New method for asteroid identification with the use of Pulkovo Apparent Motion Parameters

Details New method for asteroid identification with the use of Pulkovo Apparent Motion Parameters New method for asteroid identification with the use of Pulkovo Apparent Motion Parameters

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.500..417b&link_type=abstract

In: Proceedings of Asteroids, Comets, Meteors - ACM 2002. International Conference, 29 July - 2 August 2002, Berlin, Germany. Ed

Physics

Minor Planets, Positions, Identifications

Scientific paper

A new method for moving celestial body identification was elaborated at Pulkovo Observatory by means of taking into consideration of the first and the second derivatives of its spherical coordinates or with the use of Pulkovo Apparent Motion Parameters (AMPs), namely an angular velocity, angular acceleration, position angle and a curvature of its visible trajectory. Method was tested with a vast simulation and may be recommended for real observational practice.

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