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相关论文: Keplers's Equation and Angular Momentum: Historica…

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Kepler's orbits with corrections due to Special Relativity are explored using the Lagrangian formalism. A very simple model includes only relativistic kinetic energy by defining a Lagrangian that is consistent with both the relativistic…

地球与行星天体物理 · 物理学 2016-04-21 Tyler J. Lemmon , Antonio R. Mondragon

The aim of this note is to compare the averaged optimal coplanar transfer towards circular orbits when the costs are the transfer time transfer and the energy consumption. While the energy case leads to analyze a 2D Riemannian metric using…

最优化与控制 · 数学 2015-08-25 Bernard Bonnard , Helen Henninger , Jana Nemcova , Jean-Baptiste Pomet

In classical mechanics, the Kepler potential and the Harmonic potential share the following remarkable property: in either of these potentials, a bound test particle orbits with a radial period that is independent of its angular momentum.…

经典物理 · 物理学 2021-02-25 Paul Ramond , Jérôme Perez

Up to now, the rotational velocities of galaxies are not clearly understood and the experimental Tully Fisher rule, linking the total galactic mass to the fourth power of the velocity, through an acceleration coefficient of about 10-10 m/s2…

综合物理 · 物理学 2016-10-21 Jacques Fleuret

Proceeding like Newton with a discrete time approach of motion and a geometrical representation of velocity and acceleration, we obtain Kepler's laws without solving differential equations. The difficult part of Newton's work, when it calls…

科普物理 · 物理学 2009-11-13 J. -P. Provost , C. Bracco

The formalism of classical particle dynamics is reinvestigated according to the basic requirement of causal consistency, and a new equation of particle dynamics, which is more general and more in line with classical mechanics experiments…

天体物理学 · 物理学 2016-02-03 ChiYi Chen

We prove that the classical Lambert theorem about the elapsed time on an arc of Keplerian orbit extends without change to the Kepler problem on a space of constant curvature. We prove that the Hooke problem has a property similar to…

数学物理 · 物理学 2019-10-15 Alain Albouy , Lei Zhao

Newton's Theorem of Revolving Orbits derives the force that is necessary to explain a particular precession that leaves the shape of an orbit unchanged. Newton showed that for an orbiting body that is already subject to any central force,…

经典物理 · 物理学 2024-05-06 Nolan Samboy , Joseph Gallant

An earlier paper [1] presented a gravity theory based on the optics of de Broglie waves rather than curved space-time. While the universe's geometry is flat, it agrees with the standard tests of general relativity. A second paper [2] showed…

天体物理学 · 物理学 2007-05-23 Kris Krogh

In the Special Theory of Relativity space and time intervals are different in different frames of reference. As a consequence, the quantity 'velocity' of classical mechanics splits into different quantities in Special Relativity, coordinate…

物理教育 · 物理学 2007-05-23 Thomas Greber , Heinz Blatter

We derive a simple analytical expression for the two-body force in a sub-class of MOND-like theories and make testable predictions in the modification to the two-body orbital period, shape, and precession rate, and escape speed etc. We…

星系天体物理 · 物理学 2010-11-11 Hongsheng Zhao , Baojiu Li , Olivier Bienaymé

We investigate perturbations in the Kepler problem. We offer an overview of the dynamical system using Newtonian, Lagrangian and Hamiltonian Mechanics to build a foundation for analyzing perturbations. We consider the effects of a…

经典物理 · 物理学 2022-11-30 Jesse Dimino

The long-term dynamical evolution of a Keplerian binary orbit due to the emission and absorption of gravitational radiation is investigated. This work extends our previous results on transient chaos in the planar case to the three…

广义相对论与量子宇宙学 · 物理学 2009-10-31 C. Chicone , B. Mashhoon , D. G. Retzloff

We analytically derive the secular changes of the orbital parameters, i.e., energy, angular momentum, and Carter constant, for general bound orbits in Kerr spacetime, at leading order in the mass ratio, through the 6th post-Newtonian (6PN)…

广义相对论与量子宇宙学 · 物理学 2026-03-31 Norichika Sago , Ryuichi Fujita , Soichiro Isoyama , Hiroyuki Nakano

The regularities in the structure of the planetary system, expressed by the Titius-Bode law, can be accounted also by using a more general formula, derived not by fit but from a logarithmic integrality constraint on the angular momentum…

经典物理 · 物理学 2021-12-21 M. Grigorescu

The gravitational action of the smooth energy-matter components filling in the universe can affect the orbit of a planetary system. Changes are related to the acceleration of the cosmological scale size R. In a universe with significant…

天体物理学 · 物理学 2008-11-26 M. Sereno , Ph. Jetzer

The longitudinal Doppler shift is a measure of hyperbolic distance. Transformations of uniform motion are determined by the Doppler shift, while its square root transforms to a uniformly accelerated frame. A time-velocity space metric is…

综合物理 · 物理学 2008-05-16 B. H. Lavenda

Using the Hamiltonian formulation, we have attempted to obtain the equations of motion of systems with internal angular momentum that are moving with respect to a reference system when subjected to an interaction. This interaction involves…

化学物理 · 物理学 2007-05-23 Manuel Dorado Gonzalez

Newton's deduction of the inverse square law from Kepler's ellipse and area laws together with his "superb theorem" on the gravitation attraction of spherically symmetric bodies, are the major steps leading to the discovery of the law of…

历史与综述 · 数学 2014-08-29 Wu-Yi Hsiang , Eldar Straume

Orbital motion of a body can be found from Newtonian equation of motion. However, it is useful to express the motion through time derivatives of Keplerian orbital elements, mainly if the motion is perturbed by small perturbing force. The…

天体物理仪器与方法 · 物理学 2009-07-27 P. Pastor