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Credit & Copyright: Craig Stocks
(Utah Desert Remote Observatories)
Explanation:
What's causing the commotion in the Tadpole Nebula?
Star
formation.
Dusty emission in the
Tadpole Nebula, IC 410,
lies about 12,000 light-years away in the northern constellation of the
Charioteer
(Auriga).
The cloud of glowing gas is over 100 light-years across,
sculpted by
stellar winds and radiation from embedded
open star cluster
NGC 1893.
Formed in the interstellar cloud
a mere
4 million years ago, bright newly formed cluster stars are seen
all around the star-forming nebula.
Notable on the lower-right of the featured image are two relatively dense streamers
of material trailing away from the nebula's central regions.
Potentially sites of ongoing star formation in
IC 410, these
cosmic tadpole
shapes are about 10 light-years long.
The image was processed
highlighting the emission from sulfur (red), hydrogen (green), and oxygen (blue)
gas -- but with the
stars digitally removed.
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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: star formation
Publications with words: star formation
See also:
- NGC 1893 and the Tadpoles of IC 410
- Star Factory Messier 17
- APOD: 2023 August 28 Á Star Formation in the Pacman Nebula
- APOD: 2023 July 10 Á Stars, Dust and Nebula in NGC 6559
- NGC 1333: Stellar Nursery in Perseus
- APOD: 2023 March 21 Á Dark Nebulae and Star Formation in Taurus
- An Unusual Globule in IC 1396