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The Antarctic Planet Interferometer

机译:南极行星干涉仪

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The Antarctic Planet Interferometer is a concept for an instrument designed to detect and characterize extrasolar planets by exploiting the unique potential of the best accessible site on earth for thermal infrared interferometry. High-precision interferometric techniques under development for extrasolar planet detection and characterization (differential phase, nulling and astrometry) all benefit substantially from the slow, low-altitude turbulence, low water vapor content, and low temperature found on the Antarctic plateau. At the best of these locations, such as the Concordia base being developed at Dome C, an interferometer with two-meter diameter class apertures has the potential to deliver unique science for a variety of topics, including extrasolar planets, active galactic nuclei, young stellar objects, and protoplanetary disks.
机译:南极行星干涉仪是一种仪器的概念,旨在通过利用地球上最佳可及位置的独特潜力来探测和表征太阳系外行星的热红外干涉仪。正在开发的用于太阳系外行星探测和表征(微分相位,零位和天体测量)的高精度干涉测量技术,都将从南极高原缓慢,低空的湍流,低水汽含量和低温中受益。在这些位置中最好的位置,例如在Dome C开发的Concordia基座,具有两米直径级孔径的干涉仪有可能为各种主题提供独特的科学知识,包括太阳系外行星,活跃的银河核,年轻的恒星物体和原行星盘。

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