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#Scorpius

3 wallpapers tagged "Scorpius"

Pismis 24, HD 319718, NGC 6357
Pismis 24, HD 319718, NGC 6357
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Webb captured this sparkling scene of star birth in Pismis 24, a young star cluster about 5,500 light-years from Earth in the constellation Scorpius. This region is one of the best places to explore the properties of hot young stars and how they evolve. Read the full image description.

Image Credit: NASA, ESA, CSA, STScI; Image Processing: Alyssa Pagan (STScI)

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NGC 6072; IRAS F16097-3606
NGC 6072; IRAS F16097-3606
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NASA’s James Webb Space Telescope’s view of planetary nebula NGC 6072 in the near-infrared shows a complex scene of multiple outflows expanding out at different angles from a dying star at the center of the scene. There is one stretching from roughly 11 to 5 o’clock, another from 1 to 7 o’clock, and possibly a third from 12 to 6 o’clock. These outflows push gas toward the equatorial plane, forming a disk that appears to span from 9 to 3 o’clock. Astronomers suspect there is at least one other star interacting with the material cast off by the central dying star, creating the abnormal appearance of this planetary nebula. In this image, the red areas represent cool molecular gas, for example, molecular hydrogen. Read the full image description.

Image Credit: NASA, ESA, CSA, STScI

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Cat's Paw Nebula, NGC 6334
Cat's Paw Nebula, NGC 6334
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To celebrate NASA’s James Webb Space Telescope’s third year of highly productive science, astronomers used the telescope to scratch beyond the surface of the Cat’s Paw Nebula (NGC 6334), a massive, local star-forming region. This area is of great interest to scientists, having been subject to previous study by NASA’s Hubble and retired Spitzer space telescopes, as they seek to understand the multiple steps required for a turbulent molecular cloud to transition to stars. With its near-infrared capabilities and sharp resolution, the telescope “clawed” back a portion of a singular “toe bean,” revealing a subset of mini toe bean-reminiscent structures composed of gas, dust, and young stars. Webb’s view reveals a chaotic scene still in development: Massive young stars are carving away at nearby gas and dust, while their bright starlight is producing a bright nebulous glow represented in blue. This is only a chapter in the region’s larger story. The disruptive young stars, with their relatively short lifespans and luminosity, will eventually quench the local star formation process. The Cat’s Paw Nebula is located approximately 4,000 light-years away in the constellation Scorpius. To dive deeper into Webb’s image of the Cat’s Paw, embark on a narrated tour, get closer to the image, or read the press release. Additionally, learn more about Webb’s three years of science observations.

Image Credit: NASA, ESA, CSA, STScI

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