|
Credit & Copyright: Dean Carr
Explanation:
Why is the Lobster Nebula forming some of the most massive stars known?
No one is yet sure.
Cataloged as NGC 6357, the Lobster Nebula houses the open star cluster
Pismis 24 near its center --
a home to unusually bright and massive stars.
The overall
blue glow
near the inner star forming region results from the
emission of
ionized
hydrogen gas.
The surrounding nebula,
featured here,
holds a complex tapestry of gas,
dark dust, stars still forming, and newly born stars.
The intricate patterns are caused by complex interactions between
interstellar
winds,
radiation pressures,
magnetic fields, and
gravity.
NGC 6357 spans about 400 light years and lies about 8,000
light years away toward the constellation of the
Scorpion.
Free Download:
2019 APOD Calendar (v5)
|
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: emission nebula - star formation
Publications with words: emission nebula - star formation
See also:
- APOD: 2024 April 24 Á Dragons Egg Bipolar Emission Nebula
- APOD: 2024 March 13 Á The Seagull Nebula
- APOD: 2024 February 21 Á Seagull Nebula over Pinnacles Peak
- NGC 1893 and the Tadpoles of IC 410
- The Light, the Dark, and the Dusty
- APOD: 2023 December 13 Á Deep Field: The Heart Nebula
- The Ghosts of Gamma Cas