Cambridge Optical Aperture Synthesis Telescope

COAST, the Cambridge Optical Aperture Synthesis Telescope, is a multi-element optical astronomical interferometer with baselines of up to 100 metres, which uses aperture synthesis to observe stars with angular resolution as high as one thousandth of one arcsecond (producing images with much higher resolution than can be obtained using individual telescopes such as the Hubble Space Telescope). The principal limitation is that COAST can only image bright stars. COAST was the first long-baseline interferometer to obtain high-resolution images of the surfaces of stars other than our sun (although the surfaces of other stars had previously been imaged at lower resolution using Aperture Masking Interferometry on the William Herschel Telescope).

Cambridge Optical Aperture Synthesis Telescope
Cmglee Cambridge MRAO COAST bunker.jpg
The interior of the COAST bunker in June 2014
Alternative namesCOAST Edit this at Wikidata
Part ofMullard Radio Astronomy Observatory Edit this on Wikidata
Location(s)Cambridge, Cambridgeshire, East of England, England
Coordinates52°09′50″N 0°02′28″E / 52.164°N 0.041°E / 52.164; 0.041Coordinates: 52°09′50″N 0°02′28″E / 52.164°N 0.041°E / 52.164; 0.041 Edit this at Wikidata
Telescope styleastronomical interferometer
optical telescope Edit this on Wikidata Edit this at Wikidata
Cambridge Optical Aperture Synthesis Telescope is located in the United Kingdom
Cambridge Optical Aperture Synthesis Telescope
Location of Cambridge Optical Aperture Synthesis Telescope
Commons page Related media on Wikimedia Commons
Part of COAST and the exterior of its bunker in June 2014

The COAST array was conceived by John E. Baldwin, and is operated by the Cavendish Astrophysics Group. It is situated at the Mullard Radio Astronomy Observatory in Cambridgeshire, England.

External linksEdit