Escape velocity when in earth's orbit

AI Thread Summary
The discussion focuses on calculating the period of an unpowered spacecraft moving from Earth's orbit to Mars orbit using Kepler's 3rd law and determining the necessary initial velocity in Earth's orbit. The user applies the Vis Viva equation, questioning the units for velocity when using astronomical units (AU) for both the semi-major axis and distance from the sun. They confirm that if G and M are set to 1, the resulting velocity squared corresponds to Earth's average orbital speed, with a noted difference due to ignoring Earth's mass. The average orbital speed of Earth is mentioned as 18.5 miles per second, providing a reference for the calculated escape velocity.
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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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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?
 
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.
 
Can someone please translate that into miles per second?
 
try google
 
Radrook said:
Can someone please translate that into miles per second?

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