Planet Formation in Circumstellar Disk

Jupiter-Mass planet opens a gap in a solar nebula. The gas around the planet is heated by the accretion of mass onto the planetary surface. The simulation was done by HH Klahr and W. Kley at the University of Tübingen. The ray tracer used is PovRay 3.5. The purpose of this tracing is not a physical model that accurately reproduces photometry at various wavelengths or other fancy physical parameters. The idea is to visualize the development of density and size scales during the collapse. No ...
Author: Astropov; Tags: Astronomy Astrophysics Star Formation Planet Formation Raytracing


















