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Science Widely confirmed5 publishers 2 min read Published Updated

Warwick's color model turns the white dwarf WD J1330+6435 chartreuse green

Warwick astronomers calculate that some white dwarfs would look green, pink, cyan, yellow or purple, including what may be the first green star. The colors are computed from spectra, since no white dwarf is near enough to see.

The Scientist · Science desk

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Illustration accompanying Warwick's color model turns the white dwarf WD J1330+6435 chartreuse green
Generated illustration

What happened

  • The study, led by Mark Hollands and published in RAS Techniques and Instruments, finds that certain white dwarfs seen up close would shine in colors well beyond white and pale blue.
  • The coolest white dwarf atmospheres reach about 1 gram per cubic centimeter, roughly the density of water and millions of times denser than the sun's photosphere.
  • Carbon-rich white dwarfs come out pink or purple, those polluted with asteroid and comet debris lean yellow, and cooler hydrogen-helium ones often look cyan or pale blue.
  • WD J1330+6435, at roughly 4,000 degrees Celsius, carries calcium, lithium and sodium from accreted rocky material and appears chartreuse green in the team's models.
  • WD J1011+2845, 48 light-years away, produces a deep salmon-pink glow and may be the reddest star ever recorded.

Why it matters

  • What it limits constraint Nobody can check these colors by eye, so each one is only as good as the measured spectrum and the color-vision model that produced it.
  • What it limits constraint For the coolest white dwarfs with trace elements in the atmosphere, color stops tracking temperature the way it does for perfect radiators.
  • What doesn't add up contradiction Phys.org calls WD J1330+6435 the first known genuinely green star, while Discover says only that it could be; the 'first' is the researchers' own reading of the literature.

No white dwarf is close enough for its color to be seen directly, so the team computed it [5]. The inputs were spectra that astronomers already collect routinely, run through a model of human color vision to get the color an eye would register [5][6]. A spectrum already records a star's temperature and its chemical makeup, and this pipeline adds a third output, color [7].

The baseline the study departs from is the perfect radiator. "Most stars, including most white dwarfs, behave like 'perfect radiators,' so their color is set almost entirely by temperature. But nobody had really looked into what else might be possible for white dwarfs," said Dr. Mark Hollands, who led the work [2].

For white dwarfs the departure comes from the atmosphere. At densities near that of water, trace carbon, calcium and sodium interact with the dense helium plasma around them, and that interaction broadens the band of colors they absorb compared with what they would absorb at lower densities [4].

In the green case the absorbing element is sodium. "The traces of sodium in the atmosphere of this white dwarf absorb the orange part of the spectrum, leaving behind a ghostly green glow," Hollands said [10].

The reddest case has a different cause. WD J1011+2845 has a deep convection zone that has lifted carbon from its core to its surface, and the resulting carbon molecules push almost all of the star's light to wavelengths beyond 600 nanometers [14].

Discover, which attributes the Hollands quotes to a Warwick press release [12], notes that most of the white dwarfs seen are still white [11]. In our view the green is a credible prediction for that one star, conditional on the measured spectrum and the color-vision model behind it. The thing this doesn't tell you is how many white dwarfs fall outside the white-to-blue range, or how uncertain the computed colors are, and neither report says.

What to watch

  • The paper's own uncertainty on the computed colors and the number of stars behind each color group, which would show how firm the green is.
  • Whether other teams recompute WD J1330+6435's color from separate spectra or a different color-vision model and also land on green.
  • Whether searches of existing spectra for cool, sodium-rich white dwarfs turn up a second green candidate.

Clarity's read

What the record supports and how the coverage leans. The claims behind it follow.

Reality

Evidence60
Adoption
Not scored
Hype gap+25
Incentives30
Confidence68

Perspective Coverage

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Claim ledger

Ranked by verification strength, evidence, and original report placement.

  1. [1]

    The study, published in RAS Techniques and Instruments and led by Dr. Mark Hollands of the University of Warwick, shows that if viewed up close, certain white dwarfs would shine in colors such as green, pink, cyan, yellow and purple.

    Reported Supported Source: phys.org, reporting University of Warwick researchView cited source
  2. [2]

    "Most stars, including most white dwarfs, behave like 'perfect radiators,' so their color is set almost entirely by temperature. But nobody had really looked into what else might be possible for white dwarfs," said Dr. Mark Hollands.

    Reported Supported Source: Dr. Mark Hollands, Warwick Prize Fellow, University of WarwickView cited source
  3. [3]

    The coolest white dwarf atmospheres can reach around 1 gram per cubic centimeter, roughly the density of water and millions of times denser than the sun's photosphere.

    Reported Supported Source: phys.org, reporting the Warwick studyView cited source
  4. [4]

    At these densities, trace elements such as carbon, calcium and sodium interact with the surrounding dense helium plasma and absorb light across a wider range of colors than they would at lower densities, shifting a star's color away from the orange, white and blue of a perfect radiator.

    Reported Supported Source: phys.org, reporting the Warwick studyView cited source
  5. [5]

    No white dwarf is close enough for its color to be seen directly, so the team calculated it from data astronomers already collect routinely: a star's spectrum.

    Reported Supported Source: phys.org, reporting the Warwick studyView cited source
  6. [6]

    The team ran the spectra through a model of human color vision to reveal what color each star's light would appear as to the eye.

    Reported Supported Source: phys.org, reporting the Warwick studyView cited source
  7. [7]

    A spectrum can reveal not just a star's temperature or its chemical makeup, but its true color as well.

    Reported Supported Source: phys.orgView cited source
  8. [8]

    Applying the method across the sky, the team found colors fall into distinct groups linked to atmospheric contents: carbon-rich white dwarfs are typically pink or purple, those enriched with debris from asteroids and comets tend toward yellow, and cooler mixed hydrogen-helium white dwarfs often take on a cyan or pale blue tinge.

    Reported Supported Source: phys.org, reporting the Warwick studyView cited source
  9. [9]

    WD J1330+6435, roughly 4,000 degrees Celsius, has accreted rocky material from its planetary system, enriching its atmosphere with calcium, lithium and sodium, and appears chartreuse green in the team's models.

    Reported Supported Source: phys.org, reporting the Warwick studyView cited source
  10. [10]

    "The traces of sodium in the atmosphere of this white dwarf absorb the orange part of the spectrum, leaving behind a ghostly green glow," Hollands said.

    Reported Supported Source: Dr. Mark HollandsView cited source
  11. [11]

    Most of the white dwarfs seen are still white.

    Reported Supported Source: Discover magazineView cited source
  12. [12]

    Discover attributes the Hollands quotations to a Warwick press release.

    Reported Supported Source: Discover magazineView cited source
  13. [13]

    WD J1011+2845, a nearby white dwarf just 48 light-years from Earth, produces a deep salmon-pink glow and may be the reddest star ever recorded.

    Reported Supported Source: phys.org, reporting the Warwick studyView cited source
  14. [14]

    WD J1011+2845 has a deep convection zone that has lifted carbon from its core to its surface, and the resulting carbon molecules distort its light so heavily that almost all of it is squeezed into wavelengths beyond 600 nanometers.

    Reported Supported Source: phys.org, reporting the Warwick studyView cited source
  15. [15]

    As far as the researchers are aware, no other star, living or dead, has ever been credibly reported as green, making this the first known genuinely green star in the galaxy.

    Reported Insufficient Source: phys.org, reporting the Warwick researchers' own assessmentView cited source
  16. [16]

    Discover writes that WD J1330+6435, which appeared chartreuse green in the team's models, could be the first genuine green star in the galaxy.

    Reported Insufficient Source: Discover magazine, citing the Warwick press releaseView cited source

Sources

5 independent publishers whose own reporting we read for this story.

  1. discovermagazine.com

    1 article · October 14, 2026

    White Dwarf Stars "Can Produce Colors Nobody Expected," Including What May Be the First Green Star
  2. livescience.com

    1 article · October 16, 2026

    Astronomers discover the first-ever green star, plus the reddest 'white dwarf' ever seen
  3. phys.org

    1 article · October 14, 2026

    Green, pink and purple: Astronomers reveal the surprising true colors of white dwarf stars
  4. popsci.com

    1 article · October 15, 2026

    Astronomers discover first green star and the reddest star ever recorded
  5. space.com

    1 article · October 15, 2026

    Astronomers discover the 1st ever green star, a cosmic zombie just in time for Halloween

Topics and entities

Topics

  • Astronomy research
  • Stellar color and spectroscopy
  • White dwarfs

Entities