R
rogerinnh
Guest
A recent article on the space.com site about an early solar system being detected got me to thinking about the formation of planetary systems. We always refer to them as solar systems, beacuse the planets rotate about a star. After all, without the star, we wouldn't be able to see them. But I wonder how often a planetary system might evolve from the cosmic dust but without the central, most-massive, object actually becoming a star. Could there be planetary systems in which the central object is simply another planet? In such a system would the central planet necessarily be a gas planet, or could it be a rocky planet? Is it possible that there are actually more non-solar planetary systems than solar planetary systems? Of course, detecting such systems would be mighty difficult, since we can barely even detect solar planetary systems with their huge central star illuminating its neighborhood.