e/Kepler orbit

Information
has gloss	eng: In celestial mechanics, a Kepler orbit describes the motion of an orbiting body as an ellipse, parabola, or hyperbola, which forms a two-dimensional orbital plane in three-dimensional space. (A Kepler orbit can also form a straight line.) It considers only the gravitational attraction of two bodies, neglecting perturbations due to gravitational interactions with other objects, atmospheric drag, solar radiation pressure, a non-spherical central body, and so on. It is thus said to be a solution of a special case of the two-body problem, known as the Kepler problem. As a theory in classical mechanics, it also does not take into account the effects of general relativity. Keplerian orbits can be parametrized into six orbital elements in various ways.
lexicalization	eng: Kepler orbit
instance of	(noun) the path of an electron around the nucleus of an atom electron orbit, orbit

Meaning
Russian
has gloss	rus: Кеплеровы элементы — шесть элементов орбиты, определяющих положение небесного тела в пространстве в задаче двух тел: * большая полуось (a\,\!), * эксцентриситет (e\,\!), * наклонение (i\,\!), * аргумент перицентра (\omega\,\!), * долгота восходящего узла (\Omega\,\!), * средняя аномалия (M_o\,\!).
lexicalization	rus: Кеплеровы элементы орбиты

Media
media:img	Eccentricity.png
media:img	Elipse.svg
media:img	Inclination in Elliptical Orbit.png
media:img	Kepler's equation scheme.svg
media:img	NewtonsLawOfUniversalGravitation.svg
media:img	Orbit ru.svg
media:img	Orbit1.svg