Escape Velocity from Solar System

In summary, the escape velocity of an interstellar spacecraft from the solar system is calculated using the equation v = \sqrt{v_E^2 + (v_S - v_0)^2}, where v_E is the escape velocity from the Earth, v_S is the escape velocity from the gravitational field of the Sun at the orbit of the Earth, and v_0 is the Earth's orbital velocity about the Sun. The extra energy provided by v_0 at the beginning of the trip makes it easier to escape. The direction of the escape velocity vector from the Sun is perpendicular to both the Earth's escape velocity vector and the Earth's orbital velocity vector. These assumptions make it easier to calculate the escape velocity.
  • #1
e(ho0n3
1,357
0
Here is a celestial mechanics problem I can't seem to solve:To escape the solar system, an interstellar spacecraft must overcome the gravitational attraction of both the Earth and Sun. Ignore the effects of the other bodies in the solar system. Show that the escape velocity is

[tex]v = \sqrt{v_E^2 + (v_S - v_0)^2}[/tex]

where [itex]v_E[/itex] is the escape velocity from the Earth; [itex]v_S = \sqrt{2GM_S/r_{SE}}[/itex] is the escape velocity from the gravitational field of the Sun at the orbit of the Earth but far from the Earth's influence ([itex]M_S[/itex] is the mass of the Sun and [itex]r_{SE}[/itex] is the Sun-Earth distance); and [itex]v_0[/itex] is the Earth's orbital velocity about the Sun.

The thing I don't understand here is how the orbital velocity of the Earth plays a role. Suppose I took the Earth out of the picture and the spacecraft is orbitting the sun with orbital velocity equal to that of Earth's. Isn't the escape velocity from the sun just [itex]v_S[/itex]. What do I need [itex]v_0[/itex] for?
 
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  • #2
[itex]v_0[/itex] gives you some extra energy at the beginning of the trip, so naturally it'll take less to get away.

cookiemonster
 
  • #3
cookiemonster said:
[itex]v_0[/itex] gives you some extra energy at the beginning of the trip, so naturally it'll take less to get away.

cookiemonster
If you happen to escape in the same direction as the orbital velocity vector, then I guess it would help.

I think this all depends on where on Earth I am taking of from. Or does it make no difference? I'm still confused.
 
  • #4
From the equation for v, it seems that

[tex]\vec{v} = (v_E, v_S - v_0) = \vec{v}_E + \vec{v}_S - \vec{v}_0[/tex]

where [itex]\vec{v}_E = (v_E, 0)[/itex], [itex]\vec{v}_S = (0, v_S)[/itex], and [itex]\vec{v}_0 = (0, v_0)[/itex]. This is interesting since the escape velocity vector from the Sun has the same direction as the Earth's orbital vel. vector and both of these vectors are perpendicular to Earth's escape vel. vector. I guess when you make these assumptions, it is easy to show what the escape velocity is. I really don't know how one would come to these sorts of conclusions though.
 

1. What is escape velocity from the Solar System?

Escape velocity from the Solar System is the minimum speed that an object must reach in order to break free from the gravitational pull of the Sun and escape into space. It is a measure of the strength of the Sun's gravitational force.

2. How is escape velocity calculated?

The formula for escape velocity is Ve = √(2GM/R), where G is the gravitational constant, M is the mass of the Sun, and R is the distance from the center of the Sun to the object. This formula takes into account the mass and distance of the object in relation to the Sun's gravity.

3. What is the escape velocity from Earth's orbit around the Sun?

The escape velocity from Earth's orbit around the Sun is approximately 42.1 km/s or 25.9 mi/s. This means that any object traveling at this speed or higher will be able to break free from Earth's orbit and escape into space.

4. Can escape velocity vary in different parts of the Solar System?

Yes, escape velocity can vary in different parts of the Solar System. This is because the strength of the Sun's gravitational force decreases the further away an object is from the Sun. Therefore, an object would need a different velocity to escape the gravitational pull depending on its location in the Solar System.

5. What is the significance of escape velocity from the Solar System?

The escape velocity from the Solar System is significant because it determines whether an object can break free from the Sun's gravitational pull and travel into space. It is also an important factor in space exploration and understanding the dynamics of our Solar System.

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