... lunar crust that formed near the surface must have survived the early bombardment, but the implications of this observation for the early impact history will require significant advances in our understanding of regolith dynamics on the Moon (Chapman et al ...
[
Текст
]
Ссылки http://www.mso.anu.edu.au/~charley/papers/NormanLineweaver2008.pdf -- 604.5 Кб -- 07.05.2008 Похожие документы
... life forms, the free energy of the Moon is dissipated by heat flow due to the large temperature gradients (low entropy structures) between regolith in the sunshine at 350 K and the shadows at 150 K. The input of low entropy solar radiation maintains the ...
[
Текст
]
Ссылки http://www.mso.anu.edu.au/~charley/papers/LineweaverEgan2008v2.pdf -- 826.4 Кб -- 18.03.2009 Похожие документы