Finding gravity on a star/planet

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To calculate the acceleration of gravity on the surface of a neutron star with a mass of 3.0x10^30 kg and a radius of 8000 m, the gravitational force equation F = G * m / (d^2) is used, where G is the gravitational constant (6.67x10^-11). The force felt by an object under gravity is proportional to the mass of the star and inversely proportional to the square of the distance from its center. The resulting force calculation yields a value of 3.1265625 x 10^12, which is reasonable for a neutron star despite initial concerns about its magnitude compared to Earth's gravity. It's crucial to ensure all units are consistent, and the calculations confirm that such extreme values are typical for neutron stars. Understanding the relationship between mass, distance, and gravitational force is essential for accurate calculations.
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Homework Statement



"The mass of a certain neutron star is 3.0x10^30kg (1.5 solar masses) and its radius is 8000 m (8km). What is the acceleration of gravity at the surface of this condensed burned-out star?"



I have no idea where to start
 
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Nothing!

So from that sight, I gather this:

F=Gx(m1m2/d^2) ...right?

So:
G=F/(m1m2/d^2)

meaning:
F/((3.0 x 10^30) x m2/8000^2) ... Whats m2 and F?
 
The m1m2 will get you the total attraction between both bodies. You only need one, so lose the m2 (just set it to 1).

You don't need to flip the equation around. You're solving for F. That's your answer.

G is the gravitational constant, which you are given on that page (6.67x10^-11).
 
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Ok, so...

F = (6.67x10^-11) x [ (3.0x10^30)/(8000^2) ]

so F = 3.1265625 x 10^12Isn't that a bit strong considering Earth is ^-11 and this star has only an 8km radius? Or am I looking too much into it?
 
But you should try to understand what you're doing with this equation, don't just plug the numbers in.

The force an object feels under gravity of a massive object is directly proportional to the mass of the massive object.
i.e.: F is proportional to m : as m gets bigger the force gets bigger

and inversely proportional to the square of its distance
i.e. F is proportional to 1/(d^2) : as d gets bigger the force get smaller - and quickly

Put those together and you've got F proportional to m / (d^2).

This is only proportional though, which means you have no units. The gravtitational constant allows you to convert it to units.
So:
F = G * m / (d^2)
 
I haven't checked the numbers but this is a neutron star, and you are on its surface. Millions or billions of g's is par for the course.

What you need to do is check every one of your numbers to make sure you've got the units right. Is everything in kg or metres, not grams or kilometres? That's a really easy mistake to make.
 
I'm sure its all in the correct units.
Thank you both for your help
=]
 
  • #10
Well, isn't Earth (6.67x10^-11)?
So this star being (3.12x10^12) seems a bit extreme
 
  • #11
gigglin_horse said:
Well, isn't Earth (6.67x10^-11)?
So this star being (3.12x10^12) seems a bit extreme
No. Earth is 9.8x10^0.

The 6.67x10^-11 is the universal gravitational constant.

Think of this:

Your car's engine revs are proportional to your car's speed (let's pretend) but to apply units to that you'd have to have a constant that says "X revs equals Y miles per hour". Say, maybe your constant is q=.05
i.e.: velocity = q * revs

revs = 1000

So, v = .05 * 1000
v = 50mph

the consant there is q
 
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