Newton's Law Of Universal Gravitation

In summary: So, it's basically the only option, to the extent that the orbits really are elliptical (which is really only a good approximation).
  • #1
sheenktk
1
0
Can anyone tell me that why we take r square instead of r?
 
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  • #2
Because if we took r instead of r^2 then predictions of such theory would not fit to experimental results. Especially plredicted planet movements would not fit to observations. If we take r^2 - they fit perfectly well.
 
  • #3
The original reason why Newton did that is that the only central force law (in terms of powers of r--and this might be valid for any function of r, but I'm not sure) that produces elliptical orbits for the planets with the Sun at the focus of the ellipse. So, it's basically the only option, to the extent that the orbits really are elliptical (which is really only a good approximation).

A linear force law also produces elliptical orbits, but then the Sun would have to be at the center of the ellipses, which is not what we see.

Newton's law of gravity was one of his greatest achievements because he was able to demonstrate these facts using Euclidean geometry. His proofs are complicated, but they are described in a somewhat readable form in Brackenridge's book, The Key to Newton's Dynamics (I say it's complicated, but it's possible to give a fairly simple outline of the main points, which is done in the first few chapters--unfortunately, I am too rusty on it to describe it here, and I never found the time to finish the rest of the book).There may also be other explanations for the r^2 (I saw one in a book about quantum field theory, and you could derive it as some sort of limiting case in general relativity).
 
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  • #4
Imagine we are talking about light instead of gravity for a moment...

A bulb emits light at a rate of 1 watt. If you construct a sphere around the bulb with a radius of 1 meter then the total interior surface area of the sphere is 4pi and the intensity of the light striking the interior is 1/4pi watts per square meter.

If the sphere were 2 meters in diameter then the surface area would be 16pi and the intensity of the light striking the interior is 1/16pi watts per square meter.

As you can see, the intensity of light striking the interior of the sphere is inversely proportional to the square of it's radius.

Now if we imagine that a mass is a source radiating gravitons just like a light bulb radiates photons the reason for the inverse square law becomes obvious.
 
  • #5
homeomorphic said:
A linear force law also produces elliptical orbits, but then the Sun would have to be at the center of the ellipses,

Yeah, like shown here:

[URL]http://bluelyon.files.wordpress.com/2011/02/isaac-Newton-pound-note.jpg[/URL]

Trajectories for different laws of gravity:

http://megaswf.com/serve/1161536
 
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Related to Newton's Law Of Universal Gravitation

1. What is Newton's Law of Universal Gravitation?

Newton's Law of Universal Gravitation is a physical law that describes the force of gravity between two objects with mass. It states that every object in the universe attracts every other object with a force directly proportional to the product of their masses and inversely proportional to the square of the distance between them.

2. Who discovered Newton's Law of Universal Gravitation?

Isaac Newton discovered and published the Law of Universal Gravitation in his famous work, Principia Mathematica, in 1687. This law is one of the three laws of motion that form the basis of classical mechanics.

3. How does Newton's Law of Universal Gravitation relate to other laws of physics?

Newton's Law of Universal Gravitation is a fundamental law of physics that explains the force of gravity between objects. It is closely related to the laws of motion, as it is based on the principles of mass, acceleration, and force. It also plays a crucial role in understanding the motion of celestial bodies and the structure of the universe.

4. What factors affect the strength of gravitational force according to Newton's Law of Universal Gravitation?

The strength of gravitational force between two objects is affected by two factors: the masses of the objects and the distance between them. As the masses of the objects increase, the force of gravity between them increases. On the other hand, as the distance between the objects increases, the force of gravity decreases.

5. Is Newton's Law of Universal Gravitation still relevant today?

Yes, Newton's Law of Universal Gravitation is still relevant today and is widely used in various fields of science and engineering. While it has been superseded by Einstein's theory of general relativity in certain situations, Newton's law is still accurate for most everyday applications and remains an essential concept in our understanding of the physical world.

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