Construction of an areocentric areoequatorial coordinate system from photographic material obtained by the interplanetary probes Mars-4 and Mars-5

Physics

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Mars Photographs, Photomapping, Planetocentric Coordinates, Mars Probes, Mars Surface, Projection, Root-Mean-Square Errors, U.S.S.R. Space Program

Scientific paper

The method and results of construction of a set of reference points in an areocentric areoequatorial coordinate system from photographic material obtained in 1974 by the interplanetary probes Mars-4 and Mars-5 are presented. Two approaches to the use of coordinates of projection centers, obtained during the construction of the reference set, to define the orbit of the probe are examined. It is shown that a 6-parameter solution with evaluation of the phase coordinates of the probe is less effective than an 8-parameter solution which also provides the radius and gravitational constant of Mars.

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