MESSIER 78 Latitude and Longitude:

Sky map 05h 46.7m 00s, +00° 03′ 00″
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Messier 78
Reflection nebula
Image of Messier 78 captured using the Wide Field Imager camera on the MPG/ ESO 2.2-metre telescope at the La Silla Observatory.
Observation data: J2000.0 epoch
Right ascension05h 46m 46.7s [1]
Declination+00° 00′ 50″ [1]
Distance1,350  ly (415  pc) [2]  ly
Apparent magnitude (V)8.3 [3]
Apparent dimensions (V)8′ × 6′ [3]
Constellation Orion
Physical characteristics
Radius5 ly
Notable featuresPart of the Orion complex
DesignationsCed 55u, DG 80, IRAS 05442-0000, [KPS2012] MWSC 0664, NGC 2068 [1]
See also: Lists of nebulae

Messier 78 or M78, also known as NGC 2068, is a reflection nebula in the constellation Orion. It was discovered by Pierre Méchain in 1780 and included by Charles Messier in his catalog of comet-like objects that same year. [4]

M78 is the brightest diffuse reflection nebula of a group of nebulae that includes NGC 2064, NGC 2067 and NGC 2071. This group belongs to the Orion B molecular cloud complex and is about 1,350 light-years distant from Earth. [2] M78 is easily found in small telescopes as a hazy patch and involves two stars of 10th and 11th magnitude. These two B-type stars, HD 38563 A and HD 38563 B, are responsible for making the cloud of dust in M78 visible by reflecting their light. [5]

The M78 cloud contains a cluster of stars that is visible in the infrared. [2] Due to gravity, the molecular gas in the nebula has fragmented into a hierarchy of clumps, [2] whose cores have masses ranging from 0.3  M to M. [6] About 45 variable stars of the T Tauri type, [7] young stars still in the process of formation, are members as well. Similarly, 17 Herbig–Haro objects are known in M78. [8]

On May 23, 2024, the European Space Agency released an initial set of images from their Euclid mission. This included an unprecedented image of the region including M78. [9] It showed hundreds of thousands of new objects including sub-stellar sized ones for the first time.

Gallery

See also

References

  1. ^ a b c "M 78". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 14 February 2016.
  2. ^ a b c d Walker-Smith, S. L.; Richer, J. S.; Buckle, J. V.; Smith, R. J.; Greaves, J. S.; Bonnell, I. A. (March 2013), "The structure and kinematics of dense gas in NGC 2068", Monthly Notices of the Royal Astronomical Society, 429 (4): 3252–3265, arXiv: 1212.2018, Bibcode: 2013MNRAS.429.3252W, doi: 10.1093/mnras/sts582.
  3. ^ a b "Messier 78". SEDS Messier Catalog. Retrieved 30 April 2022.
  4. ^ Frommert, Hartmut; Kronberg, Christine (9 October 2018), "Messier 78", SEDS Messier pages, Students for the Exploration and Development of Space (SEDS), retrieved 5 December 2018.
  5. ^ Strom, S. E.; et al. (July 1974), "Infrared and optical observations of Herbig-Haro objects.", The Astrophysical Journal, 191: 111–142, Bibcode: 1974ApJ...191..111S, doi: 10.1086/152948.
  6. ^ Motte, F.; et al. (June 2001), "A SCUBA survey of the NGC 2068/2071 protoclusters", Astronomy and Astrophysics, 372 (3): L41–L44, arXiv: astro-ph/0105019, Bibcode: 2001A&A...372L..41M, doi: 10.1051/0004-6361:20010543, S2CID  7658059.
  7. ^ Herbig, G. H.; Kuhi, L. V. (February 1963), "Emission-Line Stars in the Region of NGC 2068", The Astrophysical Journal, 137: 398, Bibcode: 1963ApJ...137..398H, doi: 10.1086/147519.
  8. ^ Zhao, Bing; et al. (September 1999), "Newly Discovered Herbig-Haro Objects in the NGC 2068 and NGC 2071 Regions", The Astronomical Journal, 118 (3): 1347–1353, Bibcode: 1999AJ....118.1347Z, doi: 10.1086/301002.
  9. ^ "Euclid's new image of star-forming region Messier 78". The European Space Agency. ESA/Euclid/Euclid Consortium/NASA. 23 May 2024. Retrieved 27 May 2024.

External links