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Supernova warning system could alert the world to exploding stars, scientists say


A recent understanding of the last days of supergiant stars can have given scientists the clues they should predict when those stars will go supernova, collapsing in among the largest explosions known within the universe.

Scientists already knew that red supergiant stars nearing the tip of their lives have large amounts of expelled dust and gas often called circumstellar material, or CSM, in orbit around them near the time they explode and die. What wasn’t known was if this CSM was blown out from the star over a protracted period leading as much as its fiery death, or if it was expelled in a big and sudden cough just before going supernova.

Now, in a recent paper accepted for publication within the Monthly Notices of the Royal Astronomical Society and currently available on the educational paper preprint service Arxiv, researchers from the University of Liverpool and the University of Montpellier have shown that it’s the latter — dying stars must cough up the CSM near their deaths, and so the looks of that material could function an early warning sign of their coming demise.

“Regardless of the mechanism for generating this CSM, it must do it on a really rapid timescale,” the researchers write within the paper. “Specifically, the build-up of the CSM must occur inside a yr of core-collapse.”

Core-collapse supernovae occur in stars eight times as massive because the Sun or larger, typically red supergiants similar to Betelgeuse. Found around 640 light years from Earth within the constellation Orion, Betelgeuse is about 11 times more massive than the Sun, and if centered in our Solar System, would stretch out to the orbit of Jupiter.

All stars produce light and energy by fusing lighter elements into heavier ones. Stars just like the Sun primarily fuse hydrogen into helium, but some stars, especially very large ones, can proceed to fuse heavier elements similar to oxygen and silicon, until eventually they’ve fused just about all of their fuel into iron.

Even with the tremendous heat and pressure available at the guts of a red supergiant star, iron can’t be fused into heavier elements, and the star’s thermonuclear fires dimmed, it could now not push outward with enough force to beat its own gravity: The star collapses in on itself, triggering an enormous supernova explosion.

The researchers checked out the before and after photos of a certain variety of supernova, the Type IIp, which stay vivid within the sky longer than other such explosions. What they present in all their examples was a considerable amount of CSM present prior to the supernova, but they didn’t see significant dimming of the celebrities years prematurely, ruling out the likelihood that the CSM had amassed over an extended time period.

That signifies that for super red giants like Betelgeuse a minimum of, a significant construct up of CSM could possibly be a warning sign that a cataclysm is on the way in which.

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