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Protostellar jets and outflows, which appear in gold, shoot from dust-enshrouded, nascent stars.
• A “blow-out” erupts at the top-center of the ridge, spewing gas and dust into the interstellar medium.
• An unusual “arch” appears, looking like a bent-over cylinder.
This period of very early star formation is difficult to capture because, for an individual star, it lasts only about 50,000 to 100,000 years – but Webb’s extreme sensitivity and exquisite spatial resolution have chronicled this rare event.
Located roughly 7,600 light-years away, NGC 3324 was first catalogued by James Dunlop in 1826.
Visible from the Southern Hemisphere, it is located at the northwest corner of the Carina Nebula (NGC 3372), which resides in the constellation Carina. The Carina Nebula is home to the Keyhole Nebula and the active, unstable supergiant star called Eta Carinae.
NIRCam was built by a team at the University of Arizona and Lockheed Martin’s Advanced Technology.
Original image: https://images.nasa.gov/details/carina_nebula
I do not claim authorship of the images or sound. All rights belong to the developers and publishers.
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