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| | Planetary Formation: Contents of Simulating the Capture Theory |
 | | In early investigations of the capture mechanism, the protostar was assumed to be in a state of quasi-static collapse at the time of the interaction (Woolfson, 1964; Dormand and Woolfson, 1971), although a more freely collapsing protostar was recently envisaged (Dormand and Woolfson, 1988). |
 | | Protostars which collapse at a moderate rate, such that when placed on the Roche limit of the Sun, they are just disrupted at perihelion, tend to produce results similar to those obtained using slowly contracting protostars, rather than rapidly contracting ones. |
 | | Although the protostar is initially stationary in its frame of reference, the angular momentum imparted to it during the course of the interaction, results in the protoplanets containing a finite angular momentum in their spin. |
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