Newtonian Gravity: How GR Affects F=GMm/d^2

In summary: Newtonian mechanics to calculate things at extremely high speeds, they found that it was inaccurate. However, Newtonian mechanics still works well enough for predicting things on a smaller scale. Say, for example, we're trying to predict the movement of a person on a scale of 100 meters. Newtonian mechanics will be just fine for that. But if we're trying to predict the movement of a person on a scale of 10 meters, Newtonian mechanics will start to become inaccurate.In summary, Newtonian mechanics are accurate for predicting things on a smaller scale, but become inaccurate at speeds near the speed of light.
  • #1
Stratosphere
373
0
What exactly was wrong with Newtons gravity. I understan that GR says that gravity is the curveture of space and time. However if Newton was wrong wouldn't that mean that F= GMm/d^2 is actualy wrong?
 
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  • #2
Stratosphere said:
What exactly was wrong with Newtons gravity. I understan that GR says that gravity is the curveture of space and time. However if Newton was wrong wouldn't that mean that F= GMm/d^2 is actualy wrong?

Newtonian mechanics is also "wrong" at speeds near c. Do you see us abandoning Newton's laws when we build houses and buildings?

You need to look at under what conditions the classical description are no longer accurate. It doesn't mean that they are wrong. It just means that they work very well, within the accuracy that we need, only within certain range of conditions.

Zz,.
 
  • #3
Stratosphere said:
What exactly was wrong with Newtons gravity. I understan that GR says that gravity is the curveture of space and time. However if Newton was wrong wouldn't that mean that F= GMm/d^2 is actualy wrong?
For all eternity, predictions made on basis of Newtonian mechanics will remain as precise as they always have been.
 
  • #4
So F= GMm/d^2 is correct?
 
  • #5
No. It is approximately correct in a limited domain (but a very useful domain to us).
 
  • #6
How limited are we talking?
 
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  • #7
depends, we don't usually well actually we never travel anywhere near the speed of light maybe some pilots (usually military) travel past the speed of sound which is only a very and i mean very small fraction of the speed of light so in order for Newtonian physics to start to appear wrong is about 10 percent of C, though it's always wrong but very, very slightly at normal speeds. (that's only SR)
 
  • #8
again sound travels very, very, very slow compared to the speed of light
 
  • #9
You have to remember that no physics equations are really 'right' per se. They are just models to describe what we see, some models are better then others others are valid in different circumstances.

Newtons model describes gravity in every day life well enough, but like TOE said at 0.1C things start to go wrong. This is where GR model takes over.

Neither are right or wrong, just valid in different circumstances.
 
  • #10
Stratosphere said:
How limited are we talking?

How limited you're talking depends on how accurate you want to predict ;) .
 
  • #11
One of the first experimental tests of GR was its prediction of the rate of precession of the perihelion of Mercury. Newtonian gravity predicted a rate of 5557 seconds of arc per century. The actual measured value is 5600 seconds of arc per century, consistent with Einstein's prediction from GR.

http://phyun5.ucr.edu/~wudka/Physics7/Notes_www/node98.html

Differences between GR and Newtonian gravity are largest for Mercury's orbit because it's closest to the sun and experiences the strongest gravitational field. For the other planets, the differences are a lot smaller. If you don't need to deal with that level of precision, Newtonian gravity works fine on the scale of the solar system.
 
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  • #12
jtbell said:
One of the first experimental tests of GR was its prediction of the rate of precession of the perihelion of Mercury. Newtonian gravity predicted a rate of 5557 seconds of arc per century. The actual measured value is 5600 seconds of arc per century, consistent with Einstein's prediction from GR.
That was more of a post-diction than a prediction. That 43 arcsecond per century discrepancy was a known problem with Newtonian gravity at the end of the 19th century. The first successful prediction of GR was the bending of a ray light from some remote star as the ray passed by the Sun. GR predicted this result before it was observed in solar eclipses.

That 43 seconds of arc per century discrepancy between prediction and measurement is a tribute to 19th astronomers. First thing to note: 43 seconds of arc per century is an incredibly small number. It is equal to 0.00012 degrees per year. It would take three million years to accumulate an error of 360 degrees. That astronomers could even see such a discrepancy using 19th technology is quite amazing.

Second thing to note: Calculating what Newtonian mechanics predicts for the precession requires a precise understanding of the Earth's rotation (~5026 arc seconds per century of Mercury's apparent precession arises from the precession of the Earth's rotation axis), precise estimates of the masses and orbits of the other planets (~531 arc seconds per century of Mercury's precession arises from interactions with other planets), and doing all of the hairy calculations with pencil and paper. Another tribute to 19th astronomers and mathematicians.GR makes itself apparent much more readily in terms of time rather than position. Our GPS receivers would give incredibly bad positions if the special and general relativistic effects on clocks were not taken into account.
 
  • #13
ZapperZ said:
Newtonian mechanics is also "wrong" at speeds near c. Do you see us abandoning Newton's laws when we build houses and buildings?
Zz,.
When experimenters (Pound and Rebka (Harvard), 1959) put a Mossbauer Effect experiment iron-57 14.4 keV photon source at the top of a 73.8 foot tower (roof of physics building) and a detector in the basement, the experiment showed that when the photons fall to the ground, their energy increases (doppler shift). Although the energy shift due to gravity was very small (about 1 part in 10^15), the measured energy shift agreed with GR predictions to about 1%. So both apples photons gain energy when falling from trees or tall buildings.
 

1. What is Newtonian Gravity?

Newtonian Gravity is a theory proposed by Sir Isaac Newton in the 17th century that explains the force of gravity between two objects. It states that every object in the universe attracts every other object with a force that is directly proportional to the product of their masses and inversely proportional to the distance between them.

2. How does General Relativity (GR) affect the equation F=GMm/d^2?

In General Relativity, the equation F=GMm/d^2 still holds true, but the concept of gravity is explained differently. GR proposes that gravity is not a force between objects, but rather the curvature of space and time caused by the presence of mass. This curvature affects the motion of objects and is described by Einstein's field equations.

3. What is the difference between Newtonian Gravity and General Relativity?

The main difference between Newtonian Gravity and General Relativity is the way they explain the force of gravity. Newtonian Gravity describes gravity as a force between objects, while General Relativity explains it as the curvature of space and time caused by mass. Additionally, General Relativity is a more comprehensive theory that can explain phenomena such as black holes and the bending of light.

4. How does GR affect our understanding of the universe?

General Relativity has greatly impacted our understanding of the universe by providing a more accurate and comprehensive explanation of gravity. It has also helped us understand the behavior of objects in extreme conditions, such as near black holes. GR has also been confirmed through various experiments and observations, solidifying its place in our understanding of the universe.

5. Why is it important to study Newtonian Gravity and GR?

Studying Newtonian Gravity and General Relativity is important because they provide us with different perspectives on the force of gravity and its effects on the universe. While Newtonian Gravity is still useful for many practical applications, GR helps us understand phenomena on a larger scale, such as the behavior of galaxies and the expansion of the universe. Additionally, studying these theories can also lead to further advancements and discoveries in the field of physics.

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