Determination of secular polar motion from astronomical observations. The priority of O. Ya. Orlov

1Korsun, AA
1Main Astronomical Observatory of the National Academy of Sciences of Ukraine, Kyiv, Ukraine
Kinemat. fiz. nebesnyh tel (Online) 2016, 32(2):74-80
Start Page: Research in the History of Astronomy
Language: Ukrainian
Abstract: 

The purpose of this publication is to pay attention to the priority of the well-known astronomer and geophysicist, member of the Academy of Sciences of UkrSSR A. Ya. Orlov (1880—1954) in the determination of such parameters of the secular polar motion of the Earth as its speed (4 mas/year) and direction (69°W). His results obtained in 1954 were based on the astronomical observations made in the period from 1900 to 1950 with zenith-telescopes at international latitude stations. A. Ya. Orlov is well-known as the founder of the Poltava gravimetric observatory, the Main astronomical observatory, and of the school of global geodynamics, but his pioneer work on secular polar motion based on the data of astronomical observations turned out to be little known. At the present, these first secular polar motion estimates obtained by Orlov have been verified by the century-long observations (from 1900 to 2012) with different telescopes at many observatories in the world and by different methods, astronomical as well as cosmic (LLS, VLBI, GNSS, etc.).

Keywords: latitude station, secular polar motion, zenith-telescope
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