We have studied two scenarios for the in situ formation of Uranus and Neptune from a hundred or so sub-Earth-sized planetary embryos initially on low-inclination, nearly circular orbits beyond Saturn. We find that giant planets do not form during integrations of such systems. Almost no accretion occ
โฆ LIBER โฆ
On the formation and stability of Uranus' rings
โ Scribed by Paolo Farinella; Paolo Paolicchi; Federico Ferrini; Anna M. Nobili
- Publisher
- Springer Netherlands
- Year
- 1980
- Tongue
- English
- Weight
- 492 KB
- Volume
- 22
- Category
- Article
- ISSN
- 1573-0794
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
Remarks on Modeling the Formation of Ura
โ
Harold F. Levison; Glen R. Stewart
๐
Article
๐
2001
๐
Elsevier Science
๐
English
โ 106 KB
Near-infrared spectrophotometry of the s
โ
B.T. Soifer; G. Neugebauer; K. Matthews
๐
Article
๐
1981
๐
Elsevier Science
๐
English
โ 391 KB
Two-micron spectrophotometry of Uranus a
โ
P.D. Nicholson; T.J. Jones
๐
Article
๐
1980
๐
Elsevier Science
๐
English
โ 985 KB
The occultation of KME 17 by Uranus and
โ
J.L. Elliot; I.S. Glass; R.G. French; J.A. Kangas
๐
Article
๐
1987
๐
Elsevier Science
๐
English
โ 825 KB
Comparison of density waves in the rings
โ
Padmavati A. Yanamandra-Fisher
๐
Article
๐
1992
๐
Elsevier Science
๐
English
โ 488 KB
On the Stability of Graded Rings
โ
H.S. Li
๐
Article
๐
1994
๐
Elsevier Science
๐
English
โ 559 KB
Let \(R=\oplus_{n \in \mathbb{Z}} R_{n}\) be a left Noetherian, left graded regular \(\mathbb{Z}\)-graded ring (i.e., every finitely generated graded \(R\)-module has finite projective dimension). We prove that if every finitely generated graded projective \(R\)-module is graded stably free then eve