首页> 外文会议>Conference on Interferometry in Space Pt.1, Aug 26-28, 2002, Waikoloa, Hawaii, USA >Space Interferometry Mission - Dynamical Observations of Galaxies (SIMDOG) Key Project
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Space Interferometry Mission - Dynamical Observations of Galaxies (SIMDOG) Key Project

机译:空间干涉测量任务-星系动态观测(SIMDOG)重点项目

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The Space Interferometry Mission (SIM) spacecraft will be used to measure the proper motions for a sample of ~30 nearby galaxies. At this time there are no proper motion measurements of galaxies beyond the satellite systems of the Milky Way. With the capability of measuring absolute positions to 4 μas (microarcsecond) accuracy and a five-year baseline, SIM will be able to measure proper motions as small as 10 km/s over the Local Group and 40 km/s at 4 Mpc. The motion of each galaxy will be monitored by targeting 5-10 stars that are brighter than 20th magnitude. SIM measurements will lead to knowledge of the full 6-dimensional position and velocity vectors of each galaxy. In conjunction with gravitational flow modeling, improved total mass measurements of individual galaxies and the fractional contribution of dark matter to galaxies of the Local Group will be obtained. The project includes development of theoretical methods for orbital calculations.
机译:太空干涉测量任务(SIM)航天器将用于测量大约30个附近星系样本的适当运动。目前,除了银河系的卫星系统之外,没有适当的星系运动测量值。凭借能够以4μas(微弧秒)的精度测量绝对位置的能力和五年的基准,SIM将能够测量本地组上低至10 km / s的正常运动,而在4 Mpc下可测量40 km / s的正确运动。每个星系的运动将通过瞄准5至10个比20级更亮的恒星来进行监控。 SIM卡测量将使您了解每个星系的完整6维位置和速度矢量。结合重力流模型,将获得改进的单个星系的总质量测量值以及暗物质对本地群星系的分数贡献。该项目包括开发用于轨道计算的理论方法。

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