Ancient Arabic poetry from the 12th century describes a bright star in the constellation Cassiopeia, which recent research suggests was a supernova observed around 1181-1182, providing valuable historical data on stellar explosions.
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Scientists have identified the remains of a supernova that appeared in 1181, known as SN 1181, as the nebula Pa 30 in the constellation Cassiopeia. This discovery was made through the analysis of its chemical composition, suggesting it resulted from a sub-luminous Type Iax event, a special type of supernova. The nebula's central star, one of the hottest in the Milky Way, and its unique properties make it an exceptional opportunity for studying rare explosions. This finding sheds light on a historical astronomical event and provides valuable insights into the nature of supernovae.
Scientists have discovered the remnant of a rare supernova explosion that appeared in the night sky in 1181, providing a new spectacular view of the event that was visible for 185 days. The composite image, created using data from various telescopes, shows a nearly circular nebula with a central star in the constellation Cassiopeia. X-ray observations reveal the full extent of the nebula, while studies of its composition suggest it was formed in a sub-luminous Type Iax event, a special kind of supernova resulting from the merger of two white dwarf stars. This discovery offers a unique opportunity for studying rare explosions and the formation of "zombie" stars.