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Estranged planetary twins
DOI:10.1038/s41561-022-01104-z.png)
Abstract
En 中文
Venus and Earth have remarkably different surface conditions, yet the lithospheric thickness and heat flow on Venus may be Earth-like. This finding supports a tectonic regime with limited surface mobility and dominated by intrusive magmatism.
Keywords:
VENUS
Journal
IF:
16.1
Papers:
4.6K
Citations:
4.1W

