Uranus after Voyager 2 and the origin of the solar system
Abstract
The discoveries made by the Voyager 2 spacecraft at Uranus in January 1986 are discussed in the light of the modern Laplacian theory for the formation of the solar system. The most important confirmation by Voyager was the discovery of 2 new satellite groups near orbital radii 2 1/2 RU and 3 1/2 RU (RU = Uranus' equatorial radius), as first predicted in 1977. The discovery that the densities of the Uranian satellites are consistent with these bodies having condensed in a single compositional class, consisting of anhydrous rock, NH3 ice and CH4.6H2O clathrate hydrate in normal solar proportions, confirms the hypothesis that the chemistry of all planetary/regular satellite systems are accounted for by a single choice of the turbulence parameter, namely β = 0.107±0.001. The implication of the Voyager data for the origin of comets is also discussed.
- Publication:
-
Publications of the Astronomical Society of Australia
- Pub Date:
- 1986
- DOI:
- 10.1017/S1323358000018270
- Bibcode:
- 1986PASA....6..394P
- Keywords:
-
- Astronomical Models;
- Planetary Evolution;
- Solar System;
- Uranus (Planet);
- Convective Flow;
- Laplace Equation;
- Planetary Composition;
- Planetary Magnetic Fields;
- Supersonic Flow;
- Uranus Satellites;
- Voyager 2 Spacecraft;
- Lunar and Planetary Exploration