首页> 外文会议>Conference on Interferometry in Space Pt.1, Aug 26-28, 2002, Waikoloa, Hawaii, USA >A Visible Light Terrestrial Planet Finder --Planet Detection and Spectroscopy by Nulling Interferometry with a Single Aperture Telescope
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A Visible Light Terrestrial Planet Finder --Planet Detection and Spectroscopy by Nulling Interferometry with a Single Aperture Telescope

机译:可见光地球行星查找器-使用单孔径望远镜通过零位干涉法进行行星探测和光谱学

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摘要

Planet detection around a bright star is dependent on the resolution of the imaging system and the degree of light suppression of the star relative to the planet. We present a concept and a scaled precursor for a visible light Terrestrial Planet Finding (VTPF) mission. Its major feature is an imaging system for planet detection using a nulling interferometer behind a single aperture telescope. This configuration is capable of detecting earth-like planets with a 4m aperture using both imaging and spectroscopic imaging modes. We will describe the principles of the system, and show results of studies demonstrating its feasibility.
机译:围绕一颗明亮恒星的行星探测取决于成像系统的分辨率以及该恒星相对于行星的光抑制程度。我们为可见光地面行星发现(VTPF)任务提出了一个概念和一个可缩放的前体。它的主要功能是在单孔望远镜后面使用零位干涉仪进行行星探测的成像系统。这种配置能够使用成像和光谱成像模式检测孔径为4m的类地行星。我们将描述该系统的原理,并显示证明其可行性的研究结果。

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