Аннотация:The new hypsometric maps of Venus and the Moon should improve and accelerate studying the surfaces of these planets
and relief-forming processes. Additionally, these maps should be useful for students and scientists. The hypsometric
map of Venus is produced in Lambert equal-area azimuth projection. Its height contours are obtained using the
Magellan altitude data. To create Lunar Subpolar relief map the authors obtained heights from the A. Cook et.al. raster
image of South Lunar Subpolar region (latitudes from -60° to -90°) being constructed in stereographic projection.
[A.C. Cook, T.R. Watters, M.S. Robinson et.al. (2000) JGR, Vol.105, E5, 12023-12033]. Morphometric investigations
of Venus and Lunar South Pole region surface have been fulfilled using our databases. The height profiles of some
lunar craters being situated here and detailed profiles of the whole this area created by us describe the features of this
region surface with the high resolution up to 100 meters.