Venera-D Mission Scenario and Trajectory


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The article describes the trajectory scenario for the Venera-D mission. The main aspects of optimal launch dates are considered. A scenario, which enables insertion of an orbiter into a highly elliptical orbit and a lander on the surface of Venus is described. Characteristics of the choice for operational orbit and scenario ensuring scientific data transfer from the lander on the surface of Venus to the Earth are justified. In addition, possibilities of transfer of a small satellite to the vicinity of the collinear Lagrangian point of the Sun-Venus system, and also a subsatellite into the orbit of the main orbiter, are considered.

作者简介

N. Eismont

Space Research Institute, Russian Academy of Sciences

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Email: neismont@iki.rssi.ru
俄罗斯联邦, Moscow

L. Zasova

Space Research Institute, Russian Academy of Sciences

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Email: zasova@iki.rssi.ru
俄罗斯联邦, Moscow

A. Simonov

Lavochkin Association

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Email: alex.simonov@laspace.ru
俄罗斯联邦, Khimki, Moscow oblast, 141402

I. Kovalenko

Space Research Institute, Russian Academy of Sciences

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Email: irina.kovalenko@iki.rssi.ru
俄罗斯联邦, Moscow

D. Gorinov

Space Research Institute, Russian Academy of Sciences

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Email: dmitry_gorinov@rssi.ru
俄罗斯联邦, Moscow

A. Abbakumov

Space Research Institute, Russian Academy of Sciences

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Email: abbakumov@romance.iki.rssi.ru
俄罗斯联邦, Moscow

S. Bober

Space Research Institute, Russian Academy of Sciences

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Email: stasbober@rlab.iki.rssi.ru
俄罗斯联邦, Moscow

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