Calculating the period of a low Earth satelite using Kepler

AI Thread Summary
The discussion focuses on calculating the period of a low Earth orbiting satellite using Kepler's laws, specifically addressing an incorrect value for the constant T^2/R^3 for Earth. The initial calculation yielded a period of 8.72 seconds, which contradicts the known period of approximately 90 minutes. Participants clarify that the constant used was likely intended for solar orbits rather than Earth orbits, suggesting a need for a different value. The correct constant can be derived from the mass of the Earth, and the confusion stems from the provided homework materials. Ultimately, the importance of using the correct constant for accurate satellite period calculations is emphasized.
barryj
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Homework Statement


Find the period of a low Earth orbiting satellite using Kepler Laws
earth radius = 6.38E6 meters
T^2/R^3 for Earth = 2.97E-19 (sec^2/m^3)

Homework Equations



2.97E-19 = T^2/(6.38E6)^3
T^2 = (2.97E-19)(6.38^6)^3 = 77.1
T = 8.72 sec

The Attempt at a Solution


This is not correct since I know the period of a low earther is about 90 minutes or about 5600 seconds.
?
 
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barryj said:
T^2/R^3 for Earth = 2.97E-19 (sec^2/m^3)
Hello. The number on the right doesn't look correct. How did you get that value?
 
The number came from a chart that was supplied with a homework set for physics.
I realize that there are other variants of this number with different units such as
3.35 10E24km^3/yr^2) this shyulkd be the same value if the units are converted.
Maybe there is an error in one of he documents.
 
The value given in your table is incorrect. You can calculate the correct value yourself in terms of the mass of the earth.

See http://pvhslabphysics.weebly.com/keplers-3rd-law.html

Here ##a## is the radius of the orbit if the orbit is circular. If the orbit is elliptical, then ##a## is the length of the semi-major axis of the ellipse.
 
The value of the constant that you used appears to be for orbits around the sun rather than around the earth.
 
barryj said:
T^2/R^3 for Earth = 2.97E-19 (sec^2/m^3)

Your constant is wrong
 
I get it now. Yes, I need a different constant for around earth. I was confused but better now. thanks
 
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