Celestial hemisphere:  Southern  ·  Constellation: Orion (Ori)  ·  Contains:  41 Ori A)  ·  41 Ori C  ·  41 Ori D  ·  43 Ori)  ·  Great Orion Nebula  ·  M 42  ·  M 43  ·  Mairan's Nebula  ·  NGC 1976  ·  NGC 1982  ·  Orion Nebula  ·  The star Mizan Batil II (θ2 Ori  ·  The star Trapezium (θ1 Ori A  ·  The star θ1 Ori C  ·  The star θ1 Ori D
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The Orion Nebula, Peter Hannah
The Orion Nebula
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The Orion Nebula

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The Orion Nebula, Peter Hannah
The Orion Nebula
Powered byPixInsight

The Orion Nebula

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Description

One of the most famous deep sky objects, the Orion nebula is a stellar nursery where young, hot massive stars are irradiating the gas cloud from which they were born, causing it to glow and develop ripples, bubbles and bow shocks as the radiation plows into the gas. At least one bubble and a bow shock are visible in the image when zoomed. Starbirth continues today as many protostars have also been discovered in the nebula.

The main nebula is designated M42 while the smaller spherical structure adjacent to it is M43. They are about 1340 light years away and being situated near the celestial equator they are visible from northern and southern hemispheres.

At the heart of the nebula are four young stars known as the Trapezium, officially designated θ1 to θ4 Orionis. Their spectral types are O and B, the hottest and most massive known, and they may be as young as 300,000 years.

This is the closest star-forming region to the solar system. It is about 24 light years across and is one of the brightest nebulæ, being visible to the naked eye in all but the most light-polluted skies.

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The Orion Nebula, Peter Hannah