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Science Overview and Status of the SIM Project

机译:SIM项目的科学概述和现状

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This paper describes the broad goals and the current status of the Space Interferometry Mission (SIM). SIM was endorsed in the 1990 decadal report of the Astronomy and Astrophysics survey committee of the National Research Council. The SIM mission would be the first long baseline interferometer in space. The goals of SIM represent not factors of two or three improvement in astronometric accuracy, but two to three orders of magnitude improvement. The current most accurate astrometric measurements are from the Hipparcos satellite launched by ESA in 1990. Hipparchos achieved slightly better than 1 milliarcsec global astrometric accuracy. SIM's goal is 4 microarcsec accuracy for global astrometry (for a nominal 5 yr mission) and 1 microarcsec for single measurement narrow angle accuracy. The narrow angle precision translates to the ability to measure the "wobble" of stars with an error of 0.14 uas, if the target is observed 50 times during the 5 year mission. The paper gives an overview of the type of scientific questions SIM will address, concentrating on the planet detection aspects of SIM.
机译:本文介绍了空间干涉测量任务(SIM)的广泛目标和当前状态。 SIM已获得美国国家研究委员会(National Research Council)天文学和天体物理学调查委员会1990年的十年报告的认可​​。 SIM任务将是太空中的第一个长基线干涉仪。 SIM的目标不代表提高天文测量精度两到三个因素,而是代表提高两到三个数量级。当前最准确的天体测量结果来自于1990年由ESA发射的Hipparcos卫星。希帕科斯获得的全球天体测量精度略高于1毫秒。 SIM的目标是全球天体测量精度为4微弧度(标称5年任务),单次测量窄角精度精度为1微弧度。如果在5年的任务中观测到目标50次,则窄角精度将转化为以0.14 uas的误差测量恒星“摆动”的能力。本文概述了SIM将要解决的科学问题的类型,重点介绍了SIM的行星探测方面。

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