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翻訳と辞書　辞書検索 [ 開発暫定版 ] スポンサード リンク Gravitational acceleration ： ウィキペディア英語版 Gravitational acceleration (詳細はphysics, gravitational acceleration is the acceleration on an object caused by force of gravitation. Neglecting friction such as air resistance, all small bodies accelerate in a gravitational field at the same rate relative to the center of mass.〔 〕 This equality is true regardless of the masses or compositions of the bodies. At different points on Earth, objects fall with an acceleration between 9.78 and 9.83 m/s2 depending on altitude and latitude, with a conventional standard value of exactly 9.80665 m/s2 (approximately 32.174 ft/s2). Objects with low densities do not accelerate as rapidly due to buoyancy and air resistance. == For point masses == Newton's law of universal gravitation states that there is a gravitational force between any two masses that is equal in magnitude for each mass, and is aligned to draw the two masses toward each other. The formula is: :$F\; =\; G\; \backslash frac\backslash$ where $m\_1$ and $m\_2$ are the two masses, $G$ is the gravitational constant, and $r$ is the distance between the two masses. The formula was derived for planetary motion where the distances between the planets and the Sun made it reasonable to consider the bodies to be point masses. (For a satellite in orbit, the 'distance' refers to the distance from the mass centers rather than, say, the altitude above a planet's surface.) If one of the masses is much larger than the other, it is convenient to define a gravitational field around the larger mass as follows:〔 〕 :$\backslash mathbf=-\; \backslash mathbf\}$ is a unit vector directed from the large mass to the smaller mass. The negative sign indicates that the force is an attractive force. In that way, the force acting upon the smaller mass can be calculated as: :$\backslash mathbf\; =\; m\; \backslash mathbf$ where $\backslash mathbf$ is the force vector, $m$ is the smaller mass, and $\backslash mathbf$ is a vector pointed toward the larger body. Note that $\backslash mathbf$ has units of acceleration and is a vector function of location relative to the large body, independent of the magnitude (or even the presence) of the smaller mass. This model represents the "far-field" gravitational acceleration associated with a massive body. When the dimensions of a body are not trivial compared to the distances of interest, the principle of superposition can be used for differential masses for an assumed density distribution throughout the body in order to get a more detailed model of the "near-field" gravitational acceleration. For satellites in orbit, the far-field model is sufficient for rough calculations of altitude versus period, but not for precision estimation of future location after multiple orbits. The more detailed models include (among other things) the bulging at the equator for the Earth, and irregular mass concentrations (due to meteor impacts) for the Moon. The ''Gravity Recovery And Climate Experiment'' (GRACE) mission launched in 2002 consists of two probes, nicknamed "Tom" and "Jerry", in polar orbit around the Earth measuring differences in the distance between the two probes in order to more precisely determine the gravitational field around the Earth, and to track changes that occur over time. Similarly, the ''Gravity Recovery and Interior Laboratory'' (GRAIL) mission from 2011-2012 consisted of two probes ("Ebb" and "Flow") in polar orbit around the Moon to more precisely determine the gravitational field for future navigational purposes, and to infer information about the Moon's physical makeup. 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Gravitational acceleration」の詳細全文を読む スポンサード リンク 翻訳と辞書 : 翻訳のためのインターネットリソース Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.