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
β¦ LIBER β¦
The Geology and Habitability of Terrestrial Planets: Fundamental Requirements for Life
β Scribed by G. Southam; L. J. Rothschild; F. Westall
- Publisher
- Springer Netherlands
- Year
- 2007
- Tongue
- English
- Weight
- 874 KB
- Volume
- 129
- Category
- Article
- ISSN
- 0038-6308
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Simulations of the Atmospheres of Synchr
β
M.M. Joshi; R.M. Haberle; R.T. Reynolds
π
Article
π
1997
π
Elsevier Science
π
English
β 887 KB
Chemical fingerprints of life in terrest
β
Amos Banin; Jerzy Navrot
π
Article
π
1979
π
Elsevier Science
π
English
β 829 KB
Dust particles in the atmospheres of ter
β
Vladimir A. Basiuk; Rafael Navarro-Gonzalez
π
Article
π
1996
π
Springer Netherlands
π
English
β 1015 KB
Relevance of oxygen and ozone detections
β
A. LΓ©ger; M. Pirre; F.J. Marceau
π
Article
π
1994
π
Elsevier Science
π
English
β 367 KB
A Raman spectroscopic study of the igneo
β
Linda C. Prinsloo; Philippe Colomban; Johan D. Brink; Ian Meiklejohn
π
Article
π
2010
π
John Wiley and Sons
π
English
β 315 KB
## Abstract The geology of Marion Island is typical of the oceanic volcanoes forming the Hawaiian archipelago, which is generally seen as an analogue for the geology on Mars. Because of the cold climate, the relatively young igneous rocks on Marion Island exhibit no visible alteration from the orig
Required thermal environments for the qu
β
Toshinori Ishii; Tamaho Yashiro; Noriaki Okamura; Takehiro Sano; Joseph Akira Yo
π
Article
π
1996
π
Springer US
π
English
β 920 KB