{"id":16637,"date":"2026-10-28T14:01:50","date_gmt":"2026-10-28T18:01:50","guid":{"rendered":"https:\/\/zobi.alcowep.com\/bourtagshdrevxnls658739\/webb-sees-turbulent-star-nursery\/"},"modified":"2026-10-28T14:01:50","modified_gmt":"2026-10-28T18:01:50","slug":"webb-sees-turbulent-star-nursery","status":"publish","type":"post","link":"https:\/\/zobi.alcowep.com\/bourtagshdrevxnls658739\/webb-sees-turbulent-star-nursery\/","title":{"rendered":"Webb Sees Turbulent Star Nursery"},"content":{"rendered":"

Webb Sees Turbulent Star Nursery<\/h2>\n

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\"A<\/a><\/figure>
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ESA\/Webb, NASA & CSA, E. Sabbi, M. Zamani (ESA\/Webb); Acknowledgement: M. H. \u00d6zsara\u00e7<\/div>\n<\/figcaption><\/div>\n<\/div>\n<\/div>\n

In this Webb image released on Oct. 22, 2026, we see a turbulent cauldron of star formation filled with dense clumps of gas. This region is named N159 and is located 161,000 light-years away in the Large Magellanic Cloud, one of the satellite galaxies orbiting the Milky Way galaxy.<\/p>\n

This region has a lower metallicity (proportion of elements that are heavier than helium and hydrogen) than the Milky Way, giving astronomers an opportunity to learn more about conditions found in the early universe and how stars formed under those conditions.<\/p>\n

Read more about N159.<\/a><\/p>\n

Image credit: ESA\/Webb, NASA & CSA, E. Sabbi, M. Zamani (ESA\/Webb); Acknowledgement: M. H. \u00d6zsara\u00e7<\/em><\/p>\n

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\nHQ Web Team <\/p>\n","protected":false},"excerpt":{"rendered":"

In this Webb image released on Oct. 22, 2026, we see a turbulent cauldron of star formation filled with dense clumps of gas. This region is named N159 and is located 161,000 light-years away in the Large Magellanic Cloud, one of the satellite galaxies orbiting the Milky Way galaxy. This region has a lower metallicity [\u2026] Continue reading → <\/span><\/a><\/p>\n

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