Astronomy

Astronomers find the first known green star: a white dwarf about 280 light-years away

A University of Warwick study finds that the white dwarf WD J1330+6435 would glow chartreuse green up close, because sodium from swallowed rocky debris absorbs its orange light.

The Helix Nebula, a glowing orange and blue ring of gas around a white dwarf, with the headline Astronomers find the first known green star

Photograph: The Helix Nebula, a planetary nebula with a white dwarf at its center, in a Hubble and Kitt Peak composite. It is not WD J1330+6435; no image of that star’s color exists. Cropped, with No Ground headline overlay. Credit: NASA/STScI (PIA18164).

The first known green star sits about 280 light-years from Earth. You can’t see the color with your own eyes. Through a telescope it’s just a faint dot, so no one has ever seen its color directly. But a new study from the University of Warwick says that if you could get close enough to see its disk, the white dwarf WD J1330+6435 would look chartreuse green.

The paper, “Any colour you like: The diverse chromaticities of white dwarfs,” is published in the journal RAS Techniques and Instruments. Warwick announced it on Oct. 15. As far as the researchers know, “no other star, living or dead, has ever been credibly reported as green, making this the first known genuinely green star in the Galaxy.”

Hubble image of planetary nebula NGC 2440, glowing clouds of gas around a white dot, the white dwarf at its center
A white dwarf is what’s left when a star like the Sun runs out of fuel. Here, the white dot at the center of planetary nebula NGC 2440 is a young white dwarf, surrounded by the gas its star cast off. Credit: NASA, ESA, and K. Noll (STScI); Acknowledgment: The Hubble Heritage Team (STScI/AURA) (GSFC_20171208_Archive_e000210).

Which star is green?

WD J1330+6435 is a cool white dwarf, the dense leftover core of a dead star. Warwick says it is roughly 4,000 degrees Celsius. It has also swallowed rocky material from its old planetary system, which added calcium, lithium and sodium to its atmosphere.

The same Warwick-led team analyzed the star in a 2021 Nature Astronomy paper. There they spotted lithium in its spectrum from the Sloan Digital Sky Survey (SDSS) and put it 87 ± 7 parsecs away. That’s about 280 light-years.

Artist’s illustration of a white dwarf surrounded by a disk of dust, with an asteroid falling toward it
Artist’s illustration, not WD J1330+6435: a NASA illustration of a white dwarf pulling in rocky debris from its old planetary system. That’s the same process that put sodium and calcium into the green star’s atmosphere. Credit: NASA, ESA, and G. Bacon (STScI) (GSFC_20171208_Archive_e001500).

Why does it look green?

Most stars glow like “perfect radiators,” so temperature sets their color: cooler stars look orange, Sun-like stars white, and the hottest pale blue. White dwarfs can break that rule because their atmospheres are extremely dense. The coolest ones reach about 1 gram per cubic centimeter, roughly the density of water. Under that pressure, trace elements absorb light across a much wider range of colors than usual.

In WD J1330+6435, sodium absorbs orange light and calcium absorbs violet. According to the paper, that leaves the star’s light peaking around 500 nanometers, in the green.

“The traces of sodium in the atmosphere of this white dwarf absorb the orange part of the spectrum, leaving behind a ghostly green glow. Imagine standing on a planet and looking up at a green star. It feels like something out of science fiction.” — Dr. Mark Hollands, University of Warwick, who led the work

How did astronomers find it?

Nobody photographed it in green. The team worked out each star’s color from its spectrum, its light split up by wavelength. They ran those spectra through a model of human color vision. For cool stars like this one, they used observed SDSS spectra.

The paper adds a caveat: the star’s spectrum is “somewhat noisy,” so its exact shade “may differ slightly in reality.” The team’s older 2021 model of the star gave a similar hue, which the authors say gives them confidence that it really is green. Two other white dwarfs in the study, WD J0851+1543 and WD J1351+2645, also come out green, but much paler.

Hubble view of the dense globular star cluster 47 Tucanae, with young white dwarfs identified
White dwarfs are small and faint. Hubble had to hunt for young ones among the crowded stars of globular cluster 47 Tucanae. Credit: NASA, ESA, and H. Richer and J. Heyl (University of British Columbia); acknowledgement: J. Mack (STScI) and G. Piotto (University of Padova) (GSFC_20171208_Archive_e000722).

Pink, yellow and the reddest star yet

Green isn’t the only surprise. Carbon-rich white dwarfs tend toward pink or purple, while those polluted by asteroid and comet debris lean yellow. The team says WD J1011+2845, 48 light-years away, may be the reddest star ever recorded. Its glow is a deep salmon pink.

Among the 151 white dwarfs within about 65 light-years of Earth, five had unusual colors: two yellow and three pink. That suggests roughly one in 30 white dwarfs shines in an odd color. The rest came out white, with a median color temperature of about 6,800 kelvin. That corrects a common belief that white dwarfs are usually blue. Hot blue ones are brighter, so surveys see more of them.

“One in thirty might not sound like a huge fraction, but across the entire population of white dwarfs in the Universe, that is still a lot of oddly coloured stars out there.” — Professor Boris Gänsicke, University of Warwick
The Ring Nebula seen by Hubble and the Large Binocular Telescope, a glowing ring of gas around a central dying star
The Ring Nebula: the glowing gas shell around an old, dying, Sun-like star. Credit: NASA, ESA, C.R. Robert O’Dell (Vanderbilt University), G.J. Ferland (University of Kentucky), W.J. Henney and M. Peimbert (National Autonomous University of Mexico); Large Binocular Telescope data: David Thompson (University of Arizona) (GSFC_20171208_Archive_e001464).

What’s confirmed and what isn’t

  • Confirmed: the peer-reviewed paper, its authors (Mark A. Hollands, Boris T. Gänsicke, Pier-Emmanuel Tremblay and Detlev Koester), the star’s name, its roughly 4,000°C temperature, and its sodium-, calcium- and lithium-rich atmosphere.
  • Modeled, not seen: the green color is calculated from the star’s spectrum. No one has seen it by eye.
  • Distance: 87 ± 7 parsecs (about 280 light-years), from the team’s 2021 Nature Astronomy paper. The new release doesn’t give a distance.

No Ground. Stay curious.

Tags: white dwarf, green star, WD J1330+6435, University of Warwick, astronomy