Barnard's Loop (catalogue designation Sh 2-276) is an emission nebula in the constellation of Orion. It is part of the Orion molecular cloud complex which also contains the dark Horsehead and bright Orion nebulae. The loop takes the form of a large arc centered approximately on the Orion Nebula. The stars within the Orion Nebula are believed to be responsible for ionizing the loop.

Quick Facts Emission nebula, Observation data: J2000 epoch ...
Barnard's Loop
Emission nebula
H II region
Thumb
Barnard's Loop can be seen on this image as a diffuse red semicircle.
Observation data: J2000 epoch
Right ascension05h 27.5m
Declination−03° 58
Distanceeither 518 or 1434 ly
Apparent magnitude (V)5
Apparent dimensions (V)10°
ConstellationOrion
Physical characteristics
Radiuseither 50 or 150 ly
DesignationsSh 2-276
See also: Lists of nebulae
Close

The loop extends over about 600 arcminutes as seen from Earth, covering much of Orion. It is best seen in long-exposure photographs, although observers under very dark skies may be able to see it with the naked eye.

Recent estimates place it at a distance of either 159 parsecs (518 light-years) or 440 pc (1434 ly), giving it dimensions of either about 100 or 300 ly across, respectively.[1][2] It is thought to have originated in a supernova explosion about 2 million years ago, which may have also created several known runaway stars, including AE Aurigae, Mu Columbae and 53 Arietis, which are believed to have been part of a multiple star system in which one component exploded as a supernova.[3]

Although this faint nebula was certainly observed by earlier astronomers, it is named after the pioneering astrophotographer E. E. Barnard who photographed it and published a description in 1894.[4]

References

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