Hubbry Logo
search button
Sign in
Cambridge Optical Aperture Synthesis Telescope
Cambridge Optical Aperture Synthesis Telescope
Comunity Hub
arrow-down
History
arrow-down
starMore
arrow-down
bob

Bob

Have a question related to this hub?

bob

Alice

Got something to say related to this hub?
Share it here.

#general is a chat channel to discuss anything related to the hub.
Hubbry Logo
search button
Sign in
Cambridge Optical Aperture Synthesis Telescope
Community hub for the Wikipedia article
logoWikipedian hub
Welcome to the community hub built on top of the Cambridge Optical Aperture Synthesis Telescope Wikipedia article. Here, you can discuss, collect, and organize anything related to Cambridge Optical Aperture Synthesis Teles...
Add your contribution
Cambridge Optical Aperture Synthesis Telescope

Part of COAST and the exterior of its bunker in June 2014

Key Information

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 much higher resolution images than individual telescopes, including 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 Sun (although the surfaces of other stars had previously been imaged at lower resolution using aperture masking interferometry on the William Herschel Telescope).

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.

See also

[edit]

References

[edit]
[edit]