The Hubble Area Telescope caught a supernova because it explodes
The Hubble Area Telescope caught a supernova because it explodes
Speak about being in the fitting place on the proper time.
2010 Hubble Space Telescope took some footage of the Abell 370 cluster of galaxies. That in itself is hardly a groundbreaking feat. However a staff of astronomers systematically reviewing archival Hubble photos found one thing unimaginable in these photos: a picture of a new child. supernova which exploded about 11.5 billion years in the past, taken a number of hours after the star died.
A staff led by Wenlei Chen, a postdoctoral researcher on the College of Minnesota, was on the lookout for gravitational lensing transients, and that is precisely what a supernova is. It’s hidden behind Abell 370, nonetheless, as a result of mild is bent across the galaxy cluster by its gravitational pull; gravitational lenses — we are able to truly see it from our line of sight, albeit distorted.
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By inputting the Hubble information into fashions and analyzing particulars within the photos, similar to brightness and coloration, Chen and his staff decided that the unique star that had was a supernova was doubtless red supergiant roughly 530 occasions bigger in diameter Sun.
Additionally they discovered that the primary image of the three was taken by Hubble simply six hours after the explosion after the core collapsed, whereas the second and third had been taken about 10 and 30 days after the explosion, respectively.
And because the supernova has a excessive redshift – wavelengths of sunshine are stretched and shifted in direction of the crimson aspect of the spectrum expansion of the universe — Astronomers have been capable of estimate the supernova’s age to be roughly 11.5 billion years previous, making it one of many oldest and most distant supernovae we have ever seen.
The staff hopes their modeling will assist them research comparable distant supernovae if they’re discovered. The discoveries, in flip, will be capable of advance the research of stellar populations at excessive redshift.
This analysis was primarily based on a paper published in a journal Nature (opens in new tab) as we speak.
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