Solving Kepler's 3rd Law with 4π²/G

In summary, by substituting the given values for G, 1 year, 1 AU, and 1 solar mass into the equation 4\pi^{2}/G = 1yr^{2} M_{Sun}/AU^{3}, we can prove that Kepler's 3rd Law reduces to P^{2}=a^{3}/(m_{1}+m_{2}) when the period P is expressed in years, the semimajor axis a is expressed in AU, and the sum of the masses is expressed in solar masses. However, it should be noted that the units in this equation do not cancel completely, and a unit conversion factor is still carried through the final result.
  • #1
tony873004
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Show that
[tex]4\pi^{2}/G = 1yr^{2} M_{Sun}/AU^{3} [/tex]
and that therefore Kepler's 3rd Law reduces to
[tex]P^{2}=a^{3}/(m_{1}+m_{2})[/tex]
if the period P is expressed in years, the semimajor axis a is expressed in AU, and the sum of the masses is expressed in solar masses.

[tex]G = 6.672*10^{-11}Nm^{2}/kg^{2}[/tex]
[tex]N = kg m/s^{2}[/tex]
[tex]1 year = 3.15581*10^{7}seconds[/tex]
[tex]1 AU = 1.49598*10^{11}meters[/tex]
[tex]1 Solar mass = 1.9891*10^{30}kg[/tex]


[tex]\frac{4\pi^{2}}{6.672*10^{-11} \frac{N m^{2}}{kg^{2}}}=\frac {3.15581*10^{7}s^{2}*1.9891*10^{30}kg}{1.49598*10^{11}m^{3}}[/tex]


Substitute [tex]kg m/s^{2} for N[/tex]

[tex]\frac{4\pi^{2}}{6.672*10^{-11} \frac{kg\frac{m}{s^{2}} m^{2}}{kg^{2}}}=\frac {3.15581*10^{7}s^{2}*1.9891*10^{30}kg}{1.49598*10^{11}m^{3}}[/tex]

in the left side of the equation, cancel kg's and combine m's

[tex]\frac{4\pi^{2}}{6.672*10^{-11} \frac{\frac{m^{3}}{s^{2}}}{kg}}=\frac {3.15581*10^{7}s^{2}*1.9891*10^{30}kg}{1.49598*10^{11}m^{3}}[/tex]

re-write the equation

[tex]{4\pi^{2} * 1.49598*10^{11}m^{3} = 6.672*10^{-11} \frac{\frac{m^{3}}{s^{2}}}{kg} * 3.15581*10^{7}s^{2}*1.9891*10^{30}kg [/tex]

The m^3 on the right cancels with the m^3 on the left
the s^2's in the left side of the equation cancel with each other since one is in the denomanator of a fraction, and the other one isn't.
The kg's in the left side of the equation cancel with each other since one is in the denomanator of a fraction, and the other one isn't.

[tex]{4\pi^{2} * 1.49598*10^{11} = 6.672*10^{-11} * 3.15581*10^{7}*1.9891*10^{30} [/tex]

and when I compute this I get:

[tex]591702901743.965 = 4.1881622988912*10^{27}[/tex]
and that's just not right! Where did I go wrong?
 
Last edited:
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  • #2
[tex] 1 \mbox{year} = 3.15581 \cdot 10^7 \mbox{s} \Longrightarrow (1 \mbox{year})^2 = (3.15581 \cdot 10^7 \mbox{s})^2 \neq 3.15581 \cdot 10^7 \mbox{s}^2[/tex]

similarly for [tex]\mbox{AU}^3[/tex].
 
  • #3
:smile: Thanks, Data. That's the 2nd time you've bailed me out in the last 2 days.

I also made a small error in G. Should be [tex]6.673*10^{-11}[/tex], not [tex]6.672*10^{-11}[/tex]

So this should change my final line before computing the numbers to:

[tex]{4\pi^{2} * 1.49598*10^{33} = 6.673*10^{-11} * 3.15581*10^{14}*1.9891*10^{30} [/tex]

which gives me
[tex]5.90589231677665*10^{34} = 4.1887900210583*10^{34}[/tex]

They're not too different. At least they're in the same magnitude instead of being 16 magnitudes apart. I'm wondering if this is as good as it gets or if I made another error somewhere?

Any idea how to do the 2nd part of this question, how does this cause Kepler's 3rd law to reduce to [tex]P^{2}=a^{3}/(m_{1}+m_{2})[/tex] ?
 
Last edited:
  • #4
Almost. You forgot to square the 3.15581, and cube the 1.49598!

The second question is a really ambiguous one. In order to get it to that form, you must assume that both sides of the equation are unitless (otherwise, you keep the fraction [tex]\frac{\mbox{yr}^2}{\mbox{AU}^3}[/tex] on the right side of the equality to balance units). This in turn means you just assume the result for P is in years, etc., which is silly. Anyways, Kepler's Third Law is

[tex]P^2 = \frac{a^3}{m_1+m_2}\cdot \frac{4\pi^2}{G}[/tex]

Just substitute in the equality that you proved in the first part, and see how far you can get~
 
  • #5
Thanks, Data. I squared and cubed those numbers, and now the answers are equal. I got the second part too. I had to make a new value for G, which equaled 4pi^2, they canceled out and I was left the equation I was asked to justify.
 
  • #6
You set [tex]G = 4 \pi^2[/tex]? With what justification?
 
  • #7
[tex]G=6.673*10^{-11}N m^{2}/kg^{2}[/tex] , therefore
[tex]G=6.673*10^{-11}kg (m/s^{2}) m^{2}/kg^{2}[/tex]

substitute in the conversions from mks to AU, Solar Masses, Years

0.00000000006673 * ((1 / 1.9891E+30) * (1 / 149598000000#) / (1 / 31558100) ^ 2#) * (1 / 149598000000# ^ 2 / (1 / 1.9891E+30) ^ 2)

and magically the whole thing equals exactly 4pi^2
Sorry, I didn't feel like TEXing it.

By converting all the units in G to AU, Years, and Solar Masses. Now G cancels out with 4pi^2
[tex]P^2 = \frac{a^3}{m_1+m_2}\cdot \frac{4\pi^2}{G}[/tex]

reduces to

[tex]P^{2}=a^{3}/(m_{1}+m_{2})[/tex]

Which is what the question asked me to do.
 
  • #8
Ok, that's fine. Make sure you leave in the unit conversion term, though (ie. the magnitude equals the magnitude of [tex]4\pi^2[/tex], but there are still units hanging around that [tex]4\pi^2[/tex] does not carry). You really can't simplify it to the form in your question, as there's always a unitary conversion factor lying around. But whatever, I guess they want you to write it that way :)
 
  • #9
Yeah, those units bugged me too. So I just dropped them all together 2 steps before my final answer. When the teacher talked about this one in class, everyone had a blank stare. But she hinted that this was the way to do it. At least I'll get effort points!

Thanks for all your help, Data!
 
  • #10
I asked in class today. The units do carry down to the 1.0 computed with 4pi^2/G. Then when you replace the 4pi^2/G in the Kepler's law with 1.0&units, the units cancel with the units in the rest of Kepler's law so that P^2 comes out in years.
 
  • #11
I agree, but then the [tex]P, \ a, \ m_1, \ m_2[/tex] in your new equation aren't the same ones in the original equation (the new ones are unitless). Essentially the point is that [tex] \mbox{time} \neq \frac{\mbox{distance}}{\mbox{mass}}[/tex].
 

1. What is Kepler's 3rd Law?

Kepler's 3rd Law, also known as the Harmonic Law, states that the square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.

2. What is the significance of solving Kepler's 3rd Law with 4π²/G?

By using the equation 4π²/G, where G is the gravitational constant, we can calculate the orbital period of a planet based on its distance from the sun. This allows us to better understand the relationship between a planet's orbital period and its distance from the sun.

3. How is the value of G determined in solving Kepler's 3rd Law?

The value of G was determined through experiments by Sir Isaac Newton and is considered a fundamental constant in physics. It is often referred to as the universal gravitational constant and is used in calculations related to planetary motion and other gravitational interactions.

4. Can Kepler's 3rd Law be used for any planet in our solar system?

Yes, Kepler's 3rd Law can be used for any planet in our solar system, as long as we have accurate measurements of its orbital period and semi-major axis. It can also be applied to other celestial bodies, such as moons and comets.

5. How does solving Kepler's 3rd Law with 4π²/G help us understand the universe?

By using this equation, we can determine the orbital periods of planets and other celestial bodies in our solar system and beyond. This helps us better understand the laws of gravity and how objects move in space. It also allows us to make predictions and calculations for future space missions and explorations.

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