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Space
Space
Science
Sarah Stanley

Key Driver of Extreme Winds on Venus Identified

A swirly yellowish white orb against a dark background.

This article was originally published at Eos. The publication contributed the article to Space.com's Expert Voices: Op-Ed & Insights.

Imagine the catastrophic winds of a category 5 hurricane. Now, imagine even faster winds of more than 100 meters per second, encircling the planet and whipping clouds across the sky, with no end in sight. This scenario would be astonishing on Earth, but it's business as usual on Venus, where the atmosphere at cloud level rotates about 60 times faster than the planet itself—a phenomenon known as superrotation. In contrast, Earth's cloud-level atmosphere rotates at about the same speed as the planet's surface.

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