Lifetimes of small bodies in planetocentric (or heliocentric) orbits
Stray bodies orbiting a planet or the Sun are removed by collisions with larger objects or by expulsion from the system. However, their rate of removal generally cannot be described by the simple exponential law used to describe radioactive decay, because their effective half-life lengthens with tim...
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Veröffentlicht in: | Icarus (New York, N.Y. 1962) N.Y. 1962), 2007-06, Vol.188 (2), p.481-505 |
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