{"id":3579,"date":"2026-03-14T23:08:40","date_gmt":"2026-03-14T23:08:40","guid":{"rendered":"https:\/\/news678.top\/?p=3579"},"modified":"2026-03-14T23:08:40","modified_gmt":"2026-03-14T23:08:40","slug":"webb-captures-red-dust-swirls-tracing-new-stars-forming-in-ngc-5134","status":"publish","type":"post","link":"https:\/\/news678.top\/?p=3579","title":{"rendered":"Webb Captures Red Dust Swirls Tracing New Stars Forming in NGC 5134"},"content":{"rendered":"

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\"James
NGC 5134 is a scenic spiral galaxy 65 million light-years away from where we live, which NASA\u2019s James Webb Space Telescope was fortunate enough to capture in stunning detail. The way this image was created is actually pretty cool: two of James Webb\u2019s devices combined their near-infrared and mid-infrared data to produce an extremely clear composite view.<\/p>\n


\"James
In the near-infrared view, you can see the light from the stars themselves, as well as clusters of young ones that are forming all over the place, which is how new stars develop in the cosmos. Meanwhile, the mid-infrared wavelengths reveal the warm dust intermingled throughout the galaxy\u2019s clouds, which gives it a slightly fuzzy appearance. The tightly coiled arms wrap around a very bright core that shines bright blue-white in the center, which is where the majority of the movement occurs. Then there are the delicate blue tones of the oval disk, which are actually a mix of all the light from the many stars in the backdrop. The brilliant crimson threads running along those arms indicate regions where gas and dust are accumulating. Then there are these orange clusters where the gas and dust are particularly dense, and the gaps in between show where it has been cleaned.<\/p>\n

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    \nStar clusters can be seen as bright little points of light imbedded in the arms, while some of the smaller points of light in the surrounding space are actual galaxies that are far away. Scientists examine things like NGC 5134 because they are quite close to us, allowing them to analyze the overall mechanism that keeps galaxies active in the first place. The way it works is that these massive clouds of gas compress in on themselves, forming new stars of varying sizes, while some of the largest ones burn through their fuel quickly and then explode, spreading all heavy components into space. Meanwhile, stars like our own Sun shed their layers over time as they age, and the returned material is mixed back into the galaxy to produce the next generation of stars.<\/p>\n