A new study reveals how tiny atmospheric ripples may power the planet’s runaway jet streams.

Venus has baffled scientists for decades with its monstrous 220-mph winds—fast enough to circle the entire planet in just four days. These super-rotating winds move far faster than Venus itself spins, raising a long-standing question: what keeps them going? According to new research, the answer may lie in small, previously overlooked atmospheric waves that transfer energy upward and help sustain these extreme jet streams. The findings bring scientists closer to understanding not only Venus’s chaotic weather, but also how atmospheric physics works on other planets, including Earth.








