How Much Energy Is Needed to Move a 1kg Block Away from Earth?

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SUMMARY

The energy required to move a 1kg block from the Earth's surface to a point far away, where it comes to rest, is derived from gravitational potential energy equations. The relevant equations include U = -G(m1m2)/r and U = mgy, where G is the gravitational constant, m1 and m2 are the masses involved, and r is the distance from the center of the Earth. The final potential energy (Uf) and kinetic energy (Kf) at rest are both zero, leading to the conclusion that the work done (W) is equal to the initial potential energy (Ui). The gravitational acceleration (g) can be calculated using g = -G M/r², where M is the mass of the Earth and r is the radius from the Earth's center.

PREREQUISITES
  • Understanding of gravitational potential energy (U = -G(m1m2)/r)
  • Familiarity with kinetic energy concepts (K = 1/2mv²)
  • Knowledge of gravitational acceleration (g = -G M/r²)
  • Basic algebra and calculus for solving equations
NEXT STEPS
  • Study the derivation of gravitational potential energy equations
  • Learn about the gravitational constant (G) and its significance
  • Explore variations in gravitational acceleration across different locations on Earth
  • Investigate the relationship between mass, distance, and gravitational force
USEFUL FOR

Students studying physics, particularly those focusing on mechanics and gravitational forces, as well as educators looking for clear explanations of energy concepts in gravitational contexts.

MillerGenuine
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Homework Statement



A 1kg block rests on Earth's surface. How much energy is required to move the block very far from the earth, ending up at rest again?

Homework Equations



U = -G(m1m2)/r
Uf-Ui= -W (W= work internal)
U=mgy


The Attempt at a Solution



I know that my final potential energy will be zero, and because the object ends at rest i can say my final kinetic energy will also be zero. Not sure where to go from here, or what equation to use.
 
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You are on the right track... as you say, the final total energy will be zero.
Can you also say something about the initial energy?
 
So assuming i use the equation Kf + Uf = Ki + Ui the left side of the equation goes to zero. I am then only left with my initial conditions, and my Ki = 1/2mv^2 and U=mgy..? or does U= -G (Mm)/r ...?
 
MillerGenuine said:
So assuming i use the equation Kf + Uf = Ki + Ui the left side of the equation goes to zero. I am then only left with my initial conditions,
Exactly.

and my Ki = 1/2mv^2
Where v is the initial velocity (which is ... ?)

and U=mgy..? or does U= -G (Mm)/r ...?
Yes. The whole idea is that they are the same at or very close to the surface of the earth. You can easily show this yourself, if you equate the two,
- \frac{G M m}{r} = m g r
where r is the distance from the center of the earth, you can solve this for g:
g = - \frac{G M}{r^2}.
Just plug in the numbers for r at (or negligibly close to) the surface of the earth, at 6400 km from the center, and you will find a value very close to the usually quoted value of g = -9.81 m/s².
(This also explains the reason that g varies between different locations on earth: since the Earth is not a perfect sphere, its radius changes a bit from one point to another. It is a bit smaller at the poles, so g will be a bit larger there than at the equator).
 

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