Cookie consent

AstroBin saves small pieces of text information (cookies) on your device in order to deliver better content and for statistical purposes. You can disable the usage of cookies by changing the settings of your browser. By browsing AstroBin without changing the browser settings, you grant us permission to store that information on your device.

I agree
Contains:  NGC 2024, The star Alnitak (ζOri)
Getting plate-solving status, please wait...
NGC 2024 Flame Nebula, 





    
        

            Jerry Macon
NGC 2024 Flame Nebula

NGC 2024 Flame Nebula

Technical card

Resolution: 4656x3520

Dates:Nov. 4, 2019

Frames:
Astrodon Gen 2 L 36mm: 128x120" (gain: 99.00) -12C bin 1x1
Astrodon Gen 2 RGB 36mm: 120x120" (gain: 99.00) -16C bin 1x1

Integration: 8.3 hours

Avg. Moon age: 7.44 days

Avg. Moon phase: 50.63%

Bortle Dark-Sky Scale: 4.00

Astrometry.net job: 3106341

RA center: 5h 41' 42"

DEC center: -1° 51' 32"

Pixel scale: 0.701 arcsec/pixel

Orientation: 178.068 degrees

Field radius: 0.568

Locations: Dark Star Observatory, Taos, New Mexico, United States

Data source: Own remote observatory

Remote source: Non-commercial independent facility

Description

Images from the following two scopes (piggybacked) contributed to this image:
AG12+ASI1600MM at .70 asec/pix (RGB)
TV127is+ASI183MM at .75 asec/pix. (L)
They were all registered to the best R image taken on the AG12.
This image was unguided.

The Flame Nebula, designated as NGC 2024 and Sh2-277, is an emission nebula in the constellation Orion. It is about 900 to 1,500 light-years away.

The bright star Alnitak, the easternmost star in the Belt of Orion, shines energetic ultraviolet light into the Flame and this knocks electrons away from the great clouds of hydrogen gas that reside there. Much of the glow results when the electrons and ionized hydrogen recombine. Additional dark gas and dust lies in front of the bright part of the nebula and this is what causes the dark network that appears in the center of the glowing gas. The Flame Nebula is part of the Orion Molecular Cloud Complex, a star-forming region that includes the famous Horsehead Nebula.

At the center of the Flame Nebula is a cluster of newly formed stars, 86% of which have circumstellar disks. X-ray observations by the Chandra X-ray Observatory show several hundred young stars, out of an estimated population of 800 stars. X-ray and infrared images indicate that the youngest stars are concentrated near the center of the cluster.
(Wikipedia)

Comments

Author

jmacon
Jerry Macon
License: Attribution Creative Commons
3623
Like

Revisions

  • NGC 2024 Flame Nebula, 





    
        

            Jerry Macon
    Original
  • Final
    NGC 2024 Flame Nebula, 





    
        

            Jerry Macon
    B

Sky plot

Sky plot

Histogram

NGC 2024 Flame Nebula, 





    
        

            Jerry Macon