Astronomy & Space

Superbubble in the Large Magellanic Cloud

How the science connects

SupernovaeNebulaeStellar wind

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NASA's Hubble Space Telescope has captured an image of N44, a nebula in the Large Magellanic Cloud featuring a massive "superbubble" measuring approximately 210 by 140 light-years across. The superbubble is a vast central void created by powerful stellar winds and supernova explosions from young, massive stars at its center, which expelled the gas from which they originally formed. The nebula is characterized by this central cavity surrounded by a shell of dense, dusty gas.


This observation helps astronomers understand how massive stars shape their surrounding environments through stellar feedback processes, including winds and supernovae. Studying superbubbles provides insights into stellar evolution, star formation regulation, and the cycling of matter in galaxies.


Blue and orange stars shine through a wispy bubble of gas; the center is mostly clear, but blue and gray tendrils snake throughout most of the rest of the image. The background of the image is filled with other stars.
NASA, ESA/Hubble, D. Gouliermis

NASA’s Hubble Space Telescope captures a photogenic nebula, N44, in the Large Magellanic Cloud in this Sept. 3, 2026, image. N44 is dominated by two features: a vast central void and a shell of dense, dusty gas. The central void is a ‘superbubble’ spanning roughly 210 by 140 light-years across. The glittering stars at the center of the void are responsible for its creation; through their powerful stellar winds and explosive supernovae, these stars expelled much of the gas from which they were born.

Read more about this cosmic vista.

Image credit: NASA, ESA/Hubble, D. Gouliermis

Source: Superbubble in the Large Magellanic Cloud