The Gaia Project - technique, performance and status

نویسنده

  • S. Jordan
چکیده

Gaia is a satellite mission of the ESA, aiming at absolute astrometric measurements of about one billion stars (all stars down to 20 magnitude, with unprecedented accuracy. Additionally, magnitudes and colors will be obtained for all these stars, while radial-velocities and spectral properties will be determined only for bright objects (V < 17.5). At 15 magnitude Gaia aims at an angular accuracy of 20 microarcseconds (μas). This goal can only be reached if the geometry of the telescopes, the detectors, and the pointing of Gaia at each moment (“attitude”) can be inferred from the Gaia measurements itself with μas accuracy.

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تاریخ انتشار 2008