celestial mechanics oor Masedonies
celestial mechanics
en
(astronomy) The dynamics of celestial bodies subject to mutual gravitational attraction.
Vertalings in die woordeboek Engels - Masedonies
небесен механизам
en
branch of astronomy
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He was something of a child prodigy, having two papers on binary orbits (celestial mechanics) published before he was sixteen.
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Poincaré published two now classical monographs, "New Methods of Celestial Mechanics" (1892–1899) and "Lectures on Celestial Mechanics" (1905–1910).
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Eventually, he held the chairs of Physical and Experimental Mechanics, Mathematical Physics and Theory of Probability, and Celestial Mechanics and Astronomy.
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As a mathematician and physicist, he made many original fundamental contributions to pure and applied mathematics, mathematical physics, and celestial mechanics.
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Two gravitational constants are commonly used in Solar system celestial mechanics: G, the Newtonian gravitational constant and k, the Gaussian gravitational constant.
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Often in celestial mechanics, the primary body is much larger than any of the secondary bodies of the system, that is, M ≫ m.
Распучија, немој, не, не!WikiMatrix WikiMatrix
The term "dynamics" came in a little later with Gottfried Leibniz, and over a century after Newton, Pierre-Simon Laplace introduced the term "celestial mechanics."
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Poincaré made many contributions to different fields of pure and applied mathematics such as: celestial mechanics, fluid mechanics, optics, electricity, telegraphy, capillarity, elasticity, thermodynamics, potential theory, quantum theory, theory of relativity and physical cosmology.
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Ordinary differential equations appear in celestial mechanics (planets, stars and galaxies); numerical linear algebra is important for data analysis; stochastic differential equations and Markov chains are essential in simulating living cells for medicine and biology.
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According to Robert A. Millikan, in pure science, Gibbs "did for statistical mechanics and for thermodynamics what Laplace did for celestial mechanics and Maxwell did for electrodynamics, namely, made his field a well-nigh finished theoretical structure".
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In celestial mechanics, this is usually a Keplerian ellipse, which is correct when there are only two gravitating bodies (say, the Earth and the Moon), or a circular orbit, which is only correct in special cases of two-body motion, but is often close enough for practical use.
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Aside from successfully applying his analytic tools to problems in classical mechanics, Euler also applied these techniques to celestial problems.
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They say the Antikythera Mechanism, dating from the # st century BC, was probably used to calculate the astronomical cycles of celestial bodies
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Cosmology as a science originated with the Copernican principle, which implies that celestial bodies obey identical physical laws to those on Earth, and Newtonian mechanics, which first allowed us to understand those physical laws.
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The celestial scenes can be created using a wide variety of technologies, for example precision-engineered 'star balls' that combine optical and electro-mechanical technology, slide projector, video and fulldome projector systems, and lasers.
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15 sinne gevind in 5 ms. Hulle kom uit baie bronne en word nie nagegaan nie.