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Sulfur in the Clouds: Webb Spies a Super-Neptune's Atmosphere ⚡ экспресс

Original: "JWST-TST DREAMS: Sulfur dioxide in the atmosphere of the Neptune-mass planet HAT-P-26 b from NIRSpec G395H transmission spectroscopy"
arXiv:2509.16082 · 2025-09-19 · CC BY 4.0 · ⏱ 1 min · Exoplanets
The James Webb Space Telescope has sniffed out sulfur dioxide—the gas that smells like burnt matches—in a warm Neptune's atmosphere for the first time, proving that stellar ultraviolet light 'cooks' chemistry on planets across a range of temperatures.
Abstract

Using transmission spectroscopy with JWST (NIRSpec G395H) during a single transit, the atmosphere of exoplanet HAT-P-26 b (mass ~18.6 M⊕, radius ~6.33 R⊕) was studied. Water vapor (ln B = 4.1), carbon dioxide (ln B = 85.6), and sulfur dioxide (ln B = 13.5) were detected with high confidence, along with weak hints of hydrogen sulfide and carbon monoxide (ln B < 0.5). The detection of SO₂ on a warm super-Neptune fills the gap between previous detections on hot Jupiters and sub-Neptunes, demonstrating the role of non-equilibrium photochemistry in planetary atmospheres with temperatures below 1000 K. The measured abundances of carbon, oxygen, and sulfur indicate a metallicity around 10 times solar and a sub-solar C/O ratio. Retrieved molecular abundances within 2σ are consistent with self-consistent photochemical models. The enhanced CO₂ abundance and potential H₂S signal are sensitive to thermal structure, clouds, or vertical mixing.

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When starlight passes through a planet's atmosphere, it's as if it's sifted through a sieve: different gases filter out specific colors. By catching these leaks, the James Webb telescope identifies the chemical makeup like a connoisseur discerning a dish's ingredients by its aroma. This transit spectroscopy method was first used by David Charbonneau.

The exoplanet HAT-P-26 b turned out to be a veritable cosmic kitchen. In its air, Webb found water and carbon dioxide, but the key ingredient was sulfur dioxide—the very stuff that gives burnt matches their smell. Before, SO₂ was only 'cooked up' in the hellish heat of hot Jupiters or chilly sub-Neptunes, but now it's been spotted in lukewarm temperatures for the first time. This means the star's ultraviolet light runs the kitchen on planets cooler than 1000 °C.

A surprising twist: the amount of sulfur dioxide follows a strict recipe—the higher the metallicity (abundance of heavy elements), the more SO₂, but only up to 30 times the Sun's value; then the burner nearly shuts off. Theorists had predicted such a rich brew.

🎯 Astronomers call all elements heavier than hydrogen and helium 'metals,' so carbon, oxygen, and sulfur are metals to them too.

🎬 In the series 'The Expanse,' characters scan the atmospheres of distant planets for signs of life; now, such diagnostics are a reality for dozens of worlds.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterAlbert Einstein
Tags
exoplanet JWST spectroscopy Water carbon Standard Model
Laws
Doppler effectgravitational lensingNoether's theoremKepler's third lawMaxwell's equationsPlanck's law
Original: arXiv:2509.16082 · CC BY 4.0 · bridge42worlds