Webb Locates Dust Reservoirs in Two Supernovae

Summary
The finding suggests supernovae are likely suppliers of dust to early, young galaxies.
Supernovae, the explosive deaths of stars, are some of the universe’s biggest bursts of energy and light. When they erupt, one supernova can shine even brighter than an entire galaxy.
It’s a fitting reason for NGC 6946, located 22 million light-years away from Earth, to be nicknamed the Fireworks Galaxy. In the past century, nearly a dozen supernovae have been observed flashing in the arms of this galaxy.
This includes Supernova 2004et and Supernova 2017eaw, which researchers are now studying with the James Webb Space Telescope’s MIRI (Mid-Infrared Instrument). Their findings have been surprising—MIRI detected large amounts of dust within the ejecta of each of these objects. The mass found by researchers supports the theory that supernovae played a key role in supplying dust to the early universe.
Full Article
Researchers using NASA’s James Webb Space Telescope have made major strides in confirming the source of dust in early galaxies. Observations of two Type II supernovae, Supernova 2004et (SN 2004et) and Supernova 2017eaw (SN 2017eaw), have revealed large amounts of dust within the ejecta of each of these objects. The mass found by researchers supports the theory that supernovae played a key role in supplying dust to the early universe. Dust is a building block for many things in our universe – planets in particular. As dust from dying stars spreads through space, it carries essential ...Visit NASA Science to view the full news release including article text and associated Webb imagery, graphics, scientific visualizations, videos, captions, text descriptions, and other information.
News releases highlighting the discoveries of NASA’s James Webb Space Telescope are produced for NASA by the Space Telescope Science Institute (STScI) in Baltimore, Maryland, under NASA Contract NAS5-03127. News release content is developed by the News Team in STScI’s Office of Public Outreach.
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