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Qualitatively, how would your weight be different if you weighed yourself:

  1. $100\text{Km}$ above the earth?
  2. $100\text{Km}$ above the moon?
  3. near the equator if the earth's rotation were $10\text{h}$?

I don't know how to even start this question.

entrelac
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Ella
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  • Is gravity stronger or weaker when you do something like that? – krvolok Aug 20 '15 at 11:08
  • Also, for c) think about what a centrifugal force does when you speed up rotation. – krvolok Aug 20 '15 at 11:08
  • I am pretty sure that gravity would get weaker, but I don't know how to calculate a specific value. I also don't quite know what it means when it says that earth's rotation is 10h. – Ella Aug 20 '15 at 11:11
  • $F=m\omega^2R_{equator}$ is the centrifugal force. $\omega = \frac{2\pi}{T}$, where $T$ is the period of rotation. Usually, it's $T=24h$ :) – krvolok Aug 20 '15 at 11:20
  • I am afraid I have not been introduced to the centrifugal force, what is it? And what is 'the period of rotation'? – Ella Aug 20 '15 at 11:32
  • I suggest you check your notes. It would be very unusual to ask a question like this without having first said something about "centripetal force", "centrifugal force", "centrifugal effect", or similar words. Unless this is an exercise in getting you to do some research, in which case you should do that. – David K Aug 20 '15 at 13:41

3 Answers3

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OK, you know the gravitational law:

$$F = \frac{G M m}{r^2} $$

where $M$ is the mass of the earth and $m$ is your mass.

You weigh, on the surface of the earth

$$F_0 = \frac{G M m}{R_e^2} $$

where $R_e$ is the radius of the earth. Your weight at a height $h$ above is

$$F_h = \frac{G M m}{(R_e+h)^2} $$

Can you now compare these weights?

Ron Gordon
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  • How do you do the 100km above the moon part of the question, doesn't that equation only apply to earth? – Ella Aug 20 '15 at 11:17
  • Change to the radius of the moon and the mass of the moon. The equation is universal. – Ron Gordon Aug 20 '15 at 11:18
  • Ok. Can you explain to me what it means if the rotation of the earth is 10h? – Ella Aug 20 '15 at 11:20
  • There's a small effect that is, at the equator, proportional to the frequency of rotation squared, which is $m R_e \omega^2$. The earth's rotation being 10h means the rotation frequency increases, so the weight increases. – Ron Gordon Aug 20 '15 at 11:38
  • what does the m,Re and w stand for? – Ella Aug 20 '15 at 11:46
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  1. We know that the value of Earth's gravitational acceleration on the surface is given as $$g=\frac{Gm_e}{R_e^2}=9.81$$

Where, $M_e=\text{mass of Earth}=6\times 10^{24}\ kg$ & $R_e=\text{radius of Earth}=6400\ km$

Consider an object of wight $W$ on the Earth's surface

Then, the weight of the object at a height $h$ from the Earth's surface is given by Newton's Law of Gravitation $$mg'=\frac{GM_em}{(R_e+h)^2}$$ $$=\frac{GM_em}{R_e^2\left(1+\frac{h}{R_e}\right)^2}$$ $$=\frac{mg}{\left(1+\frac{h}{R_e}\right)^2}$$

Hence, if $mg=\text{weight on the Earth's surface}=W$

then the weight $W'$ of the object at the height $h=100\ km$ is $$W=\frac{W}{\left(1+\frac{100}{6400}\right)^2}$$ then the weight $W'$ of the object at the height $h=100\ km$ is $$W'=\frac{W}{\left(1+\frac{100}{6400}\right)^2}$$ $$W'=\frac{W}{\left(1+\frac{100}{6400}\right)^2}$$$$=\left(\frac{64}{65}\right)^2W$$ $$\color{blue}{W'=\frac{4096 W}{4225}=\frac{4096 }{4225}\times \text{(weight on the surface of Earth)}}$$

  1. Now, for moon, take the radius of moon $R_m=1737\ km$ & acceleration due to Moon's gravity as $\frac{g}{6}$ where, $g=\text{Earth's gravitational acceleration}$

Hence, at the height $h=100\ km$ from the surface of moon the weight $W''$ of object

$$W''=\frac{m\frac{g}{6}}{\left(1+\frac{100}{1737}\right)^2}$$ $$W''=\frac{\frac{W}{6}}{\left(1+\frac{100}{1737}\right)^2}$$$$=\frac{W}{6}\left(\frac{1737}{1837}\right)^2$$ $$\color{blue}{W''=\frac{3017169 W}{20247414}\approx (0.149)\times \text{(weight on the surface of Earth)}}$$

  1. We know that gravitational acceleration of Earth $g'$ due to Earth's rotation velocity $\omega$ is given as $$\color{red}{g'=g-2\omega^2R_e\cos^2\lambda}$$ Where, $\lambda=\text{angle of latitude of the point from equator}$ & $\omega=\text{angular velocity (in rad/sec)}$

But, at the equator plane $\lambda=0$ hence, the weight of the object $$W'=m(g-2\omega^2R_e\cos^20)$$ $$W'=m(g-2\omega^2R_e)$$

& for rotation time $10$ hrs we get $$\omega=\frac{2\pi}{10\times 3600}=\frac{\pi}{18000}\ rad/sec$$

Now, setting the values of mass, $m$, $g=9.81$ at the pole, $\omega=\frac{\pi}{18000}\ rad/sec$ & $R_e=6400000\ m$

weight can be calculated as $$\color{blue}{W'=m(g-2\omega^2R_e)}$$ I hope you may solve the remaining part.

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I think the key to answering this question is the word qualitatively.

The question is not asking you to calculate how much you will weigh at these various places. It is asking you whether you would weigh the same, less, or more than you do now.

David K
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