Escape Velocity and planet’s gravitational field

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SUMMARY

The escape velocity for an object on the surface of Pluto is calculated using the formula v = √(2GM/R), where G is the gravitational constant (6.7 × 10-11 m3kg-1s-2), M is the mass of Pluto (1.3 × 1022 kg), and R is the radius of Pluto (1.2 × 106 m). The calculated escape velocity is approximately 1205 m/s. It is essential to equate the kinetic energy required to escape the gravitational field with the potential energy at the surface of the planet, confirming that the mass of the object cancels out in the equation.

PREREQUISITES
  • Understanding of gravitational potential energy and kinetic energy equations
  • Familiarity with the gravitational constant (G)
  • Basic algebra and square root calculations
  • Knowledge of planetary mass and radius measurements
NEXT STEPS
  • Study the derivation of escape velocity formulas in astrophysics
  • Learn about gravitational potential energy and its implications in celestial mechanics
  • Explore the concept of energy conservation in gravitational fields
  • Investigate escape velocities for other celestial bodies, such as Earth and Mars
USEFUL FOR

Astronomy students, physics enthusiasts, and anyone interested in understanding gravitational forces and escape velocities of celestial bodies.

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
 

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