Abstract
Computational simulations of Venus’s geodynamics show the formation of large tessera plateaus. Matching of the models with spacecraft orbiter data constrains the mechanism that may have formed the topography of Ishtar Terra and other plateaus on Venus, suggesting that these features might have formed by a mechanism similar to that of the early continents on Earth.
Original language | English |
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Pages (from-to) | 717-718 |
Number of pages | 2 |
Journal | Nature Geoscience |
Volume | 17 |
Issue number | 8 |
DOIs |
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Publication status | Published - 6 Aug 2024 |