description Flame Nebula (NGC 2024) Overview
The Flame Nebula (NGC 2024) is an emission nebula in the constellation Orion, located approximately 1,400 light-years from Earth. It is part of the Orion Molecular Cloud Complex and is energized primarily by ultraviolet radiation from Alnitak, the easternmost star of Orion's Belt. The nebula contains a young star cluster still in the process of formation, which is visible in infrared observations that can penetrate the dense dust clouds, revealing active star formation within this stellar nursery.
help Flame Nebula (NGC 2024) FAQ
Where is the Flame Nebula located?
The Flame Nebula, designated as NGC 2024, is an emission nebula located in the constellation of Orion. It is situated directly adjacent to Alnitak, the easternmost star of Orion's Belt.
What makes the Flame Nebula glow?
The nebula is energized by the intense ultraviolet radiation coming from the nearby O-class supergiant star Alnitak. This radiation strips electrons from the hydrogen gas, causing the cloud to glow brightly.
Can the Flame Nebula be seen with a telescope?
It is a popular target for astrophotographers but can be difficult to observe visually due to the glare from Alnitak. A telescope with an aperture of at least 6 inches is usually required to spot it.
How far away is the Flame Nebula?
The Flame Nebula is located approximately 1,300 to 1,500 light-years away from Earth. It is part of the much larger Orion Molecular Cloud Complex.
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