Resonant Orbits in the Problem of Expanding the Reachable Landing Areas on the Surface of Venus View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

2021-05

AUTHORS

N. A. Eismont, R. R. Nazirov, K. S. Fedyaev, V. A. Zubko, A. A. Belyaev, L. V. Zasova, D. A. Gorinov, A. V. Simonov

ABSTRACT

We consider the concept of applying gravity assist maneuvers near Venus using resonant orbits with a period equal to the Venusian one. We show that the proposed operations based on this concept allow the reachable landing areas on the surface of Venus to be expanded radically. The price of this approach is an increase of the time interval needed to solve this problem by a value equal to the orbital period of Venus. The cost of the characteristic velocity in this case remains within limits close to the standard variants of planning missions to Venus. More... »

PAGES

316-330

References to SciGraph publications

  • 1988-07. Physical parameters of the atmosphere of Venus in EARTH, MOON, AND PLANETS
  • 1993-10. Physical parameters of the atmosphere of Venus from Venera 15 and 16 missions in EARTH, MOON, AND PLANETS
  • 2019-12. Venera-D Mission Scenario and Trajectory in SOLAR SYSTEM RESEARCH
  • 2014-10-05. Revisiting Lambert’s problem in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1134/s1063773721050042

    DOI

    http://dx.doi.org/10.1134/s1063773721050042

    DIMENSIONS

    https://app.dimensions.ai/details/publication/pub.1140298347


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