Formation of trans-Neptunian satellite systems at the stage of condensations
Abstract
The formation of trans-Neptunian satellite systems at the stage of rarefied preplanetesimals (i.e., condensations of dust and/or objects less than 1 m in diameter) is discussed. It is assumed that trans-Neptunian objects (including those with satellites) could form as a result of compression of parental rarefied preplanetesimals. The formulas for calculating the angular momentum of two colliding condensations with respect to their center of...
Paper Details
Title
Formation of trans-Neptunian satellite systems at the stage of condensations
Published Date
Jul 21, 2017
Journal
Volume
51
Issue
4
Pages
294 - 314
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