Satellite Orbital Speed at 10% Gravity

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Homework Help Overview

The discussion revolves around determining the height above the Earth where the acceleration due to gravity is 10% of its surface value, as well as the orbital speed of a satellite at that height. The subject area includes gravitational physics and orbital mechanics.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning, Problem interpretation

Approaches and Questions Raised

  • Participants explore the relationship between gravitational acceleration at different heights and how to manipulate the given formulas to isolate the height. There are questions about the meaning of 10% gravity and how to apply it in calculations. Some participants suggest using the Universal Law of Gravitation and emphasize the importance of visualizing the problem.

Discussion Status

The discussion includes various attempts to clarify the problem and approaches to solving it. Some participants provide algebraic insights and derivations, while others express confusion and seek further guidance. There is no explicit consensus on the best approach, but several productive lines of reasoning have been shared.

Contextual Notes

Participants note the challenge of interpreting the problem's wording and the need for a clear understanding of the gravitational concepts involved. There is mention of the original poster's struggle with the initial setup and the potential for misunderstanding the formulas.

TonkaQD4
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(a) At what height above the Earth is the acceleration due to gravity 10% of its value at the surface?
(b) What is the speed of a satellite orbiting at that height?

Note: _e means earth

g = { g_e / [1+(h/R_e)^2] }

At height 0, g = 9.83m/s^2
R = 6400km

I know that we need to isolate "h". I don't quite understand how to start this problem though. Where do we plug in that 10% or what exactly does that 10% mean? I guess the wording of the question is what makes this problem confusing. Help me start this please.
 
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The acceleration of a mass at the surface is [tex]a_0[/tex]

The acceleration of a mass at some height x above the surface is [tex]a_1[/tex]

You want to know what x is when [tex]\frac{a_1}{a_0}[/tex]=0.1

The rest is simple algebra.
 
That doesn't help me out.

Any other suggestions out there.
 
Maybe think about it this way... you have a formula that gives you some g for any value of h that you want to plug in.

Unfortunately, you need a formula that gives you the h for some value of g. That's ok, you can plug in your value for g (once you figure it out) and manipulate the equation.

Maybe if you saw Bill's equation with g's instead of a's:

g1 / g0 = 0.1 , where g0 is the acceleration due to gravity at h = 0. You can solve this for g1, which will be, in this case, 10% (0.1) of the acceleration due to gravity at h = 0.

Hope this helps.
 
Should I use the Universal Law of Gravitation instead?

F = GmM/r^2

Still not sure what to do then? I feel like I am making this problem harder than it really is.
 
Well, you probably are making this problem a bit harder than it is, but everyone does that until it 'clicks'.

Have you drawn a picture? I get the impression that you're trying to plug numbers into formulas, but you're not sure which formulas to use or why because you don't have a physical picture of what's going on. I would suggest drawing a picture. What happens to the gravitational force as you move away from the surface of the earth?

Now, as for whether or not you should use the formula for the gravitational force, you already are using it-- you just don't know it yet. Check out the following derivation, which I believe is accurate (I'm slightly out of practice :-)-- if anyone notices anything, please jump in. Now,

[tex]F = ma = \frac{GM_{e}m}{r^2}[/tex]

and since we're calling the acceleration due to gravity g, not a,

[tex]F = mg = \frac{GM_{e}m}{r^2} \Rightarrow{g = \frac{GM_{e}}{r^2}}[/tex]

So now, at the surface of the earth, [itex]r = R_e[/itex], so

[tex]g_e = \frac{GM_{e}}{{R_e}^2}[/tex]

Now, at some height above the surface of the Earth [itex]R_e[/itex], [itex]r = R_e + h[/itex], so the acceleration due to gravity there would be

[tex]g = \frac{GM_{e}}{r^2} = \frac{GM_{e}}{(R_e+h)^2}[/tex]

Now, using these two results, we can calculate the ratio [itex]\frac{g_e}{g}[/itex]:

[tex]\frac{g_e}{g} = \frac{\frac{GM_{e}}{{R_e}^2}}{\frac{GM_{e}}{(R_e+h)^2}} = \frac{(R_e + h)^2}{{R_e}^2} = \frac{{R_e}^2(1+\frac{h}{R_e})^2}{{R_e}^2} = (1+\frac{h}{R_e})^2[/tex]

so

[tex]\frac{g_e}{g} = (1+\frac{h}{R_e})^2 \Rightarrow g = \frac{g_e}{(1+\frac{h}{R_e})^2}[/tex]

Which is the formula (almost; I think you may have mis-typed it) you were originally going to use. And you should, it will help you with part (a), although I have shown an intermediate result that may actually be slightly more useful.

The math is helpful, but try to picture what's going on here, to help you decide which equations you should use. Draw a picture, if you haven't. All you're trying to do is find out how high you need to be to experience 10% of the gravitational force as you would on the surface.

Hope this helps.
 
Bill Foster said:
The acceleration of a mass at the surface is [tex]a_0[/tex]

The acceleration of a mass at some height x above the surface is [tex]a_1[/tex]

You want to know what x is when [tex]\frac{a_1}{a_0}[/tex]=0.1

The rest is simple algebra.
TonkaQD4 said:
That doesn't help me out.

Any other suggestions out there.

This certainly does help you out. [tex]\frac{a_1}{a_0}=.10[/tex]

but a_0= acceleration due to gravity or just [tex]g_{on earth}[/tex]

...so what is g in terms of G,M,m and R?

Hint: [tex]F_g=\frac{GMm}{r^2}[/tex] ... but what else is F_g equal to? Hint 2: Its a force!
Casey
 
Last edited:
Thanks. Figured it out.
 
WayneKao said:
The answer is 13838577.03 meters. hahahaha

This thread is over a year old; the joke would appear to be on you :smile:
 

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