Astronomer Have Spotted Two Distant Stars Touching, And The Results Could Be Catastrophic

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Witness VFTS 352, the hottest and most enormous “over contact binary” star system ever found. The two stars, which are so adjacent that they’re actually touching, feature a mutual mass 57 times that of our Sun. Astronomers say it’s a distinctive stellar relationship that will end in a rather histrionic finish. This remarkably large contact binary was spotted by an international group of astronomers using the ESO’s Very Large Telescope. Situated 160,000 light-years away, it’s consist of two twin stars that orbit each other in a slight over 24 hours. The stars are so close to each other that their surfaces overlap, making a stellar bridge between them. Extraordinarily, their cores are only 7.4 million miles (12 million kilometers) apart (that’s approximately 20 lunar distances). With a mass 57 times greater than our Sun, and a boiling surface temperature more than 40,000 degrees Celsius, it’s the hottest and most gigantic over contact binary ever spotted.
Image Credit: (ESO/L. Calçada)

The details of this astonishing finding were published in Astrophysical Journal. This kissing couple is exclusive in that both stars are approximately equal in terms of size. Other alike systems feature a star that’s considerably larger than the other, ultimately resulting in the cannibalization of the smaller star. But these two stars, with their approximately equal mass, may truly be sharing their cosmic material with each other. Astronomers believe that the twin stars of VFTS 352 are exchanging about 30 percent of their stellar stuff, a phenomenon identified as “internal mixing.”

Due to their unstable nature, binary systems like these obviously don’t last long. Astronomers are truly quite lucky to have spotted this system, which can meet its end in one of two ways.

The first potential consequence is the unification of the two stars, which would likely yield a swiftly rotating, and probably magnetic, enormous single star.

The second possibility is clarified by the chief theoretical astrophysicist in the group, Selma de Mink of University of Amsterdam: “If the stars are mixed well enough, they both remain compact and the VFTS 352 system may avoid merging. This would lead the objects down a new evolutionary path that is completely different from classic stellar evolution predictions. In the case of VFTS 352, the components would likely end their lives in supernova explosions, forming a close binary system of black holes. Such a remarkable object would be an intense source of gravitational waves.”
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