Аннотация:The paper presents an overview of remote sensing data used as a source one for modelling of relief features on Terrestrial planets and their satellites. In our work we analyze global active remote sensing data obtained by synthesized aperture radar (SAR) for Venus, MESSENGER laser altimeter (MLA), Lunar orbiter laser altimeter (LOLA) and Mars orbiter laser altimeter (MOLA) for Mercury, the Moon and Mars respectively. We describe in detail characteristics of space instruments and digital elevation models (DEMs) derived. Seven types of relief features identified on Mercury, Venus, Mars and the Moon were determined. There are rupēs, fossae (rimae), valles, planitiae (maria), dorsa, craters and montes. Some morphometric and morphological aspects of these features typical for each celestial body are considered too.