A special case of the n-body problem in which a general solution can be found for the orbits of two bodies under the influence of their mutual gravitational attraction. The motion of a planet around the Sun is an example as long as the attractive forces of other planets are assumed to be...
Henssonow,Gravitational Two-Body Problem,Newton''s Theorem of Revolving Orbits,Bonnet''s Theorem,Kepler Problem,Laplace–Runge–Lenz vector,Newton''s Theorem of Revolving Orbits,Newton's Theorem of Revolving Orbits 展开 摘要: Please note that the content of this book primarily consists of articles...
The modern formulation of the two-body problemappeared for the first time in the third and last book of the Philosophiae Naturalis Principia Mathematica , the treaty that Isaac Newton published owing to a decisive stimulus and material help by Edmund Halley: unanimously considered one of the most...
two-body problem The problem in celestial mechanics that is concerned with (a) the relative motion of two point masses that are influenced only by their mutual gravitational attraction and their initial velocities relative to each other or relative to a fixed frame of reference, such as the undi...
The collision singularity in a perturbedN-body problem We present a scheme to treat properly close encounters in a three-dimensional two-body problem under perturbations. It is a combination of Sundman's time transformation and Levi-Civita's spatial coordinate transformation applied to the t... ...
It's not as if I have a huge problem with my weight, but I can see a lot of room for improvement, not least because I will soon be on a sunlounger alongside a friend whose body has never deviated from a perfect size eight. The extra half-stone from winter is still hanging around ...
二维电子气 two-dimensional electron gas 二能级系统 two-level system 二端网络 two-terminal network 双光子吸收 two-photon absorption 二流体描述 two-fluid description 双粒子格林函数 two-particle Green function 二体问题 two-body problem 双频激光器 two-frequency laser 双流不稳定性 two-stre 电力 两班...
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The horizontal angle of error, θEH tends to be equal to zero since the body axis is usually aligned with the speed vector. In some cases, however, the body axis and speed vector are not aligned, for instance during side-slip—as a result of inertia during high speed banked turns, ...
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