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June 16, 2025

Image: Hubble studies a spiral's supernova scene

This NASA/ESA Hubble Space Telescope image features the barred spiral galaxy IC 758. Credit: ESA/Hubble & NASA, C. Kilpatrick
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This NASA/ESA Hubble Space Telescope image features the barred spiral galaxy IC 758. Credit: ESA/Hubble & NASA, C. Kilpatrick

This serene spiral galaxy hides a cataclysmic past. The galaxy IC 758, shown in this NASA/ESA Hubble Space Telescope image, is situated 60 million light-years away in the constellation Ursa Major.

Hubble captured this image in 2023. IC 758 appears peaceful, with its soft blue spiral arms curving gently around its hazy barred center. However, in 1999, astronomers spotted a powerful explosion in this galaxy. The supernova SN 1999bg marked the dramatic end of a star far more massive than the sun.

Researchers do not know exactly how massive this star was before it exploded, but will use these Hubble observations to measure the masses of stars in SN 1999bg's neighborhood. These measurements will help them estimate the mass of the star that went supernova. The Hubble data may also reveal whether SN 1999bg's progenitor star had a companion, which would provide additional clues about the star's life and death.

A supernova represents more than just the demise of a single star鈥攊t's also a powerful force that can shape its neighborhood. When a massive star collapses, triggering a supernova, its outer layers rebound off its shrunken core. The explosion stirs the interstellar soup of gas and dust out of which form. This interstellar shakeup can scatter and heat nearby gas clouds, preventing new stars from forming, or it can compress them, creating a burst of new star formation. The cast-off layers enrich the , from which new stars form, with manufactured in the core of the .

Provided by NASA

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The spiral galaxy IC 758, located 60 million light-years away, experienced a supernova (SN 1999bg) in 1999, marking the end of a massive star. Hubble observations aim to estimate the progenitor's mass and possible companion. Supernovae like this enrich the interstellar medium with heavy elements and can either trigger or inhibit new star formation by affecting surrounding gas and dust.

This summary was automatically generated using LLM.