Escape velocity when in earth's orbit

In summary, the conversation discusses finding the period and velocity of an unpowered spacecraft using Kepler's 3rd law and the Vis Viva equation. The units of astronomical units (AU) are used for both the semi-major axis and distance from the sun, and the question arises about the units of velocity (V^2). The conversation also mentions the Earth's orbital speed and its mass being ignored for simplicity. A request is made to translate the units into miles per second.
  • #1
University
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I have a problem where it ask to find the period/time(using Kepler's 3rd law) of an unpowered spacecraft to move from Earth's orbit to Mars orbit using the transfer orbit approach.

I found P/T using kepler's 3rd law but the second part ask to find how fast the spacecraft need to be moving at the beginning of its trip i.e while in Earth's orbit using

V2= GM(2/r-1/a) where a is the semi-major axis of the orbit, r distance from the sun.

Now the units of a is in astronomical units and r can also be AU, what units would V^2 be if I use AU for both r and a in the Vis Viva equation above?
 
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  • #2
Is G also in units of AU?
 
  • #3
Is a velocity of 3.27 * 104 m/s seems correct for an escape velocity of a unpowered spacecraft that use the least energy transfer orbit to escape the Earth's orbit and head to Mar's orbit?
 
  • #4
If you set r & a equal to AU, and G & M equal to 1, the the units are Earth's average orbital speed, thus v^2=1. Actually slightly different to its real speed because we're ignoring Earth's mass, but that's a refinement for more advanced computations.
 
  • #5
Can someone please translate that into miles per second?
 
  • #6
try google
 
  • #7
Radrook said:
Can someone please translate that into miles per second?

Earth's orbital speed is 18.5 mi/s on average.
 

1. What is escape velocity when in Earth's orbit?

Escape velocity when in Earth's orbit is the minimum speed needed for an object to escape the gravitational pull of Earth and continue on a path into space. It is approximately 11.2 kilometers per second or 25,000 miles per hour.

2. How is escape velocity calculated?

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

3. Can objects in Earth's orbit reach escape velocity?

Yes, objects in Earth's orbit can reach escape velocity if they have enough energy. This is often achieved through the use of rockets or other propulsion systems.

4. What happens if an object in Earth's orbit does not reach escape velocity?

If an object in Earth's orbit does not reach escape velocity, it will continue to orbit the Earth in a circular or elliptical path. This is known as a stable orbit.

5. Is escape velocity the same for all planets?

No, escape velocity varies for different planets depending on their mass and size. For example, the escape velocity on the Moon is much lower than on Earth due to its smaller mass and weaker gravitational pull.

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