|
Credit & Copyright: Anglo-Australian Telescope
Board
Explanation:
The photogenic
M16 shown above is composed of a
young star cluster and a
spectacular emission nebulae
lined with distinct regions of
interstellar dust.
Most of the stars in the
cluster
can be seen offset just above and to the right of the photograph's center.
This type of star cluster is called an "open" or "galactic" cluster and
typically has a few hundred young bright members. The redness of the
surrounding
emission nebula gas is caused by
electrons recombining with hydrogen nuclei, while the dark regions are
dust lanes that absorb much of
the radiation that enters it. The dust absorbs so much light it allows
astronomers to determine which stars are inside the nebula and which are in
the foreground.
|
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: dust - M 16 - open cluster
Publications with words: dust - M 16 - open cluster
See also:
- Open Star Clusters M35 and NGC 2158
- APOD: 2025 February 25 Á M41: The Little Beehive Star Cluster
- APOD: 2025 February 11 Á The Spider and the Fly
- Young Stars, Dark Nebulae
- APOD: 2024 October 29 Á NGC 602: Stars Versus Pillars from Webb
- APOD: 2024 October 22 Á M16: Pillars of Star Creation
- APOD: 2024 September 29 Á Seven Dusty Sisters