Astrometric baseline observations of solar system bodies


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Abstract

The use of ground-based and space baseline observations of Solar System bodies is considered. Baseline observations allow one to determine the distance to observed objects and (in some cases) the parameters of their orbital motion. Certain results of baseline observations of near-Earth asteroids and the results of model analysis of spacecraft observations are presented.

About the authors

A. V. Devyatkin

Central (Pulkovo) Astronomical Observatory

Author for correspondence.
Email: adev@gao.spb.ru
Russian Federation, Pulkovskoe sh. 65, St. Petersburg, 196140

D. L. Gorshanov

Central (Pulkovo) Astronomical Observatory

Email: adev@gao.spb.ru
Russian Federation, Pulkovskoe sh. 65, St. Petersburg, 196140

V. N. L’vov

Central (Pulkovo) Astronomical Observatory

Email: adev@gao.spb.ru
Russian Federation, Pulkovskoe sh. 65, St. Petersburg, 196140

S. D. Tsekmeister

Central (Pulkovo) Astronomical Observatory

Email: adev@gao.spb.ru
Russian Federation, Pulkovskoe sh. 65, St. Petersburg, 196140

M. S. Chubey

Central (Pulkovo) Astronomical Observatory

Email: adev@gao.spb.ru
Russian Federation, Pulkovskoe sh. 65, St. Petersburg, 196140

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