Giant stars can be a prime example of the “live fast, die young” principle. Unlike our own Sun, which will shine for billions of years, more massive stars can burn off their fusion fuel in just a few million years before shedding their outer layers and exploding in supernovae.
NASA this week presented a rare image from the James Webb Space Telescope (JWST) of one of these stellar giants, Wolf-Rayet stars in the last, fleeting stages of their lives. Named WR 124, it lies in the constellation Sagittarius and lies about 15,000 light-years from Earth. The dying star has at least 30 times the mass of our Sun, but it is rapidly contracting, expelling hot gas into the cold vacuum of space.
“We caught it before,” explains Anthony Moffat, a retired astrophysicist who previously observed WR 124 with the Hubble Space Telescope and was not involved in the recent JWST measurements. Moffat has been studying Wolf-Rayet stars for decades. “This is the youngest person I know,” he says. The colorful cloud in the image, somewhat erroneously called a planetary nebula, is only a few thousand years old. Now, “the nebula is hugging the star,” he says. But as time passes, it will bloom outward in the form of expanding shells or rings of gas and dust.
Stars are natural fusion reactors, glowing with the energy released when hydrogen is fused to form helium atoms. Once massive stars burn off all their hydrogen, they begin to convert helium into heavier elements through a more energetic fusion reaction, causing powerful stellar winds. Rushing at speeds of more than 150,000 kilometers per hour, these winds carry the outer layers of the star with them, throwing huge volumes of gas and dust into space.
This gas glows with infrared radiation, the same type of light that JWST detects. Astrophysicists have created an impressive image by combining data from two JWST instruments, a near-infrared camera (NIRCam) and a mid-infrared (MIRI) instrument. The Hubble Space Telescope, which predominantly collects light in the optical range, has taken pictures of WR 124 before, but the JWST observations show the star’s growing nebula in stunning new detail.
“Personally, the most exciting part of this image is that we are capturing a rare phenomenon, i.e. a Wolf-Rayet star, at a level of detail that can only be achieved with JWST,” says Macarena Garcia Marin, an astrophysicist. The European Space Agency, which works with MIRI.
Only massive stars can go through the Wolf-Rayet phase, and not all of them. Astronomers have calculated that there are only 1,000 Wolf-Rayet stars in our galaxy—about one in every 100 million. The nearest one is about 1,000 light-years away in the star system Gamma Velorum, visible from the Southern Hemisphere. According to Moffat, Wolf-Rayet stars could be a million times brighter than the Sun. “What they lack in numbers, they make up for in light,” he adds.
“This dust is spreading into space and will eventually create planets. And that’s how we got here, really,” NASA astrophysicist Amber Strone said during a panel discussion at the 2023 South by Southwest conference in Austin, Texas, where the image was first unveiled. “I think this is one of the most beautiful concepts in all of astronomy.”
But while we are all made of stardust, there seems to be a lot more to the universe than scientists can explain with a simple cataloging of obvious sources. “It’s always exciting to be in science when our theories don’t match up with our observations — and that’s where we are right now with the dust,” Strawn says. These detailed pictures of the decoupling of a dying star as it forges heavy elements and produces copious amounts of dust could help scientists refine their understanding of this underlying process.
Someday—thousands or even millions of years from now, but essentially tomorrow on a galactic scale—WR 124 will explode in a spectacular supernova. In addition to a large amount of dust and heavy elements, a black hole may remain after the explosion. But physicists don’t have a good way to predict this with certainty. Moffat suggests that the supernova remnant could instead turn into a neutron star, the last stop before the collapsing star reaches the ultimate oblivion of a black hole. Without a glimpse from some observatory that remains for us in the distant future, we may never know what will happen to WR 124. But in any case, its ultimate fate remains the same, written in stars and planets that are still not formed from his generous gift of cosmic dust.