Scientists discover exoplanet with supersonic winds — the fastest in the known universe

Astronomers have found winds on a distant world that blow at a phenomenal 5.6 miles per second (9 kilometers per second), or 20,500 miles per hour (33,000 kilometers per hour) — the fastest winds ever measured on a planet.

The faraway world, a gas giant called WASP-127b that was discovered in 2016, orbits a star 520 light-years from Earth. It zips around its host star in just four days, following a slightly skewed orbit. The exoplanet is also likely tidally locked to its star the same way the moon is to Earth — but perhaps its biggest eccentric trait is that it is slightly larger than Jupiter, yet only 16% as massive, making it one of the puffiest planets known to astronomers. So, its heavily inflated nature enables eager astronomers to look through the upper layers of its atmosphere.

A team led by Lisa Nortmann of Germany's University of Göttingen used a spectrograph on the Very Large Telescope in Chile to observe WASP-127b as it passed in front of its star, blocking some of its light. By analyzing the filtered light, which included distinct dips or "fingerprints" of various molecules that absorbed light at different wavelengths, the researchers identified the presence of carbon monoxide and water vapor in the planet's upper atmosphere.

An illustration of a blurred planet that looks like it has super high wind speeds.

This artist’s visualization of WASP-127b, a giant gas planet located about 520 light-years from Earth, shows its newly discovered supersonic jet winds that move around the planet’s equator.  (Image credit: ESO/L. Calçada)

In studying that spectra further, the researchers say they were puzzled when they noticed two different wavelength peaks for these molecules, which indicated some of those molecules were moving away from Earth while others were moving toward Earth while others were moving away at the same speed.

"I was a little bit confused," Nortmann told New Scientist. "But with a little bit more careful data analysis, it became clearer that there are two signals. I was quite excited — my first thought was immediately that it has to be some sort of super-rotating wind."

Further analysis of the collected spectra showed the movement was maximum at the planet's equator, so the team concluded the observations could be explained by supersonic winds that were constrained to the planet's equator.

“This signal shows us that there is a very fast, supersonic, jet wind around the planet’s equator," Nortmann said in a statement. "This is something we haven’t seen before."

While the reasons for the staggering weather are not fully understood, the researchers interpret these winds to be six times faster than the speed at which the planet itself rotates. For comparison, Neptune holds the record for the fastest winds in our solar system; the winds on WASP-127b are an astonishing 18 times stronger.

The recent observations also suggest the planet has slightly different temperatures between its morning and evening sides, indicating it "has complex weather patterns just like Earth and other planets of our own system," study co-author Fei Yan of the University of Science and Technology of China said in the same statement.

This research is described in a paper published last week in the journal Astronomy and Astrophysics.

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Sharmila Kuthunur
Contributing Writer

Sharmila Kuthunur is a Seattle-based science journalist focusing on astronomy and space exploration. Her work has also appeared in Scientific American, Astronomy and Live Science, among other publications. She has earned a master's degree in journalism from Northeastern University in Boston. Follow her on BlueSky @skuthunur.bsky.social

  • billslugg
    If the planet is tidally locked, the star stays fixed in the sky. There is no "morning side " or "evening side". I don't understand.
    Reply
  • 24launch
    billslugg said:
    If the planet is tidally locked, the star stays fixed in the sky. There is no "morning side " or "evening side". I don't understand.

    Sure it stays fixed in the sky, but the planet is still rotating and the atmosphere is whipping around it in the same direction as the rotation.

    I had to play around with this in my head a bit. But think of the side of the planet that's leading into the orbit as the morning side and the side that's trailing as the evening side. The winds are whipping around in the same direction as the rotation, in fact six times faster. So as the winds go around the backside they cool making the "morning" side cooler as they come back around. And of course heat up more on the daylight side making the "evening" side warmer as they head back around the nightside.

    20,500 MPH is nuts! Considering 17,500 is orbital velocity for Earth!
    Reply
  • George²
    Now I imagine how in 2050, with a new space telescope that is 50 times better than the best ones today, we can actually measure the wind speed of the closest exoplanets to us.
    Reply