Star System Formation.
- From: CharlesRCaplan@xxxxxxxxx
- Date: Tue, 19 Aug 2008 13:10:15 -0700 (PDT)
Any folks here sufficiently up to date on the more recent star system
I am assuming that the mass of the star would be irrelevant to the
orbital period of any planets because the more massive the star the
faster the accreation disk would spin.
However, what do the current theories say about quantity and masses of
planets (and other deutris) around low and high mass stars? Would a
small red star have fewer and smaller (or just fewer or just smaller)
planets than a large blue star?
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