Exploring Earth's Escape Velocity: A Non-Physics Perspective

In summary, the rocket does not need to reach escape velocity right from the start because there is a force acting on it due to the engines. The escape velocity is the velocity an object needs to escape the gravitational field if there are no forces other than gravity acting on it. However, a rocket has a constant force from the engines acting against gravity, so it doesn't need to reach escape velocity.
  • #1
Gilad Barnea
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Hi,

First FYI, I have no education in physics.
Anyway -

I know Earth's escape velocity is about 41,000 kph. Anything less, and you'll eventually fall down back to earth.

Two points that seem to contradict each other -
1. Escape velocity gets decreased the farther away you are from the center of mass.
2. I'm pretty sure most rockets I've seen don't accelerate to 41,000 kph right off the bat. They take some time to reach full speed.

So - If you managed to launch the rocket from the ground, that's the hardest part by definition. Getting it from an altitude of 100m to 200m requires less force than from 0m to 100m. Yet the rocket doesn't reach 41,000 kph before the 100m mark. And it could be even slower the higher up it goes. So it seems you start off slow (not 41,000 kph) and get even slower until you're out of Earth gravity well.

Where does the 41,000 kph thing come into play?Thanks!
 
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  • #2
The rocket does not need to reach escape velocity right from the start because there is a force acting on it due to the engines. The escape velocity is the velocity an object needs to escape the gravitational field if there are no forces other than gravity acting on it.
 
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  • #3
To elaborate a little, if I shoot an object out of a cannon, it needs to be traveling at escape velocity by the time it leaves the cannon or it will fall back to Earth. This is because, as Orodruin said, there is no other force acting on the projectile other than gravity (we're ignoring air friction here).

However, a rocket has a constant force from the engines acting against gravity, so it doesn't need to reach escape velocity.
 
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  • #4
Thanks! Got it.
 
  • #5
Most rockets don't even need to reach escape velocity. They just put objects in orbits around Earth. If the satellites "escape" then it's pretty bad.:)
 
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FAQ: Exploring Earth's Escape Velocity: A Non-Physics Perspective

1. What is escape velocity and why is it important?

Escape velocity is the speed that an object needs to reach in order to break free from the gravitational pull of a celestial body, such as Earth. It is important because it determines whether an object, like a spacecraft, can leave a planet's orbit and travel into space.

2. How is escape velocity calculated?

Escape velocity is calculated using the formula Ve = √[(2GM)/r], where G is the gravitational constant, M is the mass of the celestial body, and r is the distance from the center of the body to the object. This formula applies to any celestial body, not just Earth.

3. Can humans reach escape velocity?

Yes, humans have reached escape velocity using rockets and spacecraft. The Saturn V rocket that launched Apollo 11, the first mission to land humans on the moon, had a maximum speed of about 11.2 km/s, which is well above Earth's escape velocity of 11.2 km/s.

4. How does escape velocity differ on other planets?

Escape velocity varies among different celestial bodies due to their varying masses and sizes. For example, Mars has a smaller mass and size than Earth, so its escape velocity is lower at 5 km/s. On the other hand, the gas giant Jupiter has a much larger mass, resulting in a higher escape velocity of 59.5 km/s.

5. What are some real-world applications of understanding escape velocity?

Understanding escape velocity is crucial for space exploration and satellite launches. Engineers and scientists use this knowledge to design and launch spacecraft that can reach and explore other planets, moons, and even interstellar space. Additionally, understanding escape velocity is important for calculating orbital trajectories and ensuring the safe return of spacecraft to Earth.

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