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Imaging nonsolar planets by nulling interferometry

机译:通过零干涉法对非太阳行星成像

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A planet resembling Jupiter, circling a Sun-like star that is 10 parsecs away from us, would subtend 0.1 milliarcseconds, while the star would subtend 1 milliarcsecond. A planet circling the star at a distance of 5 AU (Jupiter's distance from the Sun) would present at most an angular separation of 0.5 arcseconds. Existing telescopes have neither the angular resolution nor sensitivity to detect such a planet directly. Jupiter-sized planets circling their star rapidly at separations of about 1 AU have revealed their presence, indirectly, by inducing minute, periodic Doppler shifts in the light of their star, and one looks forward to improvement in sensitivity to cope with the smaller shifts induced by 'Jupiters' at 5 AU and 'Earths' at 1 AU. Meanwhile, a space-based interferometer receiving at infrared wavelengths has received national support. The idea is to adjust an interferometer for a null in its median plane so as to null out the radiation received from the star; and to spin the interferometer about the Earth-star line to gain the signal-to-noise improvement associated with phase-sensitive detection. Angel and Woolf have improved the concept by proposing a four-in-line configuration that widens the central null and broadens the band to include spectral lines of water, ozone and carbon dioxide, all molecules relating to life. Hinz et al. have demonstrated the nulling principle, without going into space, using two elements of the Multiple Mirror Telescope (which has now been dismantled). The thermal radiation from Betelgeuse was attenuated sufficiently to reveal a faint zodiacal light cloud that would be conventionally lost in the glare of Betelgeuse. These factors constitute important inputs to NASA's Terrestrial Planet Finder mission. The Large Binocular Telescope, comprising two 8.4 m mirrors spaced 14.4 m between centers on a single altazimuth mount, will allow further experience with nulling interferometry on a large scale. The housing on Mt Graham, Arizona, is ready to receive the telescope structure, which has been prefabricated in Italy.
机译:一颗类似木星的行星绕着离我们10帕秒的太阳般恒星旋转,对向约0.1毫秒,而恒星对向旋转1毫秒。绕恒星旋转5 AU(木星到太阳的距离)的行星最大角度间隔为0.5弧秒。现有的望远镜既没有角分辨率也没有灵敏度来直接检测这种行星。木星大小的行星以大约1 AU的间隔快速绕其恒星旋转,已经揭示出它们的存在,这是间接地通过根据恒星引起微小的周期性多普勒频移而引起的,人们期待着提高灵敏度以应对较小的频移由“木星”在5 AU和“地球”在1 AU。同时,接收红外波长的天基干涉仪已获得国家支持。想法是将干涉仪的中值平面调整为零,以消除从恒星接收的辐射。并使干涉仪绕地球之星线旋转,以改善与相敏检测相关的信噪比。安吉尔(Angel)和伍尔夫(Woolf)通过提出一种四列式配置改进了这一概念,该配置可扩大中心零位并扩大谱带,以包括水,臭氧和二氧化碳的光谱线,所有与生命有关的分子。 Hinz等。已使用多镜望远镜(现已拆除)的两个元素演示了归零原理,而无需进入太空。来自Betelgeuse的热辐射被充分衰减以显示微弱的黄道光云,该云通常会在Betelgeuse的眩光中消失。这些因素构成了NASA的“地球行星搜寻器”任务的重要输入。大型双筒望远镜由两个8.4 m的反射镜组成,两个反射镜在单个高度安装座上的中心之间间隔14.4 m,这将为大规模零陷干涉提供进一步的经验。亚利桑那州格雷厄姆山(Mt Graham)上的房屋已准备好接受意大利预制的望远镜结构。

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