GRAVITY FIELD IN EXTERNAL PARTS OF THE SOLAR SYSTEM

Автор(и)

  • N. V. Bazey Department of Astronomy, Odessa National University, T.G.Shevchenko Park, Odessa. 65014, Ukraine, Україна
  • A. A. Bazey Astronomical Observatory, Odessa National University, T.G.Shevchenko Park, Odessa. 65014, Ukraine,, Україна

DOI:

https://doi.org/10.18524/1810-4215.2012.25.83155

Ключові слова:

nearest stars, attraction, potential energy, galactic center

Анотація

Taking into account the gravitational perturbations from the center of the galaxy and using the catalogue closest to the Sun, stars modeled surfaces of equal gravitational potential energy fields in the outskirts of the solar system. Constructed three-dimensional model of equipotential surfaces in the vicinity of the solar system. It is shown that for certain values a constant of the energy the Sun is within the common equipotential surface Toliman, Sirius and Procyon.

Посилання

Balk M.: 1965, Elements of space flight dynamics, Moscow, “Science”, 338 pp. (in Russian)

Binney J., Merrifield M.: 1998, The Galactic Astronomy, Princeton University Press, 796 pp.

Oort J.: 1950, Bull. Astron. Inst. Neth., 11, 91.

Chebotarev G.: 1965, Analytic and numerical methods of Celestial Mechanics, Moscow, “Science”, 368 pp. (in Russian)

Zakhozhaj V.: 1979, Vestnik Khar’kovskogo Universiteta, 190, 52.

NASA, Voyager, http://voyager.jpl.nasa.gov/news/ new−region.html

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Опубліковано

2012-11-15

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