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Explanation: Bright-rimmed, flowing shapes gather near the center of this rich starfield toward the boarders of the nautical southern constellations Pupis and Vela. Composed of interstellar gas and dust, the grouping of light-year sized cometary globules is about 1300 light-years distant. Energetic ultraviolet light from nearby hot stars has molded the globules and ionized their bright rims. The globules also stream away from the Vela supernova remnant which may have influenced their swept-back shapes. Within them, cores of cold gas and dust are likely collapsing to form low mass stars, whose formation will ultimately cause the globules to disperse. In fact, cometary globule CG30 (upper right in the group) sports a small reddish glow near its head, a telltale sign of energetic jets from a star in the early stages of formation.
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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: cometary globule - star formation
Publications with words: cometary globule - star formation
See also:
- APOD: 2025 April 28 B Gum 37 and the Southern Tadpoles
- APOD: 2025 March 26 B Star Formation in the Pacman Nebula
- APOD: 2024 October 22 B M16: Pillars of Star Creation
- Star Factory Messier 17
- APOD: 2024 August 19 B IC 5146: The Cocoon Nebula
- APOD: 2024 July 16 B Cometary Globules
- Protostellar Outflows in Serpens