|
Explanation: NGC 3603 is home to a massive star cluster, thick dust pillars, and a star about to explode. The central open cluster contains about 2000 bright stars, each of which is much brighter and more massive than our Sun. Together, radiations from these stars are energizing and pushing away surrounding material, making NGC 3603 one of the most interesting HII regions known. NGC 3603 is about 20,000 light-years away, and the region shown is about 20 light-years across. Possibly most interesting about this recently released, representative-color picture are the large number of dim stars visible. These stars are less massive than our Sun, demonstrating that great numbers of low-mass stars also form in active starburst regions.
|
January February March April May June July August September October November December |
| ||||||||||||||||||||||||||||||||||||||||||||||||
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: star cluster - star formation - HII region - open cluster
Publications with words: star cluster - star formation - HII region - open 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 August 7 Á The Double Cluster in Perseus

