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The RATAN-600 (Russian: РАТАН-600 – радиоастрономический телескоп Академии наук - 600, an acronym for the "Academy of Sciences Radio Telescope - 600") is a radio telescope in Zelenchukskaya, Russia. It comprises a 576 m diameter circle of rectangular radio reflectors and a set of secondary reflectors and receivers, based at an altitude of 970 m. Each of the 895 2×7.4 m reflectors can be angled to reflect incoming radio waves towards a central conical secondary mirror, or to one of five parabolic cylinders. Each secondary reflector is combined with an instrumentation cabin containing various receivers and instruments. The overall effect is that of a partially steerable antenna with a maximum resolving power of a nearly 600 m diameter dish, when using the central conical receiver, making it the world's largest-diameter individual radio telescope.

Radio Astronomical Telescope Academy Nauk 600
RATAN 600 crop.jpg
View of the observatory from a neighboring hill
Alternative namesRATAN-600 Edit this at Wikidata
Location(s)Zelenchukskaya, Russia Edit this at Wikidata
Coordinates43°49′33″N 41°35′11″E / 43.8258°N 41.5864°E / 43.8258; 41.5864Coordinates: 43°49′33″N 41°35′11″E / 43.8258°N 41.5864°E / 43.8258; 41.5864 Edit this at Wikidata
Altitude970 m (3,180 ft) Edit this at Wikidata
Wavelength1.38, 2.70, 3.90, 7.6, 13, 31.1 cm (21.72, 11.10, 7.69, 3.94, 2.31, 0.96 GHz)
Built1968 Edit this on Wikidata–1977 Edit this on Wikidata (1968 Edit this on Wikidata–1977 Edit this on Wikidata) Edit this at Wikidata
First light12 July 1974 Edit this on Wikidata
Telescope styleradio telescope Edit this on Wikidata
Diameter576 m (1,889 ft 9 in) Edit this at Wikidata
Collecting area1,200 m2 (13,000 sq ft) Edit this at Wikidata
Websitewww.sao.ru/ratan/ Edit this at Wikidata
RATAN-600 is located in Russia
RATAN-600
Location of RATAN-600
1987 USSR stamp commemorating RATAN-600

Contents

Operating modesEdit

The telescope can operate in three modes:[1]

  • Two-mirror system: A sector of the ring focuses waves to the cylindrical secondary mirror which directs them onto the receivers.
  • Three-mirror system: The linear plane mirror reflects the waves to the south sector of the ring, which focuses them on a cylindrical secondary, that reflects them onto the receivers. This is a Kraus-type periscope mirror system.
  • Entire ring: For observations near the zenith, the entire ring can be used, together with the conical secondary mirror and its receivers.

Simultaneous independent observations at various discrete azimuths are possible. For this, a sector of the ring is coupled with one of the secondary mirror-and-receiver units, which can be positioned using railway tracks, while another sector, in conjunction with another secondary mirror, is similarly used for an independent observation.

Optical specificationsEdit

It has a resolving power in the horizontal plane of 1 arcminute. At a wavelength of 8 cm, (3.75 GHz) the effective collecting area of the entire ring is 1,000 square metres (11,000 sq ft) which is 0.33% of that expected of a completely filled reflector of this size.

Transit telescopeEdit

The RATAN-600 is primarily operated as a transit telescope, in which the rotation of the Earth is used to sweep the telescope focus across the subject of observation. Radio frequency observations can be made in the frequency band 610 MHz to 30 GHz, though primarily in the centimetric waveband, with an angular resolution of up to 2 arcseconds. Observation of the Sun at radio wavelengths, in particular of the solar corona, has been a long-standing focus of the RATAN-600's scientific programme. It has also contributed to radio observation for the SETI project. The RATAN-600 has not suffered from the persistent technical problems of the neighbouring BTA-6, and has generally been in high demand since it began operation in mid-1974.

SETI candidate signalEdit

On 15 May 2015, at 18:01:15.65 sidereal time, RATAN-600 detected a strong (0.75 Jansky) signal from the direction of HD164595. More specifically, the signal intensity rose and fell as the telescope panned past in a way that closely matched what would be expected for a distant source. Since the short wavelength (2.7 cm, or 11 GHz, in the X band) is unusual for a natural source of that power, after the researchers announced the signal in late August 2016 (in the form of a request for follow-up observations) there was a flurry of excitement that it might be a SETI candidate.[2][3] Of course, the same artificial appearance also makes a terrestrial source likely. Because the signal is in a frequency band allocated to military use, it might have originated from a secret reconnaissance satellite. After further analysis, and a failure of other observatories to corroborate the signal, the Special Astrophysical Observatory concluded that it was of probably terrestrial origin.[4]

Later research suggests that it might have been a faulty satellite in a slow spin, as the frequency matches one used for inter-satellite beacons.

ReferencesEdit

  1. ^ The RATAN-600 Radio Telescope - Russian Academy of Science, Special Astrophysical Observatory
  2. ^ Gilster, Paul (27 August 2016). "An Interesting SETI Candidate in Hercules". Centauri Dreams blog. Retrieved 2016-08-30.
  3. ^ Berger, Eric (29 August 2016). "SETI has observed a "strong" signal that may originate from a Sun-like star". Ars Technica. Retrieved 2016-08-30.
  4. ^ "Monitoring of the continuum of SETI candidates with RATAN-600 (SAO RAS official comment)" (Press release). Special Astrophysical Observatory. 1 September 2016. Retrieved 2016-09-01. In the framework of this program, an interesting radio signal at a wavelength of 2.7 cm was detected in the direction of one of the objects (star system HD164595 in Hercules) in 2015. Subsequent processing and analysis of the signal revealed its most probable terrestrial origin.