12 |
Journal | Icarus |
Volume | 66 |
Issue number | 2 |
DOIs | |
State | Published - May 1986 |
Externally published | Yes |