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    Home»Space»Hubble Unveils the Supernova That Illuminated a Galaxy
    Space

    Hubble Unveils the Supernova That Illuminated a Galaxy

    By ESA/HubbleDecember 23, 20243 Comments2 Mins Read
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    Spiral Galaxy NGC 337
    NGC 337’s portrait by Hubble reveals a galaxy alive with stars at different stages, from seasoned stars at its core to newcomers at its edges, with the highlight being supernova SN 2014cx, a fascinating stellar explosion monitored even years after its peak brilliance. Credit: ESA/Hubble & NASA, C. Kilpatrick

    Explore the dynamic life of the spiral galaxy NGC 337 as captured by the Hubble Space Telescope, featuring a mix of old and new stars and the site of the stunning supernova SN 2014cx.

    This week’s featured image from the Hubble Space Telescope showcases the spiral galaxy NGC 337, located approximately 60 million light-years away in the constellation Cetus, also known as The Whale.

    The stunning image merges observations captured in two different wavelengths, revealing the galaxy’s striking features. Its golden-hued center glows with the light of older stars, while its vibrant blue edges shimmer with the energy of young, newly formed stars. Had Hubble captured NGC 337 about a decade ago, it would have witnessed an extraordinary sight among the galaxy’s hot blue stars — a dazzling supernova illuminating its outskirts.

    Named SN 2014cx, the supernova is remarkable for having been discovered nearly simultaneously in two vastly different ways: by a prolific supernova hunter, Koichi Itagaki, and by the All Sky Automated Survey for SuperNovae (ASAS-SN). ASAS-SN is a worldwide network of robotic telescopes that scans the sky for sudden events like supernovae. 

    Researchers have determined that SN 2014cx was a Type IIP supernova. The “Type II” classification means that the exploding star was a supergiant at least eight times as massive as the Sun. The “P” stands for plateau, meaning that after the light from the supernova began to fade, the level reached a plateau, remaining at the same brightness for several weeks or months before fading further. This type of supernova occurs when a massive star can no longer produce enough energy in its core to stave off the crushing pressure of gravity.

    SN 2014cx’s progenitor star is estimated to have been ten times more massive than the Sun and hundreds of times as wide. Though it has long since dimmed from its initial brilliance, researchers are still keeping tabs on this exploded star, not least through the Hubble observing program that produced this image.

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    Astronomy European Space Agency Hubble Space Telescope
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    3 Comments

    1. Anthony Scroggins on December 24, 2024 10:48 pm

      Awesome photos right there. I’d like to see more please?

      Reply
    2. William Douglas on December 25, 2024 11:14 am

      I love the site of possibilities ,that could be destinations in our future. Send more please.

      Reply
    3. Ramona on December 28, 2024 9:37 am

      12/28/24
      To Whom It Pertains;
      I am very interested in the topic as we are getting closer to the second coming of Christ.

      Reply
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