Two-faced: Wacky white dwarf keeps its surface gases separate

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Two-faced: Wacky white dwarf keeps its surface gases separate
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The burnt-out star has one side composed of hydrogen and the other composed of helium. Astronomers have never seen anything like it.

The object is a white dwarf, an ancient core of a dead star. White dwarfs are small , clocking in at about the size of Earth, but with a mass similar to that of the Sun. Under their intense gravity, heavier elements sink towards the center of the dwarf, while lighter elements float nearer to its surface.The recently observed star’s lightest elements, helium and hydrogen, sit on the surface. But instead of mixing together, they take up opposite ends of the star.

The researchers followed up on the ZTF observations using the CHIMERA instrument at the Palomar Observatory and the HiPERCAM instrument on the Gran Telescopio Canarias. Observations of the dwarf using a spectrograph at the Keck Observatory revealed that helium and hydrogen appeared to be present on opposite sides of the object.An animation of the white dwarf nicknamed Janus, which has helium on one side and hydrogen on the other.

“We don’t know which of these theories are correct, but we can’t think of any other way to explain the asymmetric sides without magnetic fields,” Fuller said in the same release.Exactly how the magnetic fields are causing Janus’s juxtaposition is not certain, but observations of other magnetized white dwarfs may clarify things.

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