Not All White Dwarfs Are White: Atmospheric Chemistry Can Tint Some Pink, Yellow, or Green

The average white dwarf really is white.
Co-author Boris Gänsicke noted that oddly colored white dwarfs remain the exception, even as five of 151 broke the rule.
Mark

So the headline is that white dwarfs aren't always white. Why does that matter beyond being a curiosity?

Mimi

Because color was assumed to track temperature alone. If dense atmospheres and trace elements like carbon can shift it, color carries chemical information too.

Luke

Careful there. The reporting says the findings could give new insight into stellar formation and evolution. That's a possibility, not something shown yet.

Mark

Fair. What did they actually find?

Mimi

Of 151 white dwarfs within 20 parsecs, five weren't white: three pink, two yellow. That's about 3.3 percent.

Luke

And that's a small sample, from modeling. The 3.3 percent describes those 151 stars. Stretching it to white dwarfs across the cosmos is an extrapolation.

Mark

Gänsicke said one in thirty is still a lot of stars.

Mimi

He also said the median white dwarf really is white. Both statements sit together.

Luke

The element links are worth noting too: carbon gives pink or purple, hydrogen and helium cyan or blue, planetary debris green. But the article reports no green or cyan among the five named stars, so those come from the broader findings, not specific examples I can check.

Mark

And brown dwarfs?

Mimi

Hollands says absorption by sodium, potassium, and titanium oxide can alter their color, and earlier work suggested violet.

Luke

That's a prior conclusion by other astronomers, relayed secondhand. Interesting, but not part of this study's results.

  • Five of 151 nearby white dwarfs refuse to look white, glowing yellow or pink against a rule that long seemed fixed.
  • Researchers test whether dense atmospheres and trace elements like carbon, calcium, and sodium can bend the light that escapes these stellar remnants.
  • Carbon-rich atmospheres tint white dwarfs pink or purple, while planetary debris leaves some glowing green.
  • The team's work, published in RAS Techniques and Instruments, now points to brown dwarfs as possible rule-breakers too.
  • Color may soon become a new instrument for reading the atmospheres of distant stars.

For as long as astronomers have looked at the heavens, they have assumed that a star's color speaks only of its heat, a slow fading from red through white to blue. A new study led from the University of Warwick now shows that a small share of the dead, dense stars called white dwarfs refuse that simple reading, glowing pink or yellow instead. The finding reminds us that even the most ordinary-seeming light carries the traces of what lies in the air around it, and that the sky keeps offering quiet corrections to our tidiest rules.

A star is supposed to glow according to its temperature and nothing else. Cool objects burn red and orange, hotter ones fade toward white, and the hottest turn pale blue. A new study led by the University of Warwick reports that some white dwarfs break that rule and appear pink or yellow instead.

The work, published in RAS Techniques and Instruments, was explained to Universe Today by lead author Dr. Mark Hollands, a Warwick postdoctoral researcher. He offered a familiar image: a blacksmith's metal shifting from red to orange as it heats. A true blackbody, glowing only by temperature, can produce only red, orange, white, and blue. White dwarfs have reason to depart from that, because their atmospheres are far denser than the Sun's. The team asked whether elements such as carbon, calcium, or sodium could change the light that escapes, and studied 151 white dwarfs within 20 parsecs, about 65 light-years, of Earth.

Five of them showed other colors: two yellow and three pink, roughly 3.3 percent of the sample. Dr. Boris Gänsicke, a Warwick physics professor and co-author, noted that one in thirty may sound small, yet across the whole cosmos it still means many oddly colored stars, while the typical white dwarf remains genuinely white.

The study also links composition to tint. Carbon makes white dwarfs look pink or purple, cooler hydrogen and helium atmospheres lean cyan or blue, and planetary debris often yields green.

Hollands suggests brown dwarfs may break the rule as well. These substellar objects emit mostly infrared light, yet some reaches the optical range, and absorption by sodium, potassium, and titanium oxide can shift their colors. Past observers have described some as violet. What comes next remains open, but color may prove a new way to read the atmospheres of stars.

A star is supposed to glow according to its temperature, and nothing else. Cooler objects burn red and orange, a hot one fades toward white by about 6000 kelvin, and hotter still, as most of the light shifts into the ultraviolet, it turns pale blue. A new study led by the University of Warwick reports that some white dwarfs break that rule, and appear pink or yellow instead.

The work was published in RAS Techniques and Instruments. Its lead author, Dr. Mark Hollands, a postdoctoral researcher at Warwick, explained the baseline to Universe Today with an image from the forge: a blacksmith's metal moves from red to orange as it heats. For a true blackbody, an idealized object whose glow depends only on temperature, red, orange, white and blue are the only colors possible.

White dwarfs have a reason to depart from that. Their atmospheres are far denser than those of main-sequence stars like the Sun. The team wanted to know whether elements such as carbon, calcium, or sodium in those atmospheres could change the light that escapes. To find out, they used computer models to study 151 white dwarfs within 20 parsecs, about 65 light-years, of Earth.

Five of the 151 showed colors other than white: two were yellow and three were pink. The researchers read that as the combined effect of a dense atmosphere and particular elements within it. The five make up roughly 3.3 percent of the sample.

Dr. Boris Gänsicke, a professor in Warwick's Department of Physics and a co-author, put the number in perspective. One in thirty might not sound like much, he said, but across all the white dwarfs in the Universe it is still a great many oddly colored stars. He added that the median across a representative population still shows that the average white dwarf really is white.

The study also links particular compositions to particular tints. Carbon in the atmosphere makes a white dwarf look pink or purple. Cooler white dwarfs with hydrogen and helium atmospheres tend toward cyan or blue. Those whose atmospheres carry debris from their original planetary system are typically green.

Hollands says white dwarfs may not be the only objects to defy the rule. Brown dwarfs, substellar objects too cool to fuse hydrogen in their cores but able to fuse deuterium, put out most of their radiation in the infrared, though some still emerges at optical wavelengths. Because they too can have dense atmospheres, absorption by sodium, potassium, and molecules such as titanium oxide can push their colors away from blackbody values. Astronomers who have studied their appearance in the past have concluded that brown dwarfs can look violet.

What comes next is open. The findings could offer new insight into how stars form and evolve, and the suggestion that brown dwarfs also break the color rule points toward color as another way to read the atmospheres of stars.

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 colored stars.
— Dr. Boris Gänsicke, University of Warwick
Brown dwarfs can also have dense atmospheres, so absorption from sodium, potassium and titanium oxide can alter their colors away from blackbody colors.
— Dr. Mark Hollands, University of Warwick (paraphrased)
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