3D map sheds light on distant planet
- A team of researchers has generated the first 3D map of a planet orbiting another star, WASP-18b, using a new technique called 3D eclipse mapping.
- The map reveals an atmosphere with distinct temperature zones, including one that is scorching hot and breaks down water vapor.
- The technique allows scientists to image exoplanets that are too bright for direct observation, enabling them to study their atmospheres in detail.
- WASP-18b, a gas giant located 400 light years from Earth, has temperatures approaching 5,000 degrees Fahrenheit and features a circular hotspot where the most direct starlight lands.
- The discovery provides evidence that the planet’s atmosphere is breaking down water vapor due to its extreme heat, offering insights into the formation and evolution of exoplanets.
Researchers have generated the first 3D map of a planet orbiting another star.
The map reveals an atmosphere with distinct temperature zones—one so scorching that it breaks down water vapor.
“Partially, this result is really cool because it’s a demonstration of a new technique,” says Rauscher, University of Michigan associate professor of astronomy.
“Scientifically, this result is also really cool because, for this particular planet, it gets incredibly hot.”
The team, co-led by Ryan Challener of Cornell University and Megan Weiner Mansfield of the University of Maryland, published its findings in the journal Nature Astronomy.
The team’s temperature map is of a planet known as WASP-18b, which is a gas giant, like Jupiter in our solar system, but it’s located 400 light years from Earth. It is so close to its star and so hot that scientists refer to it as an “ultra hot Jupiter.”
The team’s effort demonstrates a technique called 3D eclipse mapping, or spectroscopic eclipse mapping. The effort builds on a 2D model that members of the same team published in 2023, which demonstrated eclipse mapping’s potential to leverage highly sensitive observations by the JWST, Earth’s most powerful space telescope. Operated by NASA, the JWST is also supported by the European Space Agency and the Canadian Space Agency.
“Eclipse mapping allows us to image exoplanets that we can’t see directly, because their host stars are too bright,” says Challener, a postdoctoral associate at Cornell. “With this telescope and this new technique, we can start to understand exoplanets along the same lines as our solar system neighbors.”
Similar to how Earth-based telescopes enabled astronomers to start characterizing Jupiter’s Great Red Spot long ago, JWST will now enable scientists to start characterizing more exoplanet atmospheres with this technique, the team says.
Detecting exoplanets is a challenge to begin with. Light from their host stars can overwhelm what’s emitted by the planets. In terms of brightness, exoplanets are typically less than 0.1% as bright as their stars.
“The analogy is a firefly in front of a lighthouse,” Rauscher says. “But we know when the planet is in front of and when it’s behind the star. We can actually measure that tiny little dip that had been light coming from the planet.”
JWST can precisely measure how that light is lost as the planet moves behind the star. This enables scientists to link minute changes in light to specific regions to produce a brightness map across a spectrum of different light wavelengths, or colors. That spectroscopic information can be converted to temperatures in three dimensions: latitude, longitude, and altitude.
WASP-18b, which has roughly the mass of 10 Jupiters, orbits in just 23 hours and has temperatures approaching 5,000 degrees Fahrenheit. That provided JWST with a relatively strong signal, making it a good test case for the new mapping technique.
The new view of the exoplanet confirmed spectroscopically distinct regions in WASP-18b’s visible “dayside,” the side always facing the star due to its tidally locked orbit. The planet features a circular “hotspot” where the most direct starlight lands, and where winds appear too weak to redistribute the heat. Surrounding the hotspot is a colder ring nearer the planet’s outer visible edges, or limbs. Notably, Challener says, measurements showed lower levels of water vapor in the hotspot than WASP-18b’s average.
“We think that’s evidence that the planet is so hot in this region that it’s starting to break down the water,” Challener says. “That had been predicted by theory, but it’s really exciting to actually see this with real observations.”
Additional JWST observations could help improve the first 3D eclipse map’s spatial resolution, the team says. And the technique can already help map the 3D temperature variation of other hot Jupiters, which account for hundreds of the more than 6,000 exoplanets confirmed to date.
“One of the really cool things about exoplanets is that most of the planets we found are completely unlike the ones in our solar system,” Rauscher says.
“And so it’s a lot of fun to try and figure out how we take what we understand, more or less, in our solar system and stretch it to these very different situations.”
The team included about three dozen researchers from more than 20 institutions worldwide. The research was supported by JWST’s Transiting Exoplanet Community Early Release Science Program.
Source: University of Michigan
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