Orbital velocity is what the Space Shuttle needs to reach to get to orbit. |
The formula for orbital velocity is as follows:
Vo ≈ sqrt[ GM / r ]
where
Vo = Orbital velocity (m/s)
G = Gravitational constant
M = Mass of planet (kg)
r = Distance from planet's center of gravity the rocket is launching at (m)
We can easily write a Python function to solve for this. In fact, it's almost identical to the one we wrote for calculating escape velocity:
from decimal import * _GRAVITATIONAL_CONSTANT = Decimal('6.67384E-11') def orbital_velocity(mass, radius): '''Calculates the delta-V orbital velocity. Returns delta-V in meters per second for the orbital velocity for a given object given its mass in kilograms and its radius in meters.''' if mass == Decimal('0') or radius == Decimal('0'): # User gave a mass or radius which is unrealistic, # abort. return None result = Decimal((_GRAVITATIONAL_CONSTANT * mass) / radius) result = result.sqrt() return result
Let's run this using our figures for Earth (mean radius of 6,371 km, mass of 5.9736E24 kg), assuming the above code is in sci.py:
>>> from decimal import * >>> import sci >>> sci.orbital_velocity(Decimal('5.9736E24'), Decimal('6371000')) Decimal('7910.467706232366495042659538')
So, 7.9 km/s is approximately the orbital velocity according to our function. And, if we check the Wikipedia article for orbital velocity, it mentions that for low Earth orbit, the orbital velocity ranges from 6.9 km/s to 7.8 km/s! That's what I call close enough for government work.
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