White dwarf stars are the dense, cooling cores left behind when low- to medium-mass stars run out of fuel. The first known examples glowed white or pale blue, leading to the name 'white dwarf'. But new research shows these stellar remnants can emit a surprising variety of visible-light colours.
Mark Hollands, an astronomer at the University of Warwick in the U.K. and the study's first author, said the findings challenge expectations. "Most stars, including most white dwarfs, behave like 'perfect radiators', so their colour is set almost entirely by temperature. But nobody had really looked into what else might be possible for white dwarfs," he said in a statement. "It turns out these incredibly dense stars can produce colours nobody expected, and some of them genuinely surprised me."
The variety of colours is possible because of the unusual density of white dwarfs. Cooler white dwarfs have a density of about 1 gram per cubic centimeter, similar to water on Earth, but they are also millions of times denser than the Sun's visible surface. These extreme conditions create a palette far beyond the typical white or pale blue glow.
The study, published Thursday 15 October, identifies the first ever green star and the reddest white dwarf ever recorded, though the researchers have not released specific names or catalog numbers for the objects. The findings suggest that the term 'white dwarf' may be a significant understatement.