摘要 : All landforms on Titan that are unambiguously identifiable can be explained by exogenic processes (aeolian, fluvial, impact cratering, and mass wasting). Previous suggestions of endogenically produced cryovolcanic constructs and f... 展开
作者 | Moore~ J.M. Pappalardo~ R.T. |
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作者单位 | |
期刊名称 | 《Icarus: International Journal of Solar System Studies》 |
总页数 | 17 |
语种/中图分类号 | 英语 / P18 |
关键词 | Saturn satellites Titan Titan atmosphere Titan hydrology Titan surface |
馆藏号 | N2008EPST0014254 |