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单词 Hipparcos
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Hipparcos

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依巴谷卫星
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  • shipwreck n. 海难, 船只失事
  • Hipparchus 依巴谷环形山
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Hipparcos abbr. [天] 依巴谷卫星(High Precision Parallax Collecting Satellite,欧洲太空总署发射的卫星名)

网络短语:
Hipparcos star 依巴谷星
Hipparcos Catalog System 伊巴谷星表
Hipparcos-Tycho Catalogue 英语
Hipparcos s catalogue 依巴谷星表
Hipparcos and Tycho Datalogues 依巴谷〉以及〈第谷〉星表
Hipparcos and Tycho Catalogues 依巴谷〉和〈第谷〉星表
Hipparcos High Precision Parallax 依巴谷〉卫星
Hipparcos s and Tycho Catalogues 依巴谷〉和〈第谷〉星表
中文百科

依巴谷卫星

Optical micrograph of part of the main modulating grid (top) and the star mapper grid (bottom). The period of the main grid is 8.2 micrometres.
The path on the sky of one of the Hipparcos Catalogue objects, over a period of three years. Each straight line indicates the observed position of the star at a particular epoch: because the measurement is one-dimensional, the precise location along this position line is undetermined by the observation. The curve is the modelled stellar path fitted to all the measurements. The inferred position at each epoch is indicated by a dot, and the residual by a short line joining the dot to the corresponding position line. The amplitude of the oscillatory motion gives the star's parallax, with the linear component representing the star's proper motion.
Typical accuracies of the FK5, Hipparcos, Tycho-1, and Tycho-2 Catalogues as a function of time. Tycho-1 dependencies are shown for two representative magnitudes. For Tycho-2, a typical proper motion error of 2.5 milliarc-sec applies to both bright stars (positional error at J1991.25 of 7 milliarc-sec) and faint stars (positional error at J1991.25 of 60 milliarc-sec).

依巴谷卫星High Precision Parallax Collecting Satellite,缩写为Hipparcos),全称为“依巴谷高精视差测量卫星”,是欧洲太空总署发射的一颗天体测量卫星,用以测量恒星视差和自行,以古希腊天文学家喜帕恰斯的名字命名。

依巴谷卫星于****年8月8日由亚利安4号火箭运载升空。它本应于地球同步轨道上运作,但因助推火箭失效,卫星只到达近地点507千米、远地点35,888千米的狭长椭圆轨道。尽管如此,它仍能完成85%的原任务目标。与该卫星的通信于1993年8月15日中止。

英语百科

Hipparcos 依巴谷卫星

Hipparcos testing at ESTEC
Optical micrograph of part of the main modulating grid (top) and the star mapper grid (bottom). The period of the main grid is 8.2 micrometres.
The path on the sky of one of the Hipparcos Catalogue objects, over a period of three years. Each straight line indicates the observed position of the star at a particular epoch: because the measurement is one-dimensional, the precise location along this position line is undetermined by the observation. The curve is the modelled stellar path fitted to all the measurements. The inferred position at each epoch is indicated by a dot, and the residual by a short line joining the dot to the corresponding position line. The amplitude of the oscillatory motion gives the star's parallax, with the linear component representing the star's proper motion.
Typical accuracies of the FK5, Hipparcos, Tycho-1, and Tycho-2 Catalogues as a function of time. Tycho-1 dependencies are shown for two representative magnitudes. For Tycho-2, a typical proper motion error of 2.5 milliarc-sec applies to both bright stars (positional error at J1991.25 of 7 milliarc-sec) and faint stars (positional error at J1991.25 of 60 milliarc-sec).

Hipparcos was a scientific satellite of the European Space Agency (ESA), launched in **** and operated until 1993. It was the first space experiment devoted to precision astrometry, the accurate measurement of the positions of celestial objects on the sky. This permitted the accurate determination of proper motions and parallaxes of stars, allowing a determination of their distance and tangential velocity. When combined with radial velocity measurements from spectroscopy, this pinpointed all six quantities needed to determine the motion of stars. The resulting Hipparcos Catalogue, a high-precision catalogue of more than 118,200 stars, was published in 1997. The lower-precision Tycho Catalogue of more than a million stars was published at the same time, while the enhanced Tycho-2 Catalogue of 2.5 million stars was published in 2000. Hipparcos' follow-up mission, Gaia, was launched in 2013.

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更新时间:2025/6/17 23:58:43