A hybrid scenario for gas giant planet formation in rings

Details A hybrid scenario for gas giant planet formation in rings A hybrid scenario for gas giant planet formation in rings

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005icar..173..417d&link_type=abstract

Icarus, Volume 173, Issue 2, p. 417-424.

Physics

33

Scientific paper

The core-accretion mechanism for gas giant formation may be too slow to create all observed gas giant planets during reasonable gas disk lifetimes, but it has yet to be firmly established that the disk instability model can produce permanent bound gaseous protoplanets under realistic conditions. Based on our recent simulations of gravitational instabilities in disks around young stars, we suggest that, even if instabilities due to disk self-gravity do not produce gaseous protoplanets directly, they may create persistent dense rings that are conducive to accelerated growth of gas giants through core accretion. The rings occur at and near the boundary between stable and unstable regions of the disk and appear to be produced by resonances with discrete spiral modes on the unstable side.

Affiliated with

Also associated with

No associations

Rating

A hybrid scenario for gas giant planet formation in rings does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A hybrid scenario for gas giant planet formation in rings, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A hybrid scenario for gas giant planet formation in rings will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1361021