Modeling Study Provides New Details about Venus’ Crust

Planetary scientists expected the outermost layer of the crust of Earth’s hotter twin would grow thicker and thicker over time given its apparent lack of forces that would drive the crust back into the planet’s interior. But a team of planetary scientists from The Open University, NASA’s Johnson Space Center and Lunar and Planetary Institute new proposes a crust metamorphism process based on rock density and melting cycles.

An artist’s concept of active volcanoes on Venus, depicting a subduction zone where the foreground crust plunges into the planet’s interior at the topographic trench. Image credit: NASA / JPL-Caltech / Peter Rubin.

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