Discover the Relationship Between Escape Speed and Circular Orbit Speed

Click For Summary
SUMMARY

The relationship between escape speed (Ve) and circular orbit speed (Vc) is defined by the equation Ve = √(2Vc). This relationship is derived from gravitational force equations, specifically GMem/r² = m(v²/r), which relates centripetal acceleration to gravitational force. The escape velocity can also be expressed as Ve = √(2GMe/Re) or Ve = √(2gRe), where Me is the mass of the planet and Re is its radius. Understanding this relationship is crucial for comprehending how objects escape a planet's gravitational pull.

PREREQUISITES
  • Understanding of gravitational force equations
  • Knowledge of centripetal acceleration concepts
  • Familiarity with potential energy formulas in gravitational fields
  • Basic knowledge of algebra and square root calculations
NEXT STEPS
  • Study gravitational force equations and their applications
  • Learn about centripetal acceleration and its relationship with orbital motion
  • Explore potential energy calculations for objects in gravitational fields
  • Investigate the implications of escape velocity in astrophysics
USEFUL FOR

Astronomy students, physicists, and anyone interested in orbital mechanics and gravitational physics will benefit from this discussion.

starbaj12
Messages
48
Reaction score
0
Show that the escape speed from a planet is related to the speed of a circulat orbit just above the surface of the planet by Ve = square root(2Vc), where Vc is the speed of an object in the circular orbit.

I'm looking at GMem(object)/r^2 = m(o)v^2/r

But I do not know if this equation will help or how to connect it together with anything else. Any help would be great.
 
Physics news on Phys.org
OK, here's some questions that may help us help you

Do you know the formula for the potential energy of an object a distance R away from a planet - and how this relates to the escape energy?

Do you know how to relate energy to velocity, to translate escape energy into escape velocity?
 
First of all, let's agree that the equation you've set up gives Vc, since it simply says that the force of gravity produces the necessary centripetal acceleration for circular motion at distance r.

Hence, what you are lacking, is an equation which yields the escape velocity Ve.
Unless you have that, you cannot compare Vc with Ve!

So, question:
How can you find an equation which can be said to yield Ve?
Post a few of your own thoughts on it, particularly what you think is MEANT with the concept "escape velocity"!
 
Are you talking about U(r) = -GMm/r
The bigger the radius the smaller the potential energy

Ve = square root ( 2GMe/Re) = square root(2gRe)

Is this what you are talking about?
 
escape velocity to me means the speed it takes to overcome gravity (air friction negligible) leaving orthogonal from the surface of the planet
 
starbaj12 said:
Are you talking about U(r) = -GMm/r
The bigger the radius the smaller the potential energy

Ve = square root ( 2GMe/Re) = square root(2gRe)

Is this what you are talking about?
This is correct!
Now compare Ve and Vc!
 
I got it!
Thank you arildno
 

Similar threads

Replies
4
Views
4K
  • · Replies 9 ·
Replies
9
Views
2K
  • · Replies 7 ·
Replies
7
Views
6K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 9 ·
Replies
9
Views
4K
  • · Replies 3 ·
Replies
3
Views
1K
  • · Replies 17 ·
Replies
17
Views
3K
  • · Replies 10 ·
Replies
10
Views
2K
  • · Replies 8 ·
Replies
8
Views
3K