CONSTRUCTION OF 3D-MAPS SUBLIMATION ZONES FOR MAIN SPACE ICES IN SOLAR SYSTEM. QUALITY CHEMICAL ANALYSIS OF THE POSSIBLE COMPOSITION OF ATMOSPHERES OF THE CLASSICAL PLANETS SATELLITES, TRANSNEPTUNIAN OBJECTS AND COMETS

In the work a quantitative analysis of the photometry of the Gravitational Microlensing Phenomenon
(GMP) of a background star of the Milky Way by a Massive Dark Body (MDB), located on the
Solar System Periphery (SSP) are made in the case of five model bodies. The total luminous flux and
its magnification (A) are calculated. Formulas for the microlensing time (T0) and mass of microlens
are obtained. It is shown that in the case of the Nemesis/Tyuche models, the strong microlensing
for their registration are realized almost in the entire Space of Model Free Parameters (SMFP) and
optimal conditions of registration are achieved at the upper boundary of the Interval Possible Values of Heliocentric Distances (IPVHD).