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Cambridge Optical Aperture Synthesis Telescope Cambridge Optical Aperture Synthesis Telescope Cambridge Optical Aperture Synthesis Telescope 劍橋光學孔徑合成望遠鏡
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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. 劍橋光學孔徑合成望遠鏡(Cambridge Optical Aperture Synthesis Telescope，COAST)是一架基線長達100米的多元件光學，他使用來觀測恆星，可以使解析度提高到千分之一角秒 (這種非常高的解析度不是使用單一的望遠鏡，例如哈伯太空望遠鏡，可以達到的)，主要的限制是COAST只能觀測明亮的恆星。COAST是第一架長基線干涉儀，可以獲得太陽以外恆星表面的高解析影像 (雖然在這之前，威廉·赫歇爾望遠鏡使用已經獲得其它恆星表面的低解析影像。)。 COAST陣列的構想是提出的，並由執行。它位於英國劍橋郡的。 Das Cambridge Optical Aperture Synthesis Telescope (COAST) ist ein astronomisches Interferometer im Mullard Radio Astronomy Observatory in Cambridgeshire, England. Es besteht aus fünf über Siderostaten ausrichtbaren Cassegrain-Teleskopen mit jeweils 40 cm Spiegeldurchmesser, die zusammen, separiert durch eine Basislänge von bis zu 100 m, Winkelauflösungen von bis zu 0,001 Bogensekunden erreichen können. Mit COAST gelang es erstmals, hochaufgelöste Bilder von Sternenoberflächen aufzunehmen. Il Cambridge Optical Aperture Synthesis Telescope (o COAST) è un interferometro astronomico ottico multielemento con delle linee base lunghe fino a 100 metri, che utilizza una sintesi di apertura per osservare le stelle con una risoluzione angolare di un millesimo di secondo d'arco; genera pertanto delle immagini con una risoluzione più alta di quella che è possibile ottenere con un singolo telescopio, come il Telescopio Spaziale Hubble. Il limite principale di questo complesso di strumenti è che può riprendere solo stelle luminose. Il COAST fu il primo interferometro multielemento ad ottenere delle immagini ad alta risoluzione della superficie di stelle esterne al nostro sistema solare; in precedenza, la superficie delle stelle era stata ripresa, a risoluzione inferiore, utilizzando l' de
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劍橋光學孔徑合成望遠鏡(Cambridge Optical Aperture Synthesis Telescope，COAST)是一架基線長達100米的多元件光學，他使用來觀測恆星，可以使解析度提高到千分之一角秒 (這種非常高的解析度不是使用單一的望遠鏡，例如哈伯太空望遠鏡，可以達到的)，主要的限制是COAST只能觀測明亮的恆星。COAST是第一架長基線干涉儀，可以獲得太陽以外恆星表面的高解析影像 (雖然在這之前，威廉·赫歇爾望遠鏡使用已經獲得其它恆星表面的低解析影像。)。 COAST陣列的構想是提出的，並由執行。它位於英國劍橋郡的。 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. Das Cambridge Optical Aperture Synthesis Telescope (COAST) ist ein astronomisches Interferometer im Mullard Radio Astronomy Observatory in Cambridgeshire, England. Es besteht aus fünf über Siderostaten ausrichtbaren Cassegrain-Teleskopen mit jeweils 40 cm Spiegeldurchmesser, die zusammen, separiert durch eine Basislänge von bis zu 100 m, Winkelauflösungen von bis zu 0,001 Bogensekunden erreichen können. Mit COAST gelang es erstmals, hochaufgelöste Bilder von Sternenoberflächen aufzunehmen. Il Cambridge Optical Aperture Synthesis Telescope (o COAST) è un interferometro astronomico ottico multielemento con delle linee base lunghe fino a 100 metri, che utilizza una sintesi di apertura per osservare le stelle con una risoluzione angolare di un millesimo di secondo d'arco; genera pertanto delle immagini con una risoluzione più alta di quella che è possibile ottenere con un singolo telescopio, come il Telescopio Spaziale Hubble. Il limite principale di questo complesso di strumenti è che può riprendere solo stelle luminose. Il COAST fu il primo interferometro multielemento ad ottenere delle immagini ad alta risoluzione della superficie di stelle esterne al nostro sistema solare; in precedenza, la superficie delle stelle era stata ripresa, a risoluzione inferiore, utilizzando l' del William Herschel Telescope. L'allineamento del COAST fu ideato da e realizzato dal ; è situato nel Mullard Radio Astronomy Observatory nel Cambridgeshire, nel Regno Unito.
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