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Birthday · July 3, 1996

Superbubbles in the LMC

July 3, 1996

The light from the farthest visible stars set out on its journey long before your first birthday.

Superbubbles in the LMC

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APOD published July 3, 1996. Credit: C. Smith (U. Michigan), Curtis Schmidt Telescope, CTIO, Chile. A publication-date match, not a photo taken on your date. Independent of NASA.

Behind the image

Superbubbles in the LMC

Original APOD · July 3, 1996

Why is there a hole in the center of this nebula? A leading explanation is that it is caused by the stellar winds from the stars that live there. Stars - including the Sun - expel electrons, protons, and other charged ions in a steady stream - the stellar wind. The wind ions push out the normal hydrogen and helium gas found glowing in the nebula. This star forming region is located in the Large Magellanic Cloud. This picture is a composite of three separate photographs, each sensitive to only one specific color of light - a color that distinguishes a specific chemical element. It is currently not known why stars emit a stellar wind.

Image credit: C. Smith (U. Michigan), Curtis Schmidt Telescope, CTIO, Chile

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