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The Abell 370 galaxy cluster was captured by the Hubble Space Telescope. That isn't a new feat. An image of an infant supernova that exploded just hours after the star's death was discovered by a team of astronomy researchers.

The supernova is exactly what the team was looking for when they were searching. We can see it from our vantage point, even though it's hidden behind Abell 370, because of the effects of gravity.

There are clues to a dark secret contained in a Cosmic "spider web" spied by the Hubble telescope.

Through a phenomenon called gravitational lensing, three different moments in a far-off supernova explosion were captured in a single snapshot by NASA's Hubble Space Telescope.

The left panel shows the portion of Abell 370 where the multiple images of the supernova appeared. Panel A, a composite of Hubble observations from 2011 to 2016, shows the locations of the multiply-imaged host galaxy after the supernova faded. Panel B, a Hubble picture from December 2010, shows the three images of the host galaxy and the supernova at different phases in its evolution. Panel C, which subtracts the image in Panel B from that in Panel A, shows three different faces of the evolving supernova. Using a similar image subtraction process for multiple filters of data, Panel D shows the different colors of the cooling supernova at three different stages in its evolution. (Image credit: NASA, ESA, STScI, Wenlei Chen (UMN), Patrick Kelly (UMN), Hubble Frontier Fields)

Inputting the Hubble data into models and analyzing details in the images, Chen and his team determined that the original star that had gone supernova was likely a red supergiant with a diameter 530 times that of the sun.

The first image in the series was taken by Hubble just six hours after the explosion and the second and third were taken about 10 and 30 days after the explosion.

Due to the expansion of the universe, the supernova's age was estimated to be around 11 billion years old, making it one of the oldest and most distant ones.

The team hopes that their modeling will help the study of distant supernovas. They would be able to progress the study of stellar populations.

The paper was published in the journal Nature.

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