science & techESA/Hubble

A dying star's wind blasts a glowing gas shell at 150,000 km/h

the gist

Hen 2-427, better known as WR 124, is a Wolf-Rayet star, a type of very hot, massive star that throws off its outer layers in a fierce stream. The clumps of gas it ejects travel at more than 150,000 kilometres an hour, and together they have built the nebula M1-67 around it. The pair sits in the constellation Sagitta, about 15,000 light-years away. The nebula is estimated to be no more than 10,000 years old, which is very young by astronomical standards. Hubble's image shows the star and its shell in fresh detail after the picture was reprocessed with modern software.

how it works

Wolf-Rayet stars are massive stars that have burned through much of their hydrogen and now shed their outer layers through powerful stellar winds. The ejected material escapes into space and is lit up by the star's intense radiation, which makes it glow. Because the gas moves fast, it collides with and sculpts earlier material into shells and clumps. Hubble's reprocessed view makes the structure of these clumps visible.

so what

Wolf-Rayet winds are one way that heavy elements forged inside massive stars return to space, where they can become part of later stars and planets. Seeing one at close range helps astronomers test models of how the most massive stars lose material before they die.

the bigger pattern

Wolf-Rayet stars are a rare class, with only a few hundred known in the Milky Way, and they represent a late stage in the life of very massive stars. Many such stars are expected to end their lives as supernovae, and their winds seed the surrounding space with carbon, nitrogen and oxygen.

fun fact

The category is named after the astronomers Charles Wolf and Georges Rayet, who identified the first such stars in 1867.

ESA/Hubble · CC BY 4.0

Image: ESA/Hubble & NASA Acknowledgement: Judy Schmidt ( geckzilla.com )