Protoplanetary disk formation
Abstract
The process of the formation of planets in an initial nonturbulent gas-dust protoplanetary disk surrounding the sun is discussed. A working model of joint sun-protoplantary disk formation is presented. This model can be improved by determining the two- and three-dimensional structures of the disk and constructing a quantitative theory of turbulence and the magnetic field in the sun and the disk.
- Publication:
-
Astronomicheskii Vestnik
- Pub Date:
- December 1987
- Bibcode:
- 1987AVest..21..303R
- Keywords:
-
- Accretion Disks;
- Planetary Evolution;
- Protoplanets;
- Solar System;
- Gravitational Collapse;
- Meteorites;
- Molecular Clouds;
- Stellar Mass Accretion;
- Lunar and Planetary Exploration