从月球探测器改善了月球的重力场
1A. S. Konopliv, A. B. Kucinskas, W. L. Sjogren, J. G. Williams, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA. A. B. Binder, Lunar Research Institute, Gilroy, CA 95020, USA. L. L. Hood, University of Arizona,
概括
月球探测器 (LP) 的数据揭示了月球附近盆地的新月球巨星,并部分解决了四个远端巨星. 这种改进的重力模型支持一个半径为220-450公里的铁芯.
科学领域:
- 行星科学 行星科学
- 地质物理学 地质物理学
- 月球科学 月球科学
背景情况:
- 月球探测器 (LP) 航天器为重力建模提供了关键数据.
- 了解月球巨星是解读月球内部结构和演变的关键.
研究的目的:
- 开发一个改进的月球重力模型,使用LP的多普勒跟踪数据.
- 为了识别和描述月球近侧和远侧的质量度 (mascons).
主要方法:
- 利用了月球探测器 (LP) 航天器的多普勒追踪数据.
- 开发了一种改进的重力模型来分析质量分布.
主要成果:
- 在Mare Humboltianum,Mendel-Ryberg和Schiller-Zucchius撞击盆地下面的月球近面发现了三个新的mascons.
- 在远端盆地部分解决了四个巨石:赫茨普隆,库伦布-萨顿,弗洛因德利希-沙罗诺夫和马雷莫斯科文斯.
- 确定了一个改进的正常化的极性惯性瞬间 (0.3932 ± 0.0002),与月球铁核 (半径220-450公里) 一致.
结论:
- 改进的重力模型增强了我们对月球巨石和内部结构的理解.
- 这些发现提供了强有力的证据,证明月球内部有一个重要的铁芯.
- LP数据继续为月球地质和地物理提供宝贵的见解.
相关概念视频
Gravity between Spherical Bodies
Newton's law of gravitation describes the gravitational force between any two point masses. However, for extended spherical objects like the Earth, the Moon, and other planets, the law holds with an assumption that masses of spherical objects are concentrated at their respective centers.
This assumption can be proved easily by showing that the expression for gravitational potential energy between a hollow sphere of mass (M) and a point mass (m) is the same as it would be for a pair of extended...
This assumption can be proved easily by showing that the expression for gravitational potential energy between a hollow sphere of mass (M) and a point mass (m) is the same as it would be for a pair of extended...
Acceleration due to Gravity on Other Planets
The gravitational acceleration of an object near the Earth's surface is called the acceleration due to gravity. It can be measured by conducting simple experiments on Earth. However, such an experiment is impossible to conduct on the surface of other planets.
Astronomical observations are thus used to measure the acceleration due to gravity on other planets. This can be determined by observing the effect of a planet's gravity on objects close to it. The crucial factor that helps in this...
Astronomical observations are thus used to measure the acceleration due to gravity on other planets. This can be determined by observing the effect of a planet's gravity on objects close to it. The crucial factor that helps in this...
Variation in Acceleration due to Gravity near the Earth's Surface
An object's apparent weight is its weight measured by a spring balance at its location. It is different from its true weight, the force with which the Earth pulls it, because of the Earth's rotation. Mathematically, an object's apparent weight equals its true weight minus the centripetal force that keeps it in a circular motion along with the Earth's surface every 24 hours.
The difference between the true and apparent weights is proportional to the square of the Earth's angular speed. Since the...
The difference between the true and apparent weights is proportional to the square of the Earth's angular speed. Since the...
Tidal Forces
The origin of Earth's ocean tides has been a subject of continuous investigation for over 2000 years. However, the work of Newton is considered to be the beginning of the proper understanding of the phenomenon. Ocean tides are the result of gravitational tidal forces. These same tidal forces are present in any astronomical body; they are responsible for the internal heat that creates the volcanic activity on Io, one of Jupiter's moons, and the breakup of stars that get too close to black holes.
Simple Harmonic Motion and Uniform Circular Motion
While simple harmonic motion and uniform circular motion may be two separate concepts, they correlate and interlink with each other. Simple harmonic motion is an oscillatory motion in a system where the net force can be described by Hooke's law, while uniform circular motion is the motion of an object in a circular path at constant speed.
There is an easy way to produce simple harmonic motion by using uniform circular motion. For instance, consider a ball attached to a uniformly rotating...
There is an easy way to produce simple harmonic motion by using uniform circular motion. For instance, consider a ball attached to a uniformly rotating...
Gravitation
In the years before Newton, a general belief prevailed that different laws governed objects in the sky than objects on Earth. When Kepler wrote down the three laws of planetary motion, explaining in detail the geometrical properties of the planetary orbits around the Sun, there was no immediate idea to discern their connection with more fundamental laws. It was Isaac Newton who, in 1665–66, figured out the connection between planetary motion, the motion of the moon around the Earth, and the...


