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For centuries, the positions of celestial objects have been measured by ground-based instruments. One of the first catalogues of stellar positions was produced by Hipparchus of Nicaea in 129 BC who made his measurements by eye. Over the centuries, the accuracy of these measurements improved, but finally the limitations inherent in ground-based techniques were reached. The challenge to overcome these limitations was met by Hipparcos.

Why is it so important to improve the positional measurements of the stars?

Despite the apparent simplicity of the measurements: two coordinates which specify the location of a star on the celestial sphere, the amount of information that can been gleaned from these numbers is quite incredible. The variation in the coordinates with time leads to the proper-motion of the star (a measurement of its actual motion in space and its motion relative to the solar system). The parallax of the star tells us how far the star is from us. We can then determine the 3-dimensional distribution of stars in the Galaxy. This gives us an insight into the dynamics of the Galaxy and how it may have been formed. Astrometry also tells us about basic stellar properties and can even help resolve the question of the age of the Universe.

Some examples of applications of the Hipparcos results:


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Last modified: Fri Sep 10 09:05:45 MET DST 1999
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