Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984em%26p...30....1k&link_type=abstract
Earth, Moon, and Planets (ISSN 0167-9295), vol. 30, Feb. 1984, p. 1-19.
Astronomy and Astrophysics
Astronomy
5
Astronomical Catalogs, Astronomical Coordinates, Lunar Craters, Lunar Photography, Reference Stars, Selenography, Astrometry, Calibrating, Celestial Reference Systems, Coordinate Transformations, Ephemerides, Lunar Surface, Tables (Data)
Scientific paper
The selenocentric coordinates of 263 craters and one mountain are given. The scale and orientation of the selenocentric coordinates system are determined by star-calibrated lunar photographs obtained with the long-focus horizontal telescope. The origin of the system is defined by the theory of the motion of the moon. The physical libration is taken into account for the reduction of the coordinates system to the principal axes of the lunar inertia. The reference stars coordinates are reduced to the FK4 system. The position of the lunar mass center is determined by LURE-2 theory, the rotation parameters are taken from the Migus tables (Migus, 1980).
Khabibullin Sh. T.
Risvanov N. G.
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