We have numerically computed the orbital evolution of โผ10 3 particles representing high-speed ejecta from Gilgamesh, the largest impact basin on Ganymede. The integration includes the four Galilean satellites, Jupiter (including J 2 and J 4 ), Saturn, and the Sun. The integrations last 100,000 years
โฆ LIBER โฆ
Coupled Orbital and Thermal Evolution of Ganymede
โ Scribed by Adam P. Showman; David J. Stevenson; Renu Malhotra
- Publisher
- Elsevier Science
- Year
- 1997
- Tongue
- English
- Weight
- 528 KB
- Volume
- 129
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
Orbital Evolution of Impact Ejecta from
โ
Jose Luis Alvarellos; Kevin J. Zahnle; Anthony R. Dobrovolskis; Patrick Hamill
๐
Article
๐
2002
๐
Elsevier Science
๐
English
โ 479 KB
On the comparative evolution of Ganymede
โ
Patrick Cassen; Stanton J. Peale; Ray T. Reynolds
๐
Article
๐
1980
๐
Elsevier Science
๐
English
โ 535 KB
Tidal Evolution into the Laplace Resonan
โ
Adam P. Showman; Renu Malhotra
๐
Article
๐
1997
๐
Elsevier Science
๐
English
โ 570 KB
1 / 2 ศ 3/2 and 1 / 2 ศ 2 resonances can pump Ganymede's free eccentricity up to ศ10 ุ3 independent of Q Gany /Q J . We also We use the numerical model of R. Malhotra (1991, Icarus show that Ganymede's free eccentricity cannot have been 94, 399-412) to explore the orbital history of Io, Europa, and
History and evolution of Chiron's orbit
โ
H. Scholl
๐
Article
๐
1979
๐
Elsevier Science
๐
English
โ 262 KB
Stability and evolution of primeval luna
โ
Bruce A. Conway
๐
Article
๐
1986
๐
Elsevier Science
๐
English
โ 431 KB
Comparative thermal evolution of Uranus
โ
W.B. Hubbard
๐
Article
๐
1978
๐
Elsevier Science
๐
English
โ 302 KB