Reading on Newton's law of universal gravitation

In summary, according to Newton's law of universal gravitation, the force between two objects with a mass of 50kg and 100kg, and a distance of 2 meters, is 8.34e-8 N. This is a small force and in order to feel the effects of gravity, the product of the masses would need to be at least 10^11. The inverse square dependence on distance also plays a crucial role in the strength of gravity. For example, the force between the sun and Earth can be calculated using this law. Overall, an object must have a tremendous mass before a noticeable gravitational pull can be felt. This is why we do not stick to other objects of similar mass and why the Earth is
  • #1
Ukitake Jyuushirou
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i was doing some reading on Newton's law of universal gravitation. the equation is given as mass of 2 objects divided by distances square and then multiply by gravitation constant. using 50kg and 100 kg mass and a distance of 2 metres i get a value 8.34e-8 N

this a small force, which sets me thinking. how big a force is needed between 2 objects before we start to feel the effects of gravity?
 
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  • #2
Ukitake Jyuushirou said:
i was doing some reading on Newton's law of universal gravitation. the equation is given as mass of 2 objects divided by distances square and then multiply by gravitation constant. using 50kg and 100 kg mass and a distance of 2 metres i get a value 8.34e-8 N

this a small force, which sets me thinking. how big a force is needed between 2 objects before we start to feel the effects of gravity?

As you can see from Newton's law, the force between any two masses of normal size (human beings, cars, swimming pools, etc) is quite small despite the dependence on the product of the masses. The gravitational constant goes roughly as [itex]10^{-11}[/itex] (in SI units) so in order to get what you call an appreciable force, the product of the masses should be at least as large as [itex]10^{11}[/itex]. But there is another important factor here: the inverse square dependence on distance...so the smaller the distance the better.

You can plug in values of the sun and Earth to compute the approximate force of gravitation as predicted by Newton's Law.
 
  • #3
maverick280857 said:
As you can see from Newton's law, the force between any two masses of normal size (human beings, cars, swimming pools, etc) is quite small despite the dependence on the product of the masses. The gravitational constant goes roughly as [itex]10^{-11}[/itex] (in SI units) so in order to get what you call an appreciable force, the product of the masses should be at least as large as [itex]10^{11}[/itex]. But there is another important factor here: the inverse square dependence on distance...so the smaller the distance the better.

You can plug in values of the sun and Earth to compute the approximate force of gravitation as predicted by Newton's Law.
in other words, an object needs tremendous mass b4 there is a noticeable gravitational pull?

thanks :)
 
  • #4
Of course, which is why the Earth attracts us, and in turn is kept in orbit by the sun , which is of course affected by the gravitational pull of other massive objects as black holes and other stars .
This is also the reason why we don't find ourselves sticking to each other or other objects of comparable mass .
 
  • #5
Well, you could think of it like this:
Consider 2 balls of constant equal density, radius r, and let F be the magnitude of a "noticable" force.
Furthermore, let the balls touch each other.
Then, the density must satisfy the equation:
[tex]\rho=\sqrt{\frac{F}{G}}\frac{3}{2\pi{r}^{2}}[/tex]
where G is the gravitational constant.
Given some particular radius, you'll get a measure of how huge the density will have to be in order for a noticeable force to be felt.
 
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. It states that the force of gravity is directly proportional to the product of the masses of the objects and inversely proportional to the square of the distance between them.

2.

What is the history behind Newton's law of universal gravitation?

Sir Isaac Newton first published his law of universal gravitation in his book "Principia Mathematica" in 1687. However, the concept of gravity had been studied and discussed by scientists and philosophers for centuries before Newton's discovery.

3.

How does Newton's law of universal gravitation apply to everyday life?

Newton's law of universal gravitation is responsible for the gravitational pull that keeps our feet on the ground and the planets in their orbits around the sun. It also plays a role in the tides, the motion of satellites, and the formation of galaxies.

4.

What are the limitations of Newton's law of universal gravitation?

Newton's law of universal gravitation is an approximation that works well for most situations, but it breaks down at very small distances (such as the atomic scale) and very high speeds (such as near the speed of light). It also does not take into account the effects of relativity.

5.

How does Newton's law of universal gravitation relate to Einstein's theory of general relativity?

Einstein's theory of general relativity provides a more accurate and complete understanding of gravity. It expands upon Newton's law of universal gravitation by incorporating the effects of spacetime curvature and mass-energy equivalence. However, in situations where the effects of relativity are negligible, Newton's law of universal gravitation can still be used as an effective approximation.

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