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Venus’ surprisingly thin crust is more active than Earth’s, NASA reveals

Data for the study came from NASA’s Magellan mission, which orbited Venus in the 1990s. Though decades old, its radar provided detailed topographic and gravity maps of the planet.

May 15, 2025 / 14:15 IST
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This artist’s concept of the large Quetzalpetlatl Corona located in Venus’ southern hemisphere depicts active volcanism and a subduction zone, where the foreground crust plunges into the planet’s interior. A new study suggests coronae are the locations of several types of tectonic activity. (Image: NASA)

Venus, often seen as Earth's fiery twin, might still be evolving deep below its surface. A fresh look at decades-old NASA data hints that Venus is not as quiet as once thought. Scientists now suggest that the planet may have active tectonic processes.

Coronae Show Signs of Tectonic Activity

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The study focused on large, circular features called coronae. These lie across Venus’ surface and range from tens to hundreds of miles wide. Researchers say they form when hot material rises from the planet’s mantle and pushes up against the crust.

Data for the study came from NASA’s Magellan mission, which orbited Venus in the 1990s. Though decades old, its radar provided detailed topographic and gravity maps of the planet. Using these maps, researchers found that 52 out of 75 coronae show signs of motion below the surface.