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Habitability of planets is a fundamental question of planetary astrophysics. Some of exoplanets possess physical settings close to those of Venus. Therefore, the planet Venus, with its dense and hot (735 K) oxygen-free atmosphere of CO2, having a high pressure of 9.2 MPa at the surface, can be a natural laboratory for this kind of studies. The only existing direct data on the planet’s surface are still the results obtained by the Soviet VENERA landers. The TV experiments of Venera-9 and 10 (October, 1975) and Venera-13 and 14 (March, 1982) delivered 41 panoramas of Venus surface or their fragments [1]. The experiments were of extreme technical complexity. There have not been any similar missions to Venus in the subsequent 42 and 35 years. The results of these missions are studied anew. The Venera images (“panoramas”) were re-examined using modern processing techniques. As a result of these studies, rather specific objects were observed. In their morphology, some of them recalled Earth living forms. Their striking similarity to terrestrial forms was called terramorphism. The number of detected objects of the hypothetical forms of the flora and fauna of Venus reaches 15.

Signs of Hypothetical Flora and Fauna of the Planet Venus: Returning to Archive of the Old TV-Experiments