My Astrophotography – NGC 2024 (The Flame Nebula)

NGC 2024 (The Flame Nebula)

  • NGC 2024, better known as the Flame Nebula, is one of the most famous star-forming regions in the winter sky.
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  • NGC 2024 is a favourite target for astrophotographers because it lies close to the famous Horsehead Nebula, allowing both objects to be photographed in the same field of view.
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  • Object Name
    NGC 2024

  • Object Type
    Emission Nebula

  • Constellation
    Orion

  • Magnitude
    +2.0

  • Distance
    1,400 ly

  • Annotated

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Equipment

Telescope:

Mount:

Accessories:

Sky-Watcher Esprint 80ED Triplet

Sky-Watcher AZ-EQ6 GT

ZWO ASIair Plus / PixInsight

Camera:

Guiding:

Filter:

ZWO ASI585MC Pro cooling

ZWO ASI1200MM

2″ Optolong eNchance

Bortle Scale: Milton Keynes, Buckinghamshire (Bortle 6.6)


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Integration

  • Date:
    Wednesday 22nd October 2025
  • Moonlit:
    Waxing Crescent 5 days old
    Magnitude: -11.2
    Moonlit: 24%
  • Total:
    180’s x 50 subs = 2 hours 30 minutes

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Constellation :- Orion (The Hunter)

Object :-

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Object :-

Other name :-

Type :-

Magnitude :

Distance :-

Constellation :-

Right Ascension :-

Declination :-

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NGC 2024

Sh2-227 / The Flame Nebula / Tank Trap Nebula

Emission Nebula

+2.0

1,400 light years / 6 light years across

Ori (Orion / The Hunter)

05h 41m 54s

-01° 51′ 01″

Enlarge on click the map.

(Click the map above for a large view.)

Abbreviation:  Ori
English Name:  The Hunter
Genitive: Betelgeuse
Hemisphere: Northern and Southern Hemisphere. (Bold means the more area in square feet in Southern Hemisphere.)
Location: Between the constellations of Monoceros and Eridanus.
Visible between latitudes:  +90 and -40 degrees
Best season: Winter
Seen in three seasons: Autumn, Winter and Spring
Best seen in:  January (map) and February (map)
Seen between: November and early March
Right Ascension (RA): 05 hour
Declination (DEC): +05 degrees
Area (square degrees):  594 (26th)

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Facts about NGC 2025 ( The Flame Nebula)

  • Hidden within the dust is a young cluster of several hundred newly formed stars.
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  • Many are best seen in infrared or X-ray light because visible light cannot easily penetrate the dust.
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