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What did NASA and ESA’s September 3, 2026 Hubble image reveal about LHA 120 N44 in the Large Magellanic Cloud—including its location about 160,000 light years away in Dorado; the roughly 210 by 140 light year superbubble formed by central stars’ winds and supernovae; the compress
NASA and ESA’s September 3 Hubble image portrays N44 (LHA 120 N44) as a vast, active stellar nursery in the Large Magellanic Cloud: a nearby in cosmic terms laboratory for seeing how massive stars reshape gas and trigger further star format It lies about 160,000 light years away in the constellation Dorado. [1][8] N...
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Key takeaways
- NASA and ESA’s September 3 Hubble image portrays N44 (LHA 120 N44) as a vast, active stellar nursery in the Large Magellanic Cloud: a nearby in cosmic terms laboratory for seeing how massive stars reshape gas and trigger further star format
- It lies about 160,000 light years away in the constellation Dorado.
- [1][8] N44’s dominant feature is a roughly 210 by 140 light year central “superbubble,” excavated by winds from massive central stars and by their supernova explosions.
- [7][9] That feedback swept gas into a dense surrounding shell, where compression appears to have initiated a newer generation of stars.
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NASA and ESA’s September 3 Hubble image portrays N44 (LHA 120-N44) as a vast, active stellar nursery in the Large Magellanic Cloud: a nearby-in-cosmic-terms laboratory for seeing how massive stars reshape gas and trigger further star formation. It lies about 160,000 light-years away in the constellation Dorado. 1
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N44’s dominant feature is a roughly 210-by-140-light-year central “superbubble,” excavated by winds from massive central stars and by their supernova explosions.
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That feedback swept gas into a dense surrounding shell, where compression appears to have initiated a newer generation of stars. Stars in the shell may be up to about five million years younger than those in the bubble’s interior—evidence consistent with sequential, feedback-driven star formation.
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Hubble observing program #14689, led by Dimitrios Gouliermis, catalogued nearly 500,000 stars in and along the line of sight to N44. About 30,000 are pre-main-sequence stars—young objects not yet powered by sustained hydrogen fusion.
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The image’s bright blue area is a particularly hot, intensely star-forming zone, while the smaller round bubble at upper right is N44F, a separate bubble shaped by a hot massive star’s radiation and stellar winds.
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N44 is part of an emission-nebula complex about 1,000 light-years across. Because the Large Magellanic Cloud has comparatively low metallicity—fewer elements heavier than helium—N44 offers a nearby analogue for investigating star formation under chemical conditions more like those in the early universe.
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NASA and ESA’s September 3 Hubble image portrays N44 (LHA 120 N44) as a vast, active stellar nursery in the Large Magellanic Cloud: a nearby in cosmic terms laboratory for seeing how massive stars reshape gas and trigger further star format
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NASA and ESA’s September 3 Hubble image portrays N44 (LHA 120 N44) as a vast, active stellar nursery in the Large Magellanic Cloud: a nearby in cosmic terms laboratory for seeing how massive stars reshape gas and trigger further star format It lies about 160,000 light years away in the constellation Dorado.
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[1][8] N44’s dominant feature is a roughly 210 by 140 light year central “superbubble,” excavated by winds from massive central stars and by their supernova explosions.