Kepler's equation oor Italiaans
Kepler's equation
en
(mathematics, astronomy) the mathematical relationship between the mean anomaly (M) and the eccentric anomaly (E) of a planet in an elliptical orbit with eccentricity ( \textstyle \epsilon ). M = E - \epsilon \cdot \sin(E).
Vertalings in die woordeboek Engels - Italiaans
equazione di Keplero
en
mathematics
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Vertoon algoritmies gegenereerde vertalings
voorbeelde
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Voorbeelde moet herlaai word.
In particular, the Kepler equation should be valid for a spinning spiderweb.
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The Kepler equation follows directly from this.
oppure valori equivalenti in caso di impiego di un tipo di apparecchio diverso da quello che soddisfa tali requisitiLiterature Literature
The eccentric anomaly is the can opener and Kepler's equation is the spoon.
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So the exact calculation does not validate the simplified model leading to the Kepler equation.
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The Kepler equation depends on these facts.
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The Kepler equation therefore predicts a mass distribution proportional to the cube of the radius.
Anche a livello strettamente politico è necessario rafforzare la popolazione .Literature Literature
In mathematics, the Laplace limit is the maximum value of the eccentricity for which a solution to Kepler's equation, in terms of a power series in the eccentricity, converges.
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KEPLER’S LAW Newton’s law of gravity, together with his equation F = ma, explain Kepler’s law.
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What differential equations did for them Kepler’s model of elliptical orbits is not exact.
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Newton found that, for two bodies, this equation can be solved, and the result is Kepler’s ellipse.
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His earliest memoir, dealing with an analytical expression for the rectification of the ellipse, is published in the Transactions of the Royal Society of Edinburgh (1796); and this and his later papers on Cubic Equations (1799) and Kepler's Problem (1802) evince great facility in the handling of algebraic formulae.
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According to historical documents and calculations based on Kepler’s equations, a lunar eclipse occurred on that day, and not a solar eclipse, which may have been visible from Jerusalem.
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The Kepler problem is maximally superintegrable, since it has three degrees of freedom (d = 3) and five independent constant of motion; its Hamilton–Jacobi equation is separable in both spherical coordinates and parabolic coordinates, as described below.
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The equation (6.12) expresses Kepler's third law: The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.
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His equation of the centre for these planets remained the most accurate until the time of Johannes Kepler in the 17th century.
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The equations of Newton’s gravitational theory, which provide the theoretical foundations of Kepler’s celestial mechanics and seem to describe so well the gravitational force at all macroscopical scales, are not... Maurizio Gasperini in Theory of Gravitational Interactions (2017) Look Inside Get Access
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Using Kepler's third law of planetary motion, the observed period of the planet's orbit around the star (equal to the period of the observed variations in the star's spectrum) can be used to determine the planet's distance from the star (r {\displaystyle r}) using the following equation:
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The same holds true for all known physical laws in modern physics, including Newton’s three laws of classical mechanics, Kepler’s laws on the rotation of planets, various laws on the behaviour of gases, fluids, and levers, the first law of thermodynamics on the conservation of energy, the second law of thermodynamics on growing entropy, diverse laws of radiation, numerous laws of electrostatics, electrodynamics, electricity, and magnetism, (summarised in Maxwell’s four equations of electromagnetism), laws of wave theory, Einstein’s famous law on the equivalence of mass and energy, Schrödinger’s wave equation of quantum mechanics, and so on.
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18 sinne gevind in 7 ms. Hulle kom uit baie bronne en word nie nagegaan nie.