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翻訳と辞書　辞書検索 [ 開発暫定版 ] スポンサード リンク radial trajectory ： ウィキペディア英語版 radial trajectory In astrodynamics and celestial mechanics a radial trajectory is a Kepler orbit with zero angular momentum. Two objects in a radial trajectory move directly towards or away from each other in a straight line. == Classification == There are three types of radial trajectories (orbits).〔William Tyrrell Thomson (1986), Introduction to Space Dynamics, Dover〕 * Radial elliptic trajectory: an orbit corresponding to the part of a degenerate ellipse from the moment the bodies touch each other and move away from each other until they touch each other again. The relative speed of the two objects is less than the escape velocity. This is an elliptic orbit with semi-minor axis = 0 and eccentricity = 1. Although the eccentricity is 1 this is not a parabolic orbit. If the coefficient of restitution of the two bodies is 1 (perfectly elastic) this orbit is periodic. If the coefficient of restitution is less than 1 (inelastic) this orbit is non-periodic. * Radial parabolic trajectory, a non-periodic orbit where the relative speed of the two objects is always equal to the escape velocity. There are two cases: the bodies move away from each other or towards each other. * Radial hyperbolic trajectory: a non-periodic orbit where the relative speed of the two objects always exceeds the escape velocity. There are two cases: the bodies move away from each other or towards each other. This is a hyperbolic orbit with semi-minor axis = 0 and eccentricity = 1. Although the eccentricity is 1 this is not a parabolic orbit. Unlike standard orbits which are classified by their orbital eccentricity, radial orbits are classified by their specific orbital energy, the constant sum of the total kinetic and potential energy, divided by the reduced mass: : $\backslash epsilon\; =\; \backslash frac\; -\; \backslash frac$ where ''x'' is the distance between the centers of the masses, ''v'' is the relative velocity, and $\backslash mu=(m\_1\; +\; m\_2)$ is the standard gravitational parameter. Another constant is given by: : $w\; =\; \backslash frac\; -\; \backslash frac\; =\; \backslash frac$ *For elliptic trajectories, w is positive. It is the inverse of the apoapsis distance (maximum distance). *For parabolic trajectories, w is zero. *For hyperbolic trajectories, w is negative, It is $\backslash textstyle\; \backslash frac$ where $\backslash textstyle\; v\_$ is the velocity at infinite distance. 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「radial trajectory」の詳細全文を読む スポンサード リンク 翻訳と辞書 : 翻訳のためのインターネットリソース Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.