Hall's solution for Mercury's precession

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In summary, Hall's research showed that a slight change in the exponent of Newton's equation would result in precession. If the exponent was slightly less than 2, the resulting angle between minimum and maximum radius vector for an orbit of small eccentricity would be determined by the formula \theta = {\pi \over {\sqrt{n+3}}}, where n is the new exponent used in the equations of motion. Hall also mentions that if n = -2, the equation would follow Newton's law.
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Shaw
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Hall showed that a slight increase in the radius exponent in Newton's equation would cause precession. What would the result be if the exponent was slightly less than 2.
 
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FWIW:
http://books.google.com/books?id=eQY-AQAAMAAJ&pg=RA1-PA49&cad=2#v=onepage&q&f=false

In which Hall gives a formula, attributed to Bertrand,

[itex]\theta = {\pi \over {\sqrt{n+3}}}[/itex]

where [itex]\theta[/itex] is the angle between minimum and maximum radius vector for an orbit of small eccentricity, and [itex]n[/itex] is the exponent to be used in the equations of motion. He says, "If [itex]n = -2[/itex] we have the Newtonian law." So I imagine you can figure it out from there.
 
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  • #3
Thanks for this. I must be thick, but I'm still a bit puzzled.
 

1. What is Hall's solution for Mercury's precession?

Hall's solution for Mercury's precession is a mathematical model that explains the observed anomaly in Mercury's orbit around the Sun. It takes into account the gravitational pull of the other planets in the solar system and accurately predicts the precession of Mercury's orbit.

2. How does Hall's solution differ from Newton's theory of gravity?

Hall's solution includes the effects of general relativity, which Newton's theory of gravity does not. It also takes into account the gravitational influence of the other planets, while Newton's theory only considers the Sun's gravitational pull.

3. Why is it important to understand Mercury's precession?

Mercury's precession is important because it provides evidence for Einstein's theory of general relativity, which revolutionized our understanding of gravity. It also helps us better understand the dynamics of the solar system and can be used to make more accurate predictions about future planetary orbits.

4. How was Hall's solution for Mercury's precession developed?

Hall's solution was developed through a combination of mathematical calculations and observations of Mercury's orbit. Scientists used data from previous observations and refined the equations until they accurately predicted Mercury's observed precession.

5. Can Hall's solution be applied to other planets?

Yes, Hall's solution can be applied to other planets in the solar system. However, it may need to be modified to account for the specific characteristics of each planet's orbit and the gravitational influences of other nearby planets.

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