Warwick Researchers Predict Green and Pink Hues in White Dwarfs

Warwick Researchers Predict Green and Pink Hues in White Dwarfs

University of Warwick researchers said that some white dwarf stars could appear green or pink because atmospheric sodium, calcium and other elements absorb specific wavelengths, a finding reported in their latest study. The claim builds on earlier work by the same team that modeled the visible colors of white dwarfs and identified a range of possible hues.

They previously reported the discovery of WD J1330+6435, a white dwarf about 326 light-years away whose spectrum shows a pale green glow caused by sodium from accreted planetary debris, marking the first confirmed green star. Their modeling also highlighted the pinkest known white dwarf.

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University of Warwick Dr. Mark Hollands Professor Boris Gänsicke RAS Techniques and Instruments

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University of Warwick, United Kingdom

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Հոկտեմբեր 22, 2026
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Researchers report that the white dwarf WD J1330+6435 shows a pale green hue due to atmospheric absorption of certain wavelengths, marking the first convincing identification of a green star.

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Researchers at the University of Warwick have discovered a white dwarf star that appears green due to atmospheric sodium and calcium, marking the first known green star in the galaxy.

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Researchers led by the University of Warwick report that white dwarf WD J1330+6435, 326 light-years away, exhibits a green hue due to sodium from planetary debris, marking the first confirmed green star.

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Researchers at the University of Warwick have modeled the visible colors of white dwarf stars and identified a range of hues—from green to pink—based on atmospheric composition and density.

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