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Scientists were stunned after discovering the record-breaking supernova BGR



Scientists handle the lifecycle of various stars quite well. They know the kinds of stars that are likely to die in fiery supernova explosions, and they know that not all supernova are created equal. Nevertheless, space holds many unresolved secrets, and a new study published in The Astrophysical Journal shows that scientists had questioned their understanding of the supernova after observing an explosion that was so massive was that they initially thought their instruments were broken. [19659002] The explosion in question called SN2016iet was first discovered in 2016, but it took another three years for astronomers to truly understand what they saw.

"When we first saw how extraordinary SN201

6iet responded to me, my reaction was, whoa – was something terribly wrong with our data? "Harvard grad Sebastian Gomez, lead author of the newspaper, said in a statement. "After a while, we discovered that SN2016iet is an incredible puzzle located in a previously unreported galaxy a billion light-years from Earth." was created by a star that is 200 times as massive as our own sun. Researchers believe it lost a whopping 85 percent of its mass during its brief existence, ultimately leading to a colossal detonation. The tremendous amount of material that the star itself delivered along with the supernova explosion created a sight that left scientists scratching their heads for years.

"Everything about this supernova looks different – its change in brightness over time, its spectrum, the galaxy it is in, and even where it is in its galaxy," explains Professor Dr. Edo Berger. "We sometimes see supernovae that are unusual in one way but otherwise normal. This one is unique in every way.

For the future, the team plans to continue watching SN2016iet and hopefully learn more about its past and future. This is made easier by the fact that the blast was incredibly bright and located in a bare area of ​​the sky, so we may be able to teach even more.

Image Source: NASA / ESA


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