๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Ice clathrate as a possible source of the atmospheres of the terrestrial planets

โœ Scribed by Godfrey T. Sill; Laurel L. Wilkening


Publisher
Elsevier Science
Year
1978
Tongue
English
Weight
684 KB
Volume
33
Category
Article
ISSN
0019-1035

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


A Numerical Survey of Transient Co-orbit
โœ Apostolos A. Christou ๐Ÿ“‚ Article ๐Ÿ“… 2000 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 500 KB

We have investigated numerically the evolution of near-Earth asteroids (3753) Cruithne, (3362) Khufu, 1989 VA, (10563) 1993 WD, and 1994 TF2 that enter the coorbital regions of the Earth or Venus. We show that the coorbital libration modes identified in F. Namouni (1999, Icarus 137, 293-314) and F.

The Effect of a Planet in the Asteroid B
โœ Jack J. Lissauer; Elisa V. Quintana; Eugenio J. Rivera; Martin J. Duncan ๐Ÿ“‚ Article ๐Ÿ“… 2001 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 699 KB

If a planetary-mass body were present in the asteroid belt, the orbits of the terrestrial planets and those of the giant planets would be more closely coupled. A greater exchange of angular momentum could affect the stability of the terrestrial planets. Moreover, the planet in the asteroid belt coul

Simulations of the Atmospheres of Synchr
โœ M.M. Joshi; R.M. Haberle; R.T. Reynolds ๐Ÿ“‚ Article ๐Ÿ“… 1997 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 887 KB

nous of main sequence stars, having masses 0.1-0.5 times the mass of the Sun. The habitable zones around such stars Planets within the habitable zones of M dwarfs are likely to are therefore very close, being typically between 0.03 and be synchronous rotators; in other words, one side is permanently