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Source: Peer-reviewedRAS Techniques and Instruments2 sources

Scientists Calculated the True Colors of Dead Stars. One Came out Green.

Space

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A Hubble Space Telescope image of the white dwarf Stein 2051 B as a bright white point with diffraction spikes, with a much fainter background star below it.
The white dwarf Stein 2051 B, about 17 light-years from Earth, is the bright point at center; the smaller dot below it is a background star roughly 5,000 light-years farther away (illustrative). The Warwick colors come from spectra run through a model of human color vision, not from pictures like this one."Hubble Astronomers Develop a New Use for a Century-Old Relativity Experiment to Measure a White Dwarf’s Mass" by NASA's Marshall Space Flight Center, via nasa, BY-NC · CC-BY-NC-2.0

A University of Warwick team has calculated what white dwarf stars would look like to the human eye, and reports that one of them, WD J1330+6435, would appear green. Nobody has photographed one: no white dwarf is close enough for its color to be seen directly, so the team ran spectra that telescopes already collect through a model of human color vision.

A spectrum is normally read for a star's temperature and its chemical makeup; in the team's account, it also carries the color the star would show up close. The paper was published Oct. 15, 2026, in RAS Techniques and Instruments.

Density is what breaks the usual rule that a star's color follows its temperature, with cooler stars orange and the hottest ones pale blue. Mark Hollands and colleagues at Warwick report that the coolest white dwarf atmospheres can be about as dense as water, and that at those densities traces of carbon, calcium or sodium absorb light across much wider bands, producing stars that would look yellow, green, cyan, pink or purple.

A Chandra X-ray image showing a bright point source with a fainter one just above it, against a speckled magenta field.
In X-rays the white dwarf Sirius B, the brighter of the two points at center, outshines its much larger companion Sirius A (illustrative). The pink and white tones are a brightness scale for X-ray light, which the eye cannot see. "Sirius A and B: A Double Star System in Canis Major (NASA, Chandra repost, 09/26/00)" by NASA's Marshall Space Flight Center, via nasa, BY-NC

WD J1330+6435 is about 4,000 degrees Celsius and has pulled in rocky debris from its planetary system; sodium absorbs the orange part of its spectrum, leaving green. The claim of a first appears in Warwick's announcement, not in the paper: as far as the team is aware, no other star, living or dead, has ever been credibly reported as green.

Across the 151 white dwarfs within about 65 light-years of Earth, the median color temperature is about 6,800 K, which the eye reads as white. Five of them are unusually colored, two yellow and three pink, which the team extrapolates to roughly 1 in 30 white dwarfs.

"Yet if we take the median across a representative population of white dwarfs, we found that the average white dwarf really is white," said Boris Gänsicke of Warwick, a co-author of the paper.

The same models give the team a candidate for the reddest star on record: WD J1011+2845, where carbon dredged up from the core pushes nearly all of its light into the red.

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