首页> 外文会议>Second European Workshop on Exo-Astrobiology Sep 16-19, 2002 Graz, Austria >ESA'S SEARCH FOR ECTRA-SOLAR TERRESTRIAL PLANETS: MISSION UPDATE OF THE DARWIN PROJECT
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ESA'S SEARCH FOR ECTRA-SOLAR TERRESTRIAL PLANETS: MISSION UPDATE OF THE DARWIN PROJECT

机译:欧空局(ESA)对大陆架卫星的搜索:达尔文项目的任务更新

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摘要

A mission status is given for the Darwin project. The Infra Red Space Interferometer Darwin was studied, by the European Space Agency (ESA), at system level, between 1997 and 2000. The study, carried out by Alcatel space division in Cannes, France has focused on developing a system that could carry out two main scientific objectives: (1) The detection and characterisation of Earth-like planets orbiting other stars. (2) The imaging of astrophysical objects with unprecedented spatial resolution. The most challenging of these objectives consist of the recording of infrared spectra of Terrestrial exo-planets that could detect signs of biological activity at distances up to 20pc. In order to do this, the Darwin project is constructed around the new technique of 'nulling interferometry', which exploits the wave nature of light in order to extinguish the light from a bright object (the central star, the primary, in this case). At the same time the light from a nearby source (the planet) is enhanced. The contrast between planets and stars being the least in the infrared wavelength region, that has been chosen for this mission.
机译:达尔文项目的任务状态已确定。欧洲航天局(ESA)在1997年至2000年之间对达尔文红外空间干涉仪进行了系统级研究。该研究由法国戛纳的阿尔卡特航天部门进行,其研究重点是开发一种可以执行以下任务的系统两个主要的科学目标:(1)对绕其他恒星运行的类地球行星进行探测和表征。 (2)天体物体的成像具有空前的空间分辨率。这些目标中最具挑战性的是记录地面系外行星的红外光谱,该光谱可以在最远20pc的距离处检测生物活性的迹象。为了做到这一点,达尔文项目是围绕“零干涉法”的新技术构建的,该技术利用光的波特性来消灭明亮物体(在这种情况下,中心星是主星)的光。 。同时,来自附近光源(行星)的光也会增强。为此任务选择的行星和恒星之间的对比度在红外波长范围内最小。

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