Barnard's loop

Barnard's loop (Sharpless 276, part of the Orion-Eridanus Bubble) is a diffuse nebula in the constellation of Orion, the hunter.[2] The nebula was discovered by E. E. Barnard in 1895 utilising long exposure photographic methods.[3] However it may have been observed by William Herschel, one of the great nebula discoverers, in February 1786.[2] Unsurprisingly it is therefore far too faint to be observed with the naked eye. The nebula can be seen as a ring of bright gas surrounding Orion's belt. The Orion nebula along with the famous horsehead nebula are situated within Barnard's loop.

Barnard's loop
Barnard Loop - Hunter Wilson.jpg
Observational Data
Designation Sharpless 276
Right ascension 05h 27m 30s[1]
Declination -03° 58′ 00″[1]
Constellation Orion
Type of object Diffuse nebula
Dimensions >20°[2]
Astrometry
Distance from Earth 1,600 ly[2]

Properties and Structure

At 1,600 light years away, the nebula's apparent size of over 20° corresponds to a physical size of at least 582 light years.[4] The segment that is visible is believed to be part of a larger shell of material, with only the easternmost segment being visible in optical light.[5] The nebula is expanding at around 15-23 km/s.[5] The nebula contains several O and B type stars.

Even this nebula may be the inner surface of an even larger nebula that is at least 30 degrees in diameter.[6] As only the inner suface is ionized, only this is visible. The enveloping nebula would be truly vast and comprise of very hot, low density gas.[2] Observations of the nebula in ultraviolet light have suggested the existence of this larger nebula.

References

  1. ↑ 1.0 1.1 Barnard's Loop from the SIMBAD Astronomical Database
  2. ↑ 2.0 2.1 2.2 2.3 2.4 Barnard's loop from messier.seds.org
  3. ↑ Barnard's Loop Around Orion from apod.nasa.gov
  4. ↑ By direct calculation using values given here.
  5. ↑ 5.0 5.1 O'Dell, C., Ferland, G., Porter, R. and van Hoof, P. (2011). Physical Conditions in Barnard’S Loop, Components of the Orion-Eridanus Bubble, and Implications for the Warm Ionized Medium Component of the Interstellar Medium. The Astrophysical Journal, 733(1), p.9. arXiv:1103.2789
  6. ↑ Barnard's Loop from daviddarling.info