Mercury's polar ice formation. Computer illustration illustrating the formation of Mercury's polar ice deposits. (A) High-latitude impact crater lit by angled Sun rays creates a region of very warm temperatures on the rim,with lower temperatures on the floor,and extremely cold temperatures in regions of permanent shadow. (B) A comet or water-rich asteroid containing organic compounds impacts Mercury. (C) The water and organic compounds are spread over a wide region with a small fraction migrating to the poles where they become cold-trapped as ices. (D) Over time,water ice in the warmer regions vaporises,leaving more stable organic impurities at the surface. (E) The ice retreats further to a stable long-term configuration. In the coldest areas,water | |
Licence : | Droits gérés |
Crédit: | Science Photo Library / Carnegie Institution of Washington / Johns Hopkins University Applied Physics Laboratory / NASA |
Taille de l’image : | 1967 px × 5428 px |
Model Release : | Non requis |
Property Release : | Non requis |
Restrictions : | - |