orbital eccentricity oor Hebreeus

orbital eccentricity

Vertalings in die woordeboek Engels - Hebreeus

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parameter that determines the amount by which an orbit deviates from a perfect circle
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For Earth's current orbital eccentricity, incoming solar radiation varies by about 6.8%, while the distance from the Sun currently varies by only 3.4% (5.1 million km).
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However, Newton extends his theorem to an arbitrary central forces F(r) by restricting his attention to orbits that are nearly circular, such as ellipses with low orbital eccentricity (ε ≤ 0.1), which is true of seven of the eight planetary orbits in the solar system.
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Despite of this, it has an eccentric orbit of 27.7%.
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Dr. Thompson thinks it was a rogue that got pulled into an eccentric polar orbit.
אבל אם התכמון הזה נועד לעבוד עליי, הוא לא מתוחכם במיוחדOpenSubtitles2018.v3 OpenSubtitles2018.v3
Newton also applied his theorem to the planet Mercury, which has an eccentricity ε of roughly 0.21, and suggested that it may pertain to Halley's comet, whose orbit has an eccentricity of roughly 0.97.
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Propositions 43–45 are demonstration that in an eccentric orbit under centripetal force where the apse may move, a steady non-moving orientation of the line of apses is an indicator of an inverse-square law of force.
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To make his theorem applicable to other types of forces, Newton found the best approximation of an arbitrary central force F(r) to an inverse-cube potential in the limit of nearly circular orbits, that is, elliptical orbits of low eccentricity, as is indeed true for most orbits in the Solar System.
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Its orbit is highly inclined and moderately eccentric, despite being at the same distance from the Sun as the central part of the asteroid belt.
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Earth's orbit will become less eccentric for about the next 100,000 years, so changes in this insolation will be dominated by changes in obliquity, and should not decline enough to permit a new glacial period in the next 50,000 years.
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He showed by general considerations, first, that the mutual action of two planets could never cause large changes in the eccentricities and inclinations of their orbits; but then, even more importantly, that peculiarities arose in the Jupiter–Saturn system because of the near approach to commensurability of the mean motions of Jupiter and Saturn.
לראות אותך שם הלילה, על רחבת הריקודים, נהנית עם בחורים בגיל שלךWikiMatrix WikiMatrix
10 sinne gevind in 8 ms. Hulle kom uit baie bronne en word nie nagegaan nie.