|Observation data (Epoch J2000)|
|Right ascension||22h 32m 36.4s|
|Declination||+11° 43′ 51s″|
|CTA-102 , Q2230+11 , QSR B2230+114 , QSO J2232+1143 , 4C +11.69 ,|
|See also: Quasar, List of quasars|
In astronomy, CTA 102, also known by its B1950 coordinates as 2230+114 (QSR B2230+114) and its J2000 coordinates as J2232+1143 (QSO J2232+1143), is a quasar discovered in the early 1960s by a radio survey carried out by the California Institute of Technology. It has been observed by a large range of instruments since its discovery, including WMAP, EGRET, GALEX, VSOP and Parkes, and has been regularly imaged by the Very Long Baseline Array since 1995. It has also been detected in gamma rays, and a gamma-ray flare has been detected from it.
In 1963 Nikolai Kardashev proposed that the then-unidentified radio source could be evidence of a Type II or III extraterrestrial civilization on the Kardashev scale. Follow-up observations were announced in 1965 by Gennady Sholomitskii, who found that the object's radio emission was varying; a public announcement of these results caused a worldwide sensation. The idea that the emission was caused by a civilization was rejected when the radio source was later identified as one of the many varieties of a quasar.
The American folk rock band The Byrds whimsically reflected the original view that CTA-102 was a sign of extraterrestrial intelligence in their song "C.T.A.-102" from their 1967 album Younger Than Yesterday.
- "CTA 102 in the NASA Extragalactic Database". Retrieved 2008-12-24.
- "CTA-102". Internet Encyclopedia of Space; David Darling. Retrieved 2008-12-14.
- "MOJAVE Sample: 2230+114". Retrieved 2008-12-25.
- "Fermi LAT detection of a GeV flare from blazar CTA 102". Astronomers Telegram. 3 May 2011. Retrieved 3 May 2011.
- Sholomitsky, G. B. (1965). "Variability of the Radio Source CTA-102". Information Bulletin on Variable Stars 83: 1. Bibcode:1965IBVS...83....1S.
- Rogan, Johnny (2011). Byrds: Requiem for the Timeless. Rogan House. pp. 317–320. ISBN 978-0-95295-408-8.
|This galaxy-related article is a stub. You can help Wikipedia by expanding it.|