Problem involving Newton's Law of Gravitation

AI Thread Summary
The discussion revolves around calculating the acceleration due to gravity on a planet with half the mass and double the radius of Earth. The key equations used are Newton's law of gravitation and the formula for gravitational force. By equating the gravitational force equations and substituting the planet's mass and radius in terms of Earth's, it simplifies to g_planet = (1/8) g_earth. The final conclusion is that the acceleration due to gravity on the planet is g/8, confirming the solution without unnecessary calculations. This approach effectively demonstrates the application of gravitational principles.
collide
Messages
6
Reaction score
0
1. A planet has a mass 1/2 that of Earth and a radius 2 times that of Earth. What is the acceleration due to gravity on the surface of the planet in terms of g?



2.
a)F=G*m1*m2/r^{2}
b)F=mg



3. I figured that I would let the two equations equal to each other so...

G*m1*m2/r^{2}=mg
It simplifies to be g=G*m/r^{2}
However, I don't know where to go from there to get the acceleration in terms of g.

Any suggestions would be greatly appreciated. Thanks
 
Physics news on Phys.org
You're on the right track. Maybe rewriting it this way will give you a hint:
g_{earth} = G M_{earth}/R_{earth}^2

(Express M and R for the planet in terms of M and R for the earth.)
 
Doc Al said:
You're on the right track. Maybe rewriting it this way will give you a hint:
g_{earth} = G M_{earth}/R_{earth}^2

(Express M and R for the planet in terms of M and R for the earth.)

So then you would get this correct:

g_{earth} = G (1/2)M_{earth}/(2*R_{earth})^2

Which you can then simplify to be:

g_{earth} = G M_{earth}/8R_{earth}

However, I don't know where to go from there to find the acceleration:confused:
 
collide said:
So then you would get this correct:

g_{earth} = G (1/2)M_{earth}/(2*R_{earth})^2
Almost. You'd get:

g_{planet} = G M_{planet}/R_{planet}^2

g_{planet} = G (1/2)M_{earth}/(2*R_{earth})^2

Which simplifies to:

g_{planet} = (1/8) G M_{earth}/R_{earth}^2

I'll leave it to you to interpret the right hand side in terms of g for earth.
 
Should I plug in the values for M_earth, R_earth, and G to find out what g_planet equals?

And then I do g_planet=(g/x) to solve for x to find out in terms of what value for g is right? Doing this method... I get accelerated is g/8. However, is the proper way to solve this problem or am I doing more work than required?
 
collide said:
Should I plug in the values for M_earth, R_earth, and G to find out what g_planet equals?

And then I do g_planet=(g/x) to solve for x to find out in terms of what value for g is right? Doing this method... I get accelerated is g/8. However, is the proper way to solve this problem or am I doing more work than required?
That's definitely the hard way. We already determined that the acceleration due to gravity on the planet equals:

g_{planet} = (1/8) G M_{earth}/R_{earth}^2

But you should recognize the equation we stated with:

g_{earth} = G M_{earth}/R_{earth}^2

Substituting this last equation into the first gives:

g_{planet} = (1/8) g_{earth} = g/8

That's all you need to do--no calculations needed.
 
Thanks for the help, Doc Al!
 
Back
Top