Byurakan Observatory

The Byurakan Astrophysical Observatory, or Byurakan Observatory is an astronomical observatory owned and operated by the Armenian Academy of Sciences. It is located on the slope of Mount Aragats in the village of Byurakan in Armenia.

Byurakan Observatory
Alternative namesByurakan Astrophysical Observatory Edit this at Wikidata
Named afterViktor Ambartsumian Edit this on Wikidata
OrganizationArmenian Academy of Sciences
Observatory code123
LocationMount Aragats, Armenia
Coordinates40°19′51″N 44°16′06″E / 40.33083°N 44.26833°E / 40.33083; 44.26833
Altitude1,400 m (5,000 ft)
Established1946 Edit this on Wikidata
telescope2.6 m Cassegrain reflector 40°19′49″N 44°16′24″E / 40.33028°N 44.27333°E / 40.33028; 44.27333
telescope1 m Schmidt reflector
telescope50 cm Schmidt reflector
Byurakan Observatory is located in Armenia
Byurakan Observatory
Location of Byurakan Observatory
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Founded in 1946 by Viktor Hambardzumyan, it was one of the main astronomy centers of the USSR. The buildings were designed by architect Samvel Safarian. The hotel, central building and structures are for astronomical instruments.[1] The observatory has discovered special star clustersstellar associations (1947),[1] more than 1,000 flare stars, dozens of supernovae, hundreds of Herbig–Haro objects and cometary nebulae, hundreds of galaxies.

The first conference was held in November 1951 on the topic of stellar associations. On 19 September 1956 a major meeting on non-stable stars was held.[1] It has been the site of two major conferences on SETI, and is recognised as the regional center for astronomical research.[1]

Directors included V.A. Ambartsumian till 1988, E.Ye. Khachikian till 1993, H.A. Harutyunian from 1993 to 1994, and A.R. Petrosian from 1994 to 1999. Khachikian returned as director from 1999 to 2003 and Harutyunian also returned after this.[1]


Byurakan Observatory's main telescope is a 2.6 m Cassegrain reflector, along with a 1 and 0.5 m Schmidt camera as well as other smaller telescopes.


The First Byurakan Survey commenced in 1965 using the Schmidt telescope. It revealed 1500 galaxies with ultraviolet excess known as the Markarian galaxies.[1] These galaxies are designated "Markarian" or "Mrk" followed by a number, for example Mrk 501.

The Second Byurakan Survey, 1974 to 1991,[2] looked for emission line and ultraviolet excess galaxies, and quasars as well.[1]


See alsoEdit


  1. ^ a b c d e f g Massaro, Enrico; Mickaelian, Areg; Nesci, Roberto; Daniel Weedman (2008). The Digitized First Byurakan Survey (PDF). ISBN 978-88-548-2421-8. Archived from the original (PDF) on 2012-04-26.
  2. ^ Erastova, L. K; Stepanian, J. A; Chavushyan, V. H (1997). "The Second Byurakan Survey: Galaxies". Wide-Field Spectroscopy. Astrophysics and Space Science Library. Vol. 212. pp. 321–324. doi:10.1007/978-94-011-5722-3_60. ISBN 978-94-010-6413-2.

External linksEdit