51. Estimates of abundance of the short-baseline (1-3 meters) slopes for different Venusian terrains using terrestrial analogues
- Author
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Oleg Korablev, L. V. Zasova, Mikhail A. Ivanov, L. M. Zeleny, M. Gerasimov, M. Ya. Marov, and Nikolay Ignatiev
- Subjects
010504 meteorology & atmospheric sciences ,biology ,Mode (statistics) ,Astronomy and Astrophysics ,Venus ,Terrain ,biology.organism_classification ,01 natural sciences ,Planetary science ,Space and Planetary Science ,Abundance (ecology) ,0103 physical sciences ,Range (statistics) ,Frequency distribution ,Baseline (configuration management) ,010303 astronomy & astrophysics ,Geomorphology ,Geology ,0105 earth and related environmental sciences ,Remote sensing - Abstract
The interplanetary mission, Venera-D, which is currently being planned, includes a lander. For a successful landing, it is necessary to estimate the frequency distributions of slopes of the Venusian surface at baselines that are comparable with the horizontal dimensions of lander (1–3 m). The available data on the topographic variations on Venus preclude estimates of the frequency of the short-wavelength slopes. In our study, we applied high-resolution digital terrain models (DTM) for specific areas in Iceland to estimate the slopes on Venus. The Iceland DTMs have 0.5 m spatial and 0.1 m vertical resolution. From the set of these DTMs, we have selected those that morphologically resemble typical landscapes on Venus such as tessera, shield, regional, lobate, and smooth plains. The mode of the frequency distribution of slopes on the model tessera terrain is within a 30°–40° range and a fraction of the surface has slopes
- Published
- 2017
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