Gravitational Potential Energy引力势能
Gravitational potential energy is energy an object possesses because of its position in a gravitational field. The most common use of gravitational potential energy is for an object near the surface of the Earth where the gravitational acceleration can be assumed to be constant at about 9.8 m/s2. Since the zero of gravitational potential energy can be chosen at any point (like the choice of the zero of a coordinate system), the potential energy at a height h above that point is equal to the work which would be required to lift the object to that height with no net change in kinetic energy. Since the force required to lift it is equal to its weight, it follows that the gravitational potential energy is equal to its weight times the height to which it is lifted. 引力势能是物体由于处于引力场中的位置而具有的能量。引力势能最常见的应用是对于接近地球表面的物体,其中引力加速度可以假设为常数,约为9.8 m/s²。由于引力势能的零点可以任选(就像坐标系的零点选择一样),相对于该点的高度h处的势能等于将物体提升到该高度所需的功,且在此过程中动能无明显变化。由于提升物体所需的力等于其重量,因此引力势能等于其重量乘以提升的高度。
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Gravitational Potential Energy引力势能
The general expression for gravitational potential energy arises from the law of gravity and is equal to the work done against gravity to bring a mass to a given point in space. Because of the inverse square nature of the gravity force, the force approaches zero for large distances, and it makes sense to choose the zero of gravitational potential energy at an infinite distance away. The gravitational potential energy near a planet is then negative, since gravity does positive work as the mass approaches. This negative potential is indicative of a "bound state"; once a mass is near a large body, it is trapped until something can provide enough energy to allow it to escape. The general form of the gravitational potential energy of mass m is: 引力势能的通用表达式来源于万有引力定律,并等于将质量带到空间中某一点所作的反抗重力的功。由于重力的平方反比性质,当距离很大时,力会趋于零,因此合理地将引力势能的零点选择在无限远处。因此,靠近行星的引力势能是负的,因为质量接近时重力做正功。这种负的势能表明了一个‘束缚态’;一旦质量接近大质量天体,它就会被束缚住,直到有足够能量使其逃脱。质量m的引力势能的一般形式为:
![]() where G is the gravitation constant, M is the mass of the attracting body, and r is the distance between their centers. 其中,G 是引力常量,M 是吸引物体的质量,r 是它们中心之间的距离。这是计算从地球引力逃逸速度时最常用的引力势能形式。
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Gravitational Potential Energy引力势能
From the work done against the gravity force in bringing a mass in from infinity where the potential energy is assigned the value zero, the expression for gravitational potential energy is 从将质量从无穷远处带来时赋予势能零值所作的 against 重力 力 的 功,可得到引力势能的表达式
![]() This expression is useful for the calculation of escape velocity, energy to remove from orbit, etc. However, for objects near the earth the acceleration of gravity g can be considered to be approximately constant and the expression for potential energy relative to the Earth's surface becomes 这个表达式对于计算逃逸速度、从轨道中移除所需的能量等很有用。然而,对于接近地球的物体,重力加速度 g 可以认为近似为常数,因此相对于地球表面的势能表达式变为
![]() where h is the height above the surface and g is the surface value of the acceleration of gravity. 其中h是物体表面以上的高度,g是表面处的重力加速度。
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Gravitational Potential重力势能
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Gravitational Potential Integral引力势积分
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