TRANSPORT OF THE FIRST ROCKS OF THE SOLAR SYSTEM BY X-WINDS
It has been suggested that chondrules and calcium-aluminum-rich inclusions (CAIs) were formed at the inner edge of the protoplanetary disk and then entrained in magnetocentrifugal X-winds. We study trajectories of such solid bodies with the consideration of the central star gravity, the protoplaneta...
Main Author: | Hu, Renyu |
---|---|
Other Authors: | Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences |
Format: | Article |
Language: | en_US |
Published: |
Institute of Physics/American Astronomical Society
2015
|
Online Access: | http://hdl.handle.net/1721.1/95840 |
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