Calculating the period of a low Earth satelite using Kepler

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SUMMARY

The discussion focuses on calculating the orbital period of a low Earth satellite using Kepler's Laws, specifically the formula T^2/R^3. The provided constant for Earth, 2.97E-19 (sec^2/m^3), was identified as incorrect for this context. The correct orbital period for a low Earth satellite is approximately 90 minutes, or 5600 seconds. The conversation emphasizes the importance of using the appropriate constant for Earth rather than one intended for solar orbits.

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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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