Escape Velocity and planet’s gravitational field

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The discussion focuses on calculating the escape velocity for an object on Pluto's surface, emphasizing that the kinetic energy required to escape equals the gravitational potential energy at that point. The formula derived is v = √(2GM/R), leading to an escape velocity of approximately 1205 m/s. Participants confirm that overcoming the potential energy at the surface is essential for escape. Additionally, advice is given to consider the negative sign in gravitational potential energy when approaching such problems in tests. The conversation highlights the importance of understanding energy conservation in gravitational fields.
RoryP
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Homework Statement


The escape velocity is the velocity of an object at the surface of a planet that would
allow it to be removed completely from the planet’s gravitational field.
Calculate the escape velocity for an object on the surface of Pluto.

mass of Pluto: 1.3 *1022
radius of Pluto: 1.2 *106
G= 6.7 *10-11

Homework Equations


EK= 1/2mv2
Potential Energy= GM1M2/R


The Attempt at a Solution


I think i have this correct but i don't have the answers to check! So i need a professional opinion =]
So at the surface would i be right in saying the kinetic energy required to leave the planet will be equal to the Potential the body has at the surface of the planet??
So, 1/2mv2= GM1M2/R
(the mass of the object will cancel)
v=[square root]{2GM/R}
v=[square root]{2*6.7 *10-11*1.3 *1022/1.2 *106
v= 1205 ms-1
Is this the right answer?? not entirely sure!
 
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RoryP said:

Homework Statement


The escape velocity is the velocity of an object at the surface of a planet that would
allow it to be removed completely from the planet’s gravitational field.
Calculate the escape velocity for an object on the surface of Pluto.

mass of Pluto: 1.3 *1022
radius of Pluto: 1.2 *106
G= 6.7 *10-11

Homework Equations


EK= 1/2mv2
Potential Energy= GM1M2/R


The Attempt at a Solution


I think i have this correct but i don't have the answers to check! So i need a professional opinion =]
So at the surface would i be right in saying the kinetic energy required to leave the planet will be equal to the Potential the body has at the surface of the planet??
So, 1/2mv2= GM1M2/R
(the mass of the object will cancel)
v=[square root]{2GM/R}
v=[square root]{2*6.7 *10-11*1.3 *1022/1.2 *106
v= 1205 ms-1
Is this the right answer?? not entirely sure!

Yes. You need to overcome the potential at the surface. 1/2mV2 = Gmp/rp

Where rp and mp are the radius and mass of the dwarf planet Pluto
 
ahhh sweet cheers! =]
 
Hi ,
I suggest in question like this in a test:
Don't write right away GMm/R=Mv^2/2
say that Potential energy = -GMm/R notice the negative sign.
and in infinity the energy==0
than Initial kinetic energy + (which will get us minus here) potential energy=0(getting to infinity).

Just An advice from some 1 that suffered this thing on his flesh :D
 
The book claims the answer is that all the magnitudes are the same because "the gravitational force on the penguin is the same". I'm having trouble understanding this. I thought the buoyant force was equal to the weight of the fluid displaced. Weight depends on mass which depends on density. Therefore, due to the differing densities the buoyant force will be different in each case? Is this incorrect?

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