Venus is an extremely hot and dry planet with very little water in its atmosphere and no standing water on its surface. However, if Venus had had more water in the past, as the high D/H ratio implies, hydrous minerals might have formed. We present the first experimental study that examines the decom
β¦ LIBER β¦
New insights from one-dimensional spin glasses
β Scribed by Helmut G. Katzgraber; Alexander K. Hartmann; A.P. Young
- Publisher
- Elsevier
- Year
- 2010
- Tongue
- English
- Weight
- 959 KB
- Volume
- 6
- Category
- Article
- ISSN
- 1875-3892
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