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| Content Provider | Springer Nature Link |
|---|---|
| Author | Ivav, M. A. Zasova, L. V. Gerasimov, M. V. Korablev, O. I. Marov, M. Ya. Zelenyi, L. M. Ignat’ev, N. I. Tuchin, A. G. |
| Copyright Year | 2017 |
| Abstract | We discuss a change in the resurfacing regimes of Venus and probable ways of forming the terrain types that make up the surface of the planet. The interpretation of the nature of the terrain types and their morphologic features allows us to characterize their scientific priority and the risk of landing on their surface to be estimated. From the scientific point of view, two terrain types are of special interest and represent easily achievable targets: the lower unit of regional plains and the smooth plains associated with impact craters. Regional plains are probably a melting from the upper fertile mantle. The material of smooth plains of impact origin is a well-mixed and representative sample of the Venusian crust. The lower unit of regional plains is the most widespread one on the surface of Venus, and it occurs within the boundaries of all of the precalculated approach trajectories of the lander. Smooth plains of impact origin are crossed by the approach trajectories precalculated for 2018 and 2026. |
| Starting Page | 1 |
| Ending Page | 19 |
| Page Count | 19 |
| File Format | |
| ISSN | 00380946 |
| Journal | Solar System Research |
| Volume Number | 51 |
| Issue Number | 1 |
| e-ISSN | 16083423 |
| Language | English |
| Publisher | Pleiades Publishing |
| Publisher Date | 2017-02-16 |
| Publisher Place | Moscow |
| Access Restriction | One Nation One Subscription (ONOS) |
| Subject Keyword | Venus resurfacing regimes Venera-D mission landing sites Astronomy, Astrophysics and Cosmology Planetology Astronomy, Observations and Techniques Astrophysics and Astroparticles |
| Content Type | Text |
| Resource Type | Article |
| Subject | Astronomy and Astrophysics Space and Planetary Science |
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