Zooming into Supernova Remnant Cassiopeia A | James Webb Space Telescope
This zoom-in video shows the relative location of supernova remnant Cassiopeia A (Cas A) in the sky. It begins with a ground-based photo by the late astrophotographer Akira Fujii. As it zooms into smaller portions of the sky, it fades into an image from the Digital Sky Survey. It ends by crossfading into an image of Cas A from NIRCam (Near-Infrared Camera) on NASA’s James Webb Space Telescope, with added borders from a NASA’s Hubble Space Telescope image.
A new high-definition image from NASA’s James Webb Space Telescope’s near-infrared camera (NIRCam) unveils intricate details of supernova remnant Cassiopeia A (Cas A), and shows the expanding shell of material slamming into the gas shed by the star before it exploded about 300 years ago.
The most noticeable colors in Webb’s newest image are clumps of bright orange and light pink that make up the inner shell of the supernova remnant. These tiny knots of gas, comprised of sulfur, oxygen, argon, and neon from the star itself, are only detectable by NIRCam’s exquisite resolution, and give researchers a hint at how the dying star shattered like glass when it exploded.
The outskirts of the main inner shell looks like smoke from a campfire. This marks where ejected material from the exploded star is ramming into surrounding circumstellar material. Researchers say this white color is light from synchrotron radiation. It is generated by charged particles traveling at extremely high speeds spiraling around magnetic field lines.
There are also several light echoes visible in this image. This is where light from the star’s long-ago explosion has reached, and is warming, distant dust, that is glowing as it cools down.
Credits:
Video: Alyssa Pagan NASA, ESA, CSA, STScI
Acknowledgments: Akira Fujii, David Malin, Digitized Sky Survey
Duration: 33 seconds
Release Date: Dec. 10, 2023
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