Feasibility of a magma ocean dynamo on Mars
Abstract Crustal magnetization of rocks in regions of Mars surface testifies to an era of dynamo activity. I examine the possibility that the dynamo that operated then, in the first 400–600 Ma after Mars formed, was powered by a crystallizing subsurface magma ocean. Of the ways that a magma ocean dy...
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
SpringerOpen
2017-08-01
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| coleção: | Progress in Earth and Planetary Science |
| Assuntos: | |
| Acesso em linha: | http://link.springer.com/article/10.1186/s40645-017-0135-8 |
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