'We've never had this kind of look at an exploded star before.'
© X-ray: NASA/CXC/SAO; Optical: NASA/ESA/STScI; IR: NASA/ESA/CSA/STScI/Milisavljevic et al., NASA/JPL/CalTech; Image Processing: NASA/CXC/SAO/J. Schmidt and K. ArcandThis image of the supernova remnant Cassiopeia A combines data from NASA's Chandra, James Webb, Hubble and Spitzer space telescopes.
The bizarre,
grinch-like wisp of green light dubbed the Green Monster, first seen last year snaking through the glowing remnants of an exploded star,
belongs to a blast wave bordering the debris field, a new study reveals.
Last April, NASA's
James Webb Space Telescope (JWST or Webb) photographed the
unusual "wall of emission" in front of Cassiopeia A (or Cas A), an expanding shell of hot gas roughly 11,000 light-years from Earth whose light first reached us 340 years ago. For the past year, astronomers have been trying to explain its origin and presence in the well-studied
supernova remnant.
The new image, unveiled on Monday (Jan. 8) at the American Astronomical Society conference being held in New Orleans and online, combines the observing powers of Webb, as well as NASA's
Hubble, Spitzer and Chandra space telescopes, to feature Cas A in unprecedented detail. The ball of light, which stretches for 10 light-years, appears infused with red clouds, revealing dust likely warmed as it resides within gas that was heated up to millions of degrees. White, green and orange light streaks sprinkled throughout offer a cosmically messy, breathtaking new view of the stellar debris.
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