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Explanation: The massive stars of NGC 346 are short lived, but very energetic. The star cluster is embedded in the largest star forming region in the Small Magellanic Cloud, some 210,000 light-years distant. Their winds and radiation sweep out an interstellar cavern in the gas and dust cloud about 200 light-years across, triggering star formation and sculpting the region's dense inner edge. Cataloged as N66, the star forming region also appears to contain a large population of infant stars. A mere 3 to 5 million years old and not yet burning hydrogen in their cores, the infant stars are strewn about the embedded star cluster. In this false-color Hubble Space Telescope image, visible and near-infrared light are seen as blue and green, while light from atomic hydrogen emission is red.
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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
Publications with keywords: NGC 346 - star formation - star cluster
Publications with words: NGC 346 - star formation - star cluster
See also:
- APOD: 2025 December 28 Á NGC 1898: Globular Cluster in the Large Magellanic Cloud
- NGC 253: Dusty Island Universe
- APOD: 2025 October 21 Á IC 1805: The Heart Nebula
- Young Suns of NGC 7129
- APOD: 2025 October 8 Á NGC 7380: The Wizard Nebula
- APOD: 2025 December 9 Á The Heart of the Soul Nebula
- APOD: 2025 July 10 Á Lynds Dark Nebula 1251