Kepler's planetary motion and inverse square law

In summary, the conversation discusses the relationship between the inverse square law of Newton's gravitational force and Kepler's laws. It is mentioned that all of Kepler's laws can be derived from the inverse square law, and that the second law holds true for any central force field.
  • #1
shounakbhatta
288
1
Hello,

The inverse square law of Newton's gravitational force, is it somehow related to each other?

I mean to say P^2 is directly prop.a^3. Is it from the third law that the derivation of inverse sq.law of G=M.m/R2 is derived?

Thanks.
 
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  • #2
You can derive all of Kepler's laws from the inverse square law of gravitation.
 
  • #3
shounakbhatta said:
Is it from [Kepler's] third law that the derivation of inverse sq.law of G=M.m/R2 is derived?

Basically, yes. This old thread has a couple of links to files that have more details. See posts #9 and #10.

https://www.physicsforums.com/showthread.php?t=399797
 
  • #4
But I think the second law is not only for inverse square rule, in fact it holds true for any centre field force([itex]\vec{F}= f(r)\vec{r}[/itex]) because [itex]\dot{S}= \frac{1}{2}r^2 \frac{dw}{dt}[/itex] where [itex]r^2 \frac{dw}{dt}[/itex] is consevative in any central force field.
 
  • #5


Yes, Kepler's three laws of planetary motion and the inverse square law of gravitation are intimately related. Kepler's third law states that the square of a planet's orbital period is directly proportional to the cube of its semi-major axis. This means that the farther a planet is from the sun, the longer it takes to complete one orbit. This law is a consequence of the inverse square law of gravitation, which states that the force between two objects is inversely proportional to the square of the distance between them. This can be derived from Newton's laws of motion and his law of universal gravitation, which states that the force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them. So, in short, Kepler's third law is a result of the inverse square law of gravitation.
 

Related to Kepler's planetary motion and inverse square law

1. What is Kepler's planetary motion?

Kepler's planetary motion refers to the laws of planetary motion discovered by German astronomer Johannes Kepler in the early 17th century. These laws describe the motion of planets around the sun and are fundamental to our understanding of the solar system.

2. What are the three laws of Kepler's planetary motion?

The first law states that planets move in elliptical orbits with the sun at one focus. The second law, also known as the law of equal areas, states that a line connecting a planet to the sun will sweep out equal areas in equal times. The third law, also known as the harmonic law, states that the square of a planet's orbital period is directly proportional to the cube of its semi-major axis.

3. What is the inverse square law in relation to Kepler's laws?

The inverse square law is a mathematical principle that describes the relationship between the distance and intensity of a force. In the case of Kepler's laws, the inverse square law explains how the force of gravity between two objects decreases as the distance between them increases, following an inverse square relationship.

4. How did Kepler's laws contribute to our understanding of the solar system?

Kepler's laws provided a more accurate and comprehensive explanation of planetary motion compared to previous models, such as the geocentric model. They also paved the way for future developments in the field of celestial mechanics and helped shape our understanding of the laws of physics.

5. Are Kepler's laws still relevant today?

Yes, Kepler's laws are still considered fundamental principles in the field of astronomy and are used to accurately predict the movements of planets and other celestial bodies. They have also been expanded upon and incorporated into more complex models of the solar system, such as Newton's laws of motion and Einstein's theory of general relativity.

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