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Explanation: The flowing trails of dust toward Corona Australis, the constellation of the Southern Crown, are visible here because not because they glow, but because they absorb and reflect. The dust appears bluer when seen near bright stars because it preferentially reflects blue light. The densest knots of dust are so thick that no background stars or interior stars can be seen through them. These knots indicate molecular clouds filled with cool gas where future stars will likely form. The above image spans about 5 degrees while the reflection nebula lies about 500 light-years distant.
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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: reflection nebula - molecular cloud
Publications with words: reflection nebula - molecular cloud
See also:
- APOD: 2026 May 19 Á NGC 2170: The Angel Nebula
- APOD: 2026 April 7 Á IC 4592: The Blue Horsehead Reflection Nebula
- APOD: 2026 February 2 Á Orion: The Running Man Nebula
- NGC 1333: Stellar Nursery in Perseus
- APOD: 2026 January 28 Á M78: Reflecting Blue in a Sea of Red
- NGC 7023: The Iris Nebula
- A Dark Seahorse in Cepheus

