The Drag Induced Resonant Capture for Kuiper Belt Objects

Details The Drag Induced Resonant Capture for Kuiper Belt Objects The Drag Induced Resonant Capture for Kuiper Belt Objects

2004-10-19

arxiv.org/abs/astro-ph/0410426v2

Astronomy and Astrophysics

Astrophysics

Figure 1 is replaced with the correct one

Scientific paper

10.1111/j.1365-2966.2004.08504.x

It has been an interesting question that why there are one-third of Kuiper Belt Objects (KBOs) trapped into the 3:2 resonance but, in contrast, only several KBOs are claimed to be associated with the 2:1 resonance. In a model proposed by Zhou et al. (2002), the stochastic outward migration of the Neptune could reduce the number of particles in the 2:1 resonance and thus the objects in the 3:2 resonance become more distinct. As a complementary study, we investigate the effect of proto-stellar discs on the resonance capture. Our results show that the gaseous drag of a proto-stellar disc can trap KBOs into the 3:2 resonance rather easily. In addition, no objects are captured into the 2:1 resonance in our simulation.

Affiliated with

Also associated with

No associations

Rating

The Drag Induced Resonant Capture for Kuiper Belt Objects 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 The Drag Induced Resonant Capture for Kuiper Belt Objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Drag Induced Resonant Capture for Kuiper Belt Objects will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-512084