Although ongoing volcanic activity on Venus has been hypothesized, directly detecting active lava flows is challenging. Now, an analysis of Magellan radar images of Venus acquired at different times provides indications of ongoing volcanic activity in two distinct areas. This evidence also suggests a planet more volcanically active than previously thought.

Radar signatures of active lava flows on Venus

Sulcanese D.;Mitri G.
2024-01-01

Abstract

Although ongoing volcanic activity on Venus has been hypothesized, directly detecting active lava flows is challenging. Now, an analysis of Magellan radar images of Venus acquired at different times provides indications of ongoing volcanic activity in two distinct areas. This evidence also suggests a planet more volcanically active than previously thought.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11564/850853
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