A team led by Mark Hollands at the University of Warwick modeled how white dwarf stars would appear to the human eye, using existing spectral data and a model of human color vision. Most stars behave like perfect radiators, with color set almost entirely by temperature. But the researchers found that the extreme density of white dwarfs allows trace elements such as carbon, calcium and sodium to interact with dense helium plasma, producing a much wider range of colors.
"It turns out these incredibly dense stars can produce colors nobody expected, and some of them genuinely surprised me," Hollands said.
The colors fall into groups based on atmosphere. Carbon-rich white dwarfs tend to be pink or purple, those polluted by debris from asteroids or comets tend to be yellow, and those with hydrogen and helium atmospheres appear more cyan or blue.
The most striking result is WD J1330+6435, described as the first documented green star. "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. "Imagine standing on a planet and looking up at a green star. It feels like something out of science fiction."
The researchers may also have found the reddest star ever seen. White dwarf WD J1011+2845, 48 light-years from Earth, has a deep convection zone that brings carbon to the surface, squeezing almost all of its light beyond 600 nanometers and producing a salmon-pink glow unlike any ordinary star.
Most white dwarfs remain white. In a representative sample of 151 white dwarfs within 65 light-years of Earth, only five showed unusual colors: three pink and two yellow. The typical white dwarf has a color temperature of about 6,800 Kelvin, which looks white to the human eye.