My Astrophotography – NGC 2359

NGC 2359 (Thor’s Helmet Nebula)

  • NGC 2359, widely known as Thor’s Helmet, is a massive glowing cloud of gas and dust located roughly 15,000 light-years away in the constellation Canis Major.
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  • It gets its famous nickname because its round shape and sweeping, wing-like extensions perfectly resemble the battle headwear of the Norse god of thunder.
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  • Object Name
    NGC 2359

  • Object Type
    Emission Nebula

  • Constellation
    Canes Major

  • Magnitude
    +11.5

  • Distance
    15,000 light-years

  • Annotated


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Equipment

Telescope:

Mount:

Accessories:

Sky-Watcher Esprint 80ED Triplet

ZWO AM7 Equatorial Mount

ZWO ASIair Plus / PixInsight

Camera:

Guiding:

Filter:

ZWO ASI2600MC Pro cooling

ZWO ASI1200MM

2″ Optolong L-Pro

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Bortle Scale: Haw Wood Farm, Saxmundham, Suffolk (Bortle 4.2)
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Integration

  • Date:
    Sunday 19th April 2026
    Tuesday 22nd October 2024
  • Moonlit:
    Waxing crescent: 1.8 days old
    Magnitude: -9.7
    Moonlit: 5%
  • Total:
    180’s x 30 subs = 1 hours 30 minutes

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Constellation :- Canes Major (The Great Dogs)

Object :-

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Object :-

Other name :-

Type :-

Magnitude :

Distance :-

Constellation :-

Right Ascension :-

Declination :-

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NGC 2359

Thor’s Helmet Nebula

Emission Nebula

+11.5

15,000 light years / 30 light years across

CMa (Canis Major / The Great Dogs)

07h 18m 06s

+13° 12′ 27″

Enlarge on click the map.

(Click the map above for a large view.)

Abbreviation:  CMa (Canis Major)
English Name:  The Great Dogs
Genitive: Sirius
Hemisphere: Southern Hemisphere
Location: Between the constellations of Monoceros and Lepus.
Visible between latitudes:  +60 and -90 degrees
Best season: Winter
Seen in three seasons: Autumn, Winter, and Spring
Best seen in:  February (map) and March (map)
Seen between: October and March
Right Ascension (RA): 07 hour
Declination (DEC): -20 degrees
Area (square degrees):  380 (43th)

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The Glowing Colours are Chemical Reactions

  • When astrophotographers take pictures of Thor’s Helmet, it glows with brilliant teals, blues, and reds.
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  • The intense ultraviolet radiation from the central star zaps the surrounding gas.
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  • The blue-green glow comes from highly energized oxygen atoms, while the deep red strands are glowing hydrogen gas.
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