Abstract
The various models which have been put forward to define the thermal evolution of Venus are outlined and discussed. A model is then presented which deals in turn with the thermal evolution, and present thermal regime, of the crust, mantle and core. -S.J.Stone
| Original language | English |
|---|---|
| Pages (from-to) | 280-319 |
| Number of pages | 40 |
| Journal | Unknown Journal |
| State | Published - 1992 |
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