Archivo de imágenes de Hubble

Ilustración de supernova y estrella remanente

This artist's illustration shows supernova 2013ge, with its companion star at lower right. The companion star is impacted by the blast wave from the supernova, but not destroyed. Over time astronomers observed the ultraviolet (UV) light of the supernova fading, revealing a nearby...

Fecha
Jan 1, 2022
Misión
Hubble Space Telescope
ID de archivo
hubblesite-images-2022-011-01fzt6ynv6yz11h3zzfb496vb5
Por

This artist's illustration shows supernova 2013ge, with its companion star at lower right. The companion star is impacted by the blast wave from the supernova, but not destroyed. Over time astronomers observed the ultraviolet (UV) light of the supernova fading, revealing a nearby second source of UV light that maintained brightness. The theory is that the two massive stars evolved together as a binary pair, and that the current survivor siphoned off its partner's outer hydrogen gas shell before it exploded. Eventually, the companion star will also go supernova. 

Credits

Artwork

NASA, ESA, Leah Hustak (STScI)

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Fuente

La imagen y el material de referencia se acreditan al archivo oficial de la misión enlazado a continuación.

Ver en NASA.gov

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