What Determines the Escape Speed from Earth's Gravitational Pull?

In summary: Therefore, the final kinetic energy will always be positive and the particle will never escape the gravitational pull. This is a common mistake that can be avoided by properly understanding the concept of escape velocity. In summary, the escape velocity of a particle from the surface of a massive body is determined by the law of conservation of energy and the value of the first term in the equation \frac{1}{2}(mu^2) - \frac{GMm}{R} must always be greater than or equal to the second term \frac{GMm}{R}. A negative value for the first term indicates that the particle's initial velocity is too low to escape the gravitational pull and the final kinetic energy will always be positive.
  • #1
hadronthunder
3
0
Hi friends.

Somewhere in a reference book I read about escape speed of a particle for earth.
Let a particle is projected from the Earth surface. Let its mass be m and speed of projection be u. Let mass of Earth be M and its radius be R.

According to law of conservation of energy,
https://fbcdn-sphotos-a-a.akamaihd.net/hphotos-ak-prn2/q86/s720x720/1175485_1407193806174392_209657781_n.jpg
https://fbcdn-sphotos-g-a.akamaihd.net/hphotos-ak-prn2/q88/s720x720/1236159_1407193812841058_1152852378_n.jpg
The problem is that,

If the Ist term becomes negative also but its magnitude is less than the IInd term, then also final Kinetic energy will be positive. And the particle will never doesn't give the proper answer. Friend isn't it so?
Please help me in understanding this.
Thank you all in advance.
 
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  • #2
The first term in what? You mean term I in the first relation?
That's kinetic energy - does it make physical sense to have a negative kinetic energy?
 
  • #3
Simon Bridge said:
The first term in what? You mean term I in the first relation?
That's kinetic energy - does it make physical sense to have a negative kinetic energy?

The first term is in the second relation. the complete 1/2(mu2) - (GMm)R

The complete term can be negative due to less value of 1/2 (mu2).
 
  • #4
For escape velocity you're comparing the total energy at the surface of a massive body and at infinity from it.

This means that the second term [itex]\frac{GMm}{R+h}[/itex] will always be zero. So the first term can not be less in magnitude than the second one.If the first term becomes negative due to too low a value of initial velocity U, it simply means that the velocity U is too low to escape the gravity of the massive body.
 
  • #5


Hi there,

The concept of escape speed is an important one in the study of celestial bodies such as planets and moons. It refers to the minimum speed at which a particle must be launched from the surface of a planet in order to escape its gravitational pull and not fall back to the surface.

In the equations you have provided, the first term represents the potential energy of the particle at the Earth's surface, while the second term represents its kinetic energy. In order for the particle to escape, its final kinetic energy must be greater than or equal to its initial potential energy. This is because as the particle moves away from the Earth, its potential energy decreases while its kinetic energy increases.

If the first term becomes negative, it means that the potential energy of the particle at the Earth's surface is less than zero, which is not physically possible. This can happen if the particle is launched with a speed greater than the escape speed, causing it to have a negative potential energy.

In order to properly calculate the escape speed, you must use the correct values for the mass and radius of the Earth, and the mass of the particle. You can also use the equation v = √(2GM/R) where G is the gravitational constant, M is the mass of the Earth, and R is the radius of the Earth.

I hope this helps clarify the concept of escape speed for you. If you have any further questions, please don't hesitate to ask. Happy studying!
 

1. What is escape speed?

Escape speed is the minimum speed required for an object to overcome the gravitational pull of a massive body, such as a planet or a star, and escape its orbit.

2. How is escape speed calculated?

Escape speed is calculated using the formula v = √(2GM/r), where v is the escape speed, G is the gravitational constant, M is the mass of the massive body, and r is the distance from the center of the body to the object.

3. Why is escape speed important?

Escape speed is important because it determines whether or not an object can leave the gravitational influence of a massive body. It is crucial for space exploration and understanding the dynamics of celestial bodies.

4. Can escape speed be exceeded?

Yes, escape speed can be exceeded. In this case, the object will have enough kinetic energy to escape the gravitational pull of the massive body and travel into space.

5. Does escape speed vary for different planets?

Yes, escape speed varies for different planets depending on their mass and size. The larger and more massive the planet, the higher the escape speed required to leave its orbit.

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