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Source: PreprintarXiv1 source

A Nearby Giant Planet's Methane Points to a Very Cold Birthplace

Space

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A Webb mid-infrared image showing the giant planet epsilon Indi Ab as a small orange point to the left of its masked host star, against blue speckles of residual starlight.
A separate Webb mid-infrared image of the same system: the planet is the orange point at left, and the position of the star behind the central mask is marked. The colors are assigned rather than what the eye would see."Exoplanet Epsilon Indi Ab (MIRI image) (weic2421a)" by ESA/Webb, NASA, CSA, STScI, E. Matthews (Max Planck Institute for Astronomy), via Wikimedia Commons, CC BY 4.0

Astronomers using the James Webb Space Telescope have measured how much heavy hydrogen sits in the atmosphere of a nearby giant planet, and the answer resembles Uranus and Neptune rather than Jupiter and Saturn. Jerry W. Xuan of the University of California, Santa Barbara, and colleagues put the deuterium-to-hydrogen ratio of the planet, epsilon Indi Ab, at about 4.4 atoms per 100,000, roughly twice the figure for Jupiter, Saturn and the gas cloud the Sun itself formed out of. They report the finding in a preprint that has not been peer reviewed.

Deuterium is a heavy form of hydrogen, nearly all of it made in the Big Bang. The authors write that a giant planet's ratio can therefore pin down the kind of solid material the planet swallowed as it grew, because very cold ice and organic matter carry far more deuterium than the gas around them.

A Webb graphic pairing a small infrared image of two planets beside their masked star with a jagged brightness curve marked as a carbon monoxide band.
What the evidence looks like: a near-infrared spectrum of a different young giant planet, taken with the same instrument mode, and a carbon monoxide band picked out in it (illustrative). "Beta Pictoris System (NIRSpec IFU Image and Spectrum) - 55395514865" by James Webb Space Telescope, via Wikimedia Commons, CC BY 4.0

The preprint, posted Nov. 6, 2026, carries a note on its arXiv listing saying it is under review. The team reports detecting deuterated methane, methane built with heavy hydrogen, at a strength 48 times the noise in the data, in spectra from Webb's near-infrared spectrograph. Epsilon Indi Ab is a cold planet of six to eight times Jupiter's mass, roughly 4 billion years old, orbiting a nearby star.

Jupiter's and Saturn's deuterium ratios match the gas the Sun formed from, while Uranus's and Neptune's are about twice as high, a difference long attributed to the icy bodies those two took in. The authors call the resemblance striking, because epsilon Indi Ab is a gas giant whose carbon, oxygen, nitrogen and sulfur come out enriched at roughly the same level as Jupiter's.

The pale blue disk of Neptune against black space, crossed by faint cloud bands, with a darker oval and bright white clouds near the middle.
Our own ice giant, imaged by a passing spacecraft Aug. 20, 1989. Neptune and Uranus hold about twice the heavy hydrogen of Jupiter and Saturn, and that is the level the new reading matches (illustrative). "Neptune - Voyager 2 (29347980845)" by NASA / JPL / Voyager-ISS / Justin Cowart, via Wikimedia Commons, Public domain

To end up with the deuterium it has, the authors write, the planet must have gathered solids at least 30 times richer in deuterium than a typical Solar System comet. Ratios that high have been reported for the interstellar comet 3I/ATLAS and for organic molecules in star-forming regions. Their reading is that the planet was built from pristine material formed somewhere very cold, and that Webb measurements of more cold planets would test it.

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