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JWST data resolve a puffy hot Jupiter's atmosphere into a ring with raised 'gems'

Astronomers used JWST data and a technique called transmission strings to map WASP-17b's atmosphere as a ring with raised 'gems'. The temperature contrast they found matches theory, so the result is a test of the method.

The Scientist · Science desk

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WASP-17b has less mass than Jupiter in more volume WASP-17b's mean density, mass and volume, each set against Jupiter's. The density is worked out from the planet's mass and width.

Key figures for WASP-17b: mean density roughly 0.1 times Jupiter's; mass around 0.8 times Jupiter's; volume about 8 times Jupiter's.

WASP-17b has less mass than Jupiter in more volume
FigureValueNoteClaim
Mean density, roughly, against Jupiter's0.1 × Jupiter15
Mass, around0.8 Jupiter masses11
Volume, about8 × Jupiter15

What happened

  • The modelling put one gem where hot winds reach the equator and nightside, and the atmosphere of the cooler side inflates.
  • WASP-17b has about 0.8 Jupiter masses but is around twice as wide. That gives it a super-puff consistency.
  • The team's paper appeared on Wednesday, Oct. 14, in Nature Astronomy.

Why it matters

  • What's now possible capability Researchers can place features at positions around a transiting planet's limb. A single averaged value cannot do that.
  • What doesn't add up contradiction The result is described as structured and complex, yet the team says the morning-evening temperature contrast matched theory. The result replaces the assumption that the limb has one radius.
  • What it limits constraint The evidence comes from one planet, so using the ring-and-gems shape as a template for other hot Jupiters is untested.

Whether this shows atmospheres to be more complex than models assume depends on which model. The one the technique replaces is narrow. Traditional modelling maps light only as an average across the entire limb [8]. Lili Alderson of Cornell University said: "Rather than assuming your atmosphere is a circle with the same radius all the way around, our technique allows you to pull out different distances from the center to the edge of the planet." [9] Applied to JWST data on WASP-17b, the technique returned an atmosphere shaped like a ring with prominent gems rising from it [5][6].

On the physics, the result lands close to expectation. Space reports that the planet's chemical composition and temperature shift between dayside and nightside according to theory and modelling [1]. Alderson said: "Theory predicts that the morning and the evening sides should have a strong temperature difference" [2]. WASP-17b, she said, was "pretty much bang-on what we thought it would be" [3]. Hannah Wakeford of the University of Bristol said the numbers "showed us this very structured, dynamical picture of this giant world" [14]. The map adds spatial detail to a picture that theory already had.

The planet is an extreme case. It has about 0.8 times Jupiter's mass and is around twice as wide [11]. That puts its mean density near a tenth of Jupiter's [15]. The figure is rough, because the source gives the width only as "around twice".

Space's report is built on a team statement. It does not include the number of transits observed, the JWST instruments used, or an uncertainty on the height of the gems. Those details would be in the Nature Astronomy paper [12].

The result cannot show whether any existing model misses real structure. That would take a planet where the map and the prediction disagree. In our view the result validates the method on a planet where theory had a prediction to check against. Alderson called it "proof of concept that planets are, in fact, 3D objects" [4], and Space describes it as a step forward for modelling the more than 6,000 worlds in NASA's exoplanet catalog [13].

What to watch

  • Transmission strings applied to other transiting planets, especially denser hot Jupiters, to see whether a ring with gems recurs.
  • A mapped planet whose temperatures depart from the predicted morning-evening contrast, which would be the first sign that existing models miss structure.
  • The Nature Astronomy paper's own numbers: transits observed, instruments used and the uncertainty on the gems.

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  1. [1]

    Researchers found that WASP-17b's atmosphere has a chemical composition and temperature that shift between dayside and nightside according to theory and modelling.

    Reported Supported Source: Space (Robert Lea)2 sources— create a free account to open themView cited source
  2. [2]

    Alderson said: "Theory predicts that the morning and the evening sides should have a strong temperature difference".

    Reported Supported Source: Lili Alderson, Cornell University, quoted by Space2 sources— create a free account to open themView cited source
  3. [3]

    Alderson said WASP-17b was "pretty much bang-on what we thought it would be".

    Reported Supported Source: Lili Alderson, Cornell University, quoted by Space2 sources— create a free account to open themView cited source

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Sources

1 independent publisher whose own reporting we read for this story.

  1. space.com

    1 article · October 16, 2026

    Scientists find 'gemstones' in atmosphere of bizarre, scorching-hot 'marshmallow' exoplanet

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