Comparing Escape Energies of Earth, Moon, and Jupiter

In summary, the energy needed to escape from the Moon is 0.0451 times the energy needed to escape from Earth, while the energy needed to escape from Jupiter is 28.5 times the energy needed to escape from Earth. This can be calculated using the formula 1/2mv^2 - GMm/r = 0, where v is the escape velocity and r is the distance between the planet's surface and infinity.
  • #1
popo902
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Homework Statement


What multiple of the energy needed to escape from Earth gives the energy needed to escape from (a) the Moon and (b) Jupiter? Use the Table (link below) if necessary

http://edugen.wiley.com/edugen/courses/crs1650/art/qb/qu/c13/fig13-19.gif


Homework Equations



1/2mv^2 - GMm/r = 0 (energy)
v = sqrt(2GM/R)

The Attempt at a Solution



for the potential energy, do i put in the radius of the planet instead of the distance between it and something? because there's nothing else there...

at first i figured that the potential will be zero anyway because once you escape, r would be infinity and make the potential 0
then i fiugured that only v mattered in comparing the amount of energy because the mas of the projectial would be the same, the only difference would be escape speed.
but i got it wrong

these are supposedly the rigth answers
a)0.0451
b) 28.5

im very confused...
 
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  • #2
hi popo902! :smile:

the energy needed to escape is defined as the energy needed to reach infinite distance at zero speed (ie at KE = 0) …

(of course, it's 1/2 mv2, where v is escape velocity )

since KE + PE = constant, that means that the escape KE is the difference in PE between the planet's surface and infinity. :wink:
 

Related to Comparing Escape Energies of Earth, Moon, and Jupiter

1. What is escape energy and why is it important to compare between Earth, Moon, and Jupiter?

Escape energy is the minimum amount of energy required for an object to escape the gravitational pull of a celestial body. Comparing escape energies between Earth, Moon, and Jupiter allows us to understand the differences in the strength of their gravitational fields and how this affects the ability of objects to escape their surfaces.

2. How is escape energy calculated for each celestial body?

Escape energy is calculated using the formula E = GMm/r, where G is the gravitational constant, M and m are the masses of the two objects, and r is the distance between them. For Earth, M is the mass of the Earth and r is the radius of the Earth. For the Moon, M is the mass of the Moon and r is the distance from the Moon's surface to its center. For Jupiter, M is the mass of Jupiter and r is the distance from Jupiter's surface to its center.

3. What are the factors that affect the escape energies of Earth, Moon, and Jupiter?

The main factors that affect escape energies are the mass and radius of the celestial body. Generally, the larger and more massive the body, the greater the escape energy will be. In addition, the distance between the object and the surface of the celestial body also plays a role in determining the escape energy.

4. How do the escape energies of Earth, Moon, and Jupiter compare?

The escape energy of Earth is the highest among the three, followed by Jupiter and then the Moon. This is due to the larger mass and radius of Earth and Jupiter compared to the Moon. Earth's escape energy is about 11.2 km/s, while Jupiter's is about 59.5 km/s and the Moon's is about 2.4 km/s.

5. What are the practical applications of comparing escape energies between celestial bodies?

Comparing escape energies can help us understand the conditions on different celestial bodies and how they affect the movement of objects. This information is important for space exploration and planning missions to different planets and moons. It can also provide insights into the formation and evolution of our solar system.

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