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单词 Newtonian gravitational constant
释义

Newtonian gravitational constant

中文百科

万有引力常数 Gravitational constant

(重定向自Newtonian gravitational constant)
万有引力常数G,在两个物体(M1、M2)之间的影响。

万有引力常数(记作 G ),是一个包含在对有质量的物体间的万有引力的计算中的实验物理常数。它出现在牛顿的万有引力定律和爱因斯坦的广义相对论中。也称作重力常数牛顿常数。不应将其与小写的 g 混淆,后者是局部引力场(等于局部引力引起的加速度),尤其是在地球表面。

根据万有引力定律,两物体间的吸引力( F )与二者的质量( m1m2 )的乘积成正比,而与他们之间的距离( r )的平方成反比:

其中的比例常数 G 即是万有引力常数。

万有引力常数大概是物理常数中最难测量的了。在国际单位制的单位中,2010年的科学技术数据委员会推荐的万有引力常数值为:

英语百科

Gravitational constant 万有引力常数

(重定向自Newtonian gravitational constant)
The gravitational constant G is a key quantity in Newton's law of universal gravitation.

The gravitational constant is approximately 6.6741×10 N⋅m/kg and denoted by the letter G, is an empirical physical constant involved in the calculation(s) of gravitational force between two bodies. It usually appears in Sir Isaac Newton's law of universal gravitation, and in Albert Einstein's general theory of relativity. It is also known as the universal gravitational constant, Newton's constant, and colloquially as Big G. It should not be confused with "small g" (g), which is the local gravitational field of Earth (equivalent to the free-fall acceleration).

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更新时间:2025/6/17 20:07:01