Portrait In Ultraviolet

  • Released Tuesday, June 25, 2013
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About 200,000 light-years away, two small and misshapen galaxies orbit our own. Known as the Large and Small Magellenic Clouds, or LMC and SMC for short, they are the Milky Way’s closest neighbors, visible from Earth’s Southern Hemisphere as faint, glowing clouds in the night sky. Now, we can explore the breadth of these galaxies with the best ultraviolet view ever created. Astronomers wanted to view the LMC and SMC in ultraviolet because that light removes the distraction of normal stars like our sun, revealing only the hottest stars and star-formation regions. To create the mosaics, scientists stitched together thousands of individual snapshots taken by the Ultraviolet/Optical Telescope on NASA’s Swift satellite. Such detail allows us to study the evolution of each galaxy’s young stars in a single picture—an option that’s not available for own galaxy, which we must view from the inside. Watch the video to learn more.

The LMC contains the Tarantula Nebula, the most active star formation region of all the local galaxies.

The LMC contains the Tarantula Nebula, the most active star formation region of all the local galaxies.

The LMC is only one-tenth the size of our Milky Way, with only 1 percent of its mass. The SMC is even smaller.

The LMC is only one-tenth the size of our Milky Way, with only 1 percent of its mass. The SMC is even smaller.

This visible light mosaic shows the LMC and SMC in context with the plane of our own galaxy, the Milky Way.

This visible light mosaic shows the LMC and SMC in context with the plane of our own galaxy, the Milky Way.

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Credits

Please give credit for this item to:
NASA's Goddard Space Flight Center
UV light images courtesy of NASA/GSFC/Swift/S. Immler and M. Siegel, Penn State
Visible light images courtesy of Axel Mellinger, Central Michigan University

Release date

This page was originally published on Tuesday, June 25, 2013.
This page was last updated on Wednesday, May 3, 2023 at 1:52 PM EDT.