NASA's Webb Uncovers Star Formation in Cluster's Dusty Ribbons

January 11, 2023 1:15PM (EST)Release ID: 2023-101
A star cluster within a nebula. The center of the image contains arcs of orange and pink gas that form a boat-like shape. One end of these arcs points to the top right of the image, while the other end points toward the bottom left. Another plume of orange and pink gas expands from the center to the top left of the image. To the right of this plume is a large cluster of white stars. There are more of these white stars and galaxies of different sizes spread throughout the image.

Summary

New Data Provides Insights Into an Early Era of Star Formation

By peering into a well-known star cluster within the Small Magellanic Cloud, Webb’s NIRCam instrument has revealed many new pockets of star formation that have never been seen. Further, new structures appear in this image that provide a window into the stars feeding within.

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Full Article

NGC 346, one of the most dynamic star-forming regions in nearby galaxies, is full of mystery. Now, it is less mysterious with new findings from NASA’s James Webb Space Telescope.  NCG 346 is located in the Small Magellanic Cloud (SMC), a dwarf galaxy close to our Milky Way. The SMC contains lower concentrations of elements heavier than hydrogen or helium, which astronomers call metals, compared to the Milky Way. Since dust grains in space are composed mostly of metals, scientists expected there would be low amounts of dust, and that it would be hard to detect. New data from Webb reveals ...

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