Inverse Problem of the Lunar Physical Libration by Observing Stars from the Lunar Surface

Details Inverse Problem of the Lunar Physical Libration by Observing Stars from the Lunar Surface Inverse Problem of the Lunar Physical Libration by Observing Stars from the Lunar Surface

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1027p&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1027

Physics

Scientific paper

Method of solution of the inverse problem is suggested. The dependence
of accuracy of libration angles on the measuring error of selenographic
coordinates of stars is estimated. Their sensitivity to deformability of
the Moon is verified.

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