Orbit Relativistic orbital motion
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spacetime, with orbits following geodesics, provides a more accurate calculation and understanding of the exact mechanics of orbital motion. Historically...- Orbital elements are the parameters required to uniquely identify a specific orbit. In celestial mechanics these elements are considered in two-body systems...
body if perturbations were absent. That is, it is the orbit that coincides with the current orbital state vectors (position and velocity). The word osculate...- spin–orbit interaction (also called spin–orbit effect or spin–orbit coupling) is a relativistic interaction of a particle's spin with its motion inside...
In quantum mechanics there are analogous orbital and spin angular momenta which describe the orbital motion of a particle, represented as quantum mechanical...
A Rosetta orbit is a complex type of orbit. In astronomy, a Rosetta orbit occurs when there is a periastron shift during each orbital cycle. A retrograde...
{\displaystyle m_{s}} . The simple names s orbital, p orbital, d orbital, and f orbital refer to orbitals with angular momentum quantum number ℓ = 0, 1, 2...- ground movement and interplanetary travel is supported, including orbital and sub-orbital flight, although only vessel-ground collisions are supported. Docking...
Apsidal precession (redirect from Apsidal motion)main orbital elements of an orbit. Apsidal precession is considered positive when the orbit's axis rotates in the same direction as the orbital motion. An...- Angular momentum coupling (redirect from Orbit-orbit coupling)accentuates spin–orbit coupling effect. Thus, for example, uranium molecular orbital diagrams must directly incorporate relativistic symbols when considering...
- their physical and orbital parameters can be determined. For example, out of the six independent parameters that define an orbit, the radial-velocity...
per second (1,040 mph). The Earth is also orbiting around the Sun in an orbital revolution. A complete orbit around the Sun takes one year, or about 365 days;...- Two-body problem in general relativity (redirect from Relativistic two body problem)two-body problem in general relativity (or relativistic two-body problem) is the determination of the motion and gravitational field of two bodies as described...
- revolving orbits identifies the type of central force needed to multiply the angular speed of a particle by a factor k without affecting its radial motion (Figures 1...
Angular momentum (redirect from Orbital angular momentum vector)type of non-orbital angular momentum called "spin", but this angular momentum does not correspond to a spinning motion. In relativistic quantum mechanics...- circumference of the orbit is 2π (~6.283) metres. The period of the motion is 2π seconds per turn. The frequency is (2π)−1 hertz. During circular motion, the body...
- {\displaystyle mv^{2}/r} . Many orbits, such as that of the Moon around the Earth, can be approximated by uniform circular motion. In such cases, the centripetal...
Three-body problem (category Orbits)laws of motion and Newton's law of universal gravitation. It has no general closed-form solution, unlike two-body problems. When three bodies orbit each...
Fine structure (section Relativistic corrections)the Hamiltonian: the leading order relativistic correction to the kinetic energy, the correction due to the spin–orbit coupling, and the Darwin term coming...
Essential Relativistic Celestial Mechanics. London: Adam Hilger. ISBN 0-7503-0062-0. Horizons output (30 January 2011). "Barycentric Osculating Orbital Elements...
- theory of the motion of the Earth's Moon as deduced from the principles of gravitational theory (especially the Newtonian, non-relativistic theory). The
- PROBLEM OF MOTION, Ann. Math. 39:65-100, Jan. 1938. Investigation of the extent to which the relativistic equations of gravitation determine the motion of ponderable
- dilation that occurs as a result of relativistic physics. Another notable example from celestial mechanics is the orbit of Mercury, which experiences precessional