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- W2334967520 abstract "All four giant planets in the Solar system possess irregular satellites, characterized by large, highly eccentric and/or inclined orbits that are distinct from the nearly circular, uninclined orbits followed by the regular satellites. This dierence can be traced directly to dierent modes of formation. Whereas the regular satellites grew by accretion within circumplanetary disks the irregular satellites were instead captured from initially heliocentric orbits at an early epoch. Powerful survey observations in the last decade have increased the number of known irregular satellites by an order of magnitude, permitting a fresh look at the group properties of these objects. In turn, the new data motivate a re-examination of the mechanisms of capture. None of the suggested mechanisms, including gasdrag, pull-down and three-body capture, has been shown to convincingly fit the group characteristics of the irregular satellites. The sources of the irregular satellites also remain unidentified. Origin by accretion in the protoplanetary disk local to the planets is possible, as is formation in the Kuiper belt or elsewhere in the outer Solar system." @default.
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- W2334967520 date "2007-01-01" @default.
- W2334967520 modified "2023-09-27" @default.
- W2334967520 title "Irregular Satellites of the Planets: Capture Processes in the Early Solar System" @default.
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