Astrometric baseline observations of solar system bodies


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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.

作者简介

A. Devyatkin

Central (Pulkovo) Astronomical Observatory

编辑信件的主要联系方式.
Email: adev@gao.spb.ru
俄罗斯联邦, Pulkovskoe sh. 65, St. Petersburg, 196140

D. Gorshanov

Central (Pulkovo) Astronomical Observatory

Email: adev@gao.spb.ru
俄罗斯联邦, Pulkovskoe sh. 65, St. Petersburg, 196140

V. L’vov

Central (Pulkovo) Astronomical Observatory

Email: adev@gao.spb.ru
俄罗斯联邦, Pulkovskoe sh. 65, St. Petersburg, 196140

S. Tsekmeister

Central (Pulkovo) Astronomical Observatory

Email: adev@gao.spb.ru
俄罗斯联邦, Pulkovskoe sh. 65, St. Petersburg, 196140

M. Chubey

Central (Pulkovo) Astronomical Observatory

Email: adev@gao.spb.ru
俄罗斯联邦, Pulkovskoe sh. 65, St. Petersburg, 196140

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