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IC 434, Horsehead nebula

Fatalik
2023372
Category:Deep Sky
Published:
3611
IC 434, Horsehead nebulaNGC 2023NGC 2024IC 431IC 432IC 434IC 435
Resolution:
4961x3508 px
File size:
4877 KB

Photo description / processing

The Horsehead Nebula (IC 434, Barnard 33, also known as the "Horse's Head") is a dark nebula in the constellation Orion. The nebula is approximately 3.5 light-years in diameter and is located south of Alnitak (ζ Orionis), the easternmost star of Orion's Belt. It is part of the Orion Molecular Cloud Complex—a vast, star-forming region of gas and dust that surrounds the Orion Nebula, which lies at a distance of about 1,300 light-years. The Horsehead is one of the most famous nebulae. It appears as a dark, horsehead-shaped silhouette against a backdrop of red glowing gas. This glow is caused by the ionization of hydrogen clouds behind the nebula, energized by radiation from the nearby bright star Alnitak (ζ Orionis). The dark appearance of the nebula is primarily due to light being absorbed by a dense layer of dust, although there are areas (visible in photos on the left) that are cast in shadow by the base of the Horsehead's "neck." Gas streaming away from the nebula moves within a strong magnetic field. The bright spots at the base of the Horsehead Nebula are young stars in the process of formation. The nebula was first discovered in 1888 on photographic plates taken at the Harvard College Observatory.

Technical information

Telescope/Lens
Newtonian 8-inch f/5, 72ED
Camera
ZWO ASI1600MM Pro, Canon EOS 6D
Mount
Sky-Watcher EQ8
Location
Санкт-Петербург, Россия

Light pollution

Blue, Bortle 3 zone

Exposure

  • 30 × 180″ · ISO/Gain: 1600
  • 7 × 300″ · ISO/Gain: 140 · Ha 7nm

Total exposure: 2 h 5 m

Photo versions

IC 434, Horsehead nebula
Current photoUpdated
IC 434, Horsehead nebula

Nov 8th, 2019

2 h 5 m

The Horsehead Nebula (IC 434, Barnard 33, also known as the "Horse's Head") is a dark nebula in the constellation Orion. The nebula is approximately 3.5 light-years in diameter and is located south of Alnitak (ζ Orionis), the easternmost star of Orion's Belt. It is part of the Orion Molecular Cloud Complex—a vast, star-forming region of gas and dust that surrounds the Orion Nebula, which lies at a distance of about 1,300 light-years. The Horsehead is one of the most famous nebulae. It appears as a dark, horsehead-shaped silhouette against a backdrop of red glowing gas. This glow is caused by the ionization of hydrogen clouds behind the nebula, energized by radiation from the nearby bright star Alnitak (ζ Orionis). The dark appearance of the nebula is primarily due to light being absorbed by a dense layer of dust, although there are areas (visible in photos on the left) that are cast in shadow by the base of the Horsehead's "neck." Gas streaming away from the nebula moves within a strong magnetic field. The bright spots at the base of the Horsehead Nebula are young stars in the process of formation. The nebula was first discovered in 1888 on photographic plates taken at the Harvard College Observatory.

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