๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Cosmochemistry and structure of the giant planets and their satellites

โœ Scribed by David J. Stevenson

Publisher
Elsevier Science
Year
1985
Tongue
English
Weight
954 KB
Volume
62
Category
Article
ISSN
0019-1035

No coin nor oath required. For personal study only.

๐Ÿ“œ SIMILAR VOLUMES

Photoevaporation of the Solar Nebula and
Photoevaporation of the Solar Nebula and the Formation of the Giant Planets
โœ Frank H. Shu; Doug Johnstone; David Hollenbach ๐Ÿ“‚ Article ๐Ÿ“… 1993 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 611 KB

We review the prevailing theories for the formation of the jovian planets and comment that they do not provide a natural explanation for the oft-noted subdivision into two separate classes: the gas-rich giants, Jupiter and Saturn, and the gas-poor giants, Uranus and Neptune. To account for the obser

Structure and Transport in the Solar Neb
Structure and Transport in the Solar Nebula from Constraints on Deuterium Enrichment and Giant Planets Formation
โœ A. Drouart; B. Dubrulle; D. Gautier; F. Robert ๐Ÿ“‚ Article ๐Ÿ“… 1999 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 494 KB

A simplified analytical model of an evolutionary nebula is used to generate temperature-density radial profiles following the procedure elaborated by Dubrulle (Icarus 106, 59, 1993). Each nebula disk is characterized by its initial mass M D , its initial radius R D , and the coefficient of turbulent