Calculating the period of a low Earth satelite using Kepler

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Homework Help Overview

The discussion revolves around calculating the period of a low Earth orbiting satellite using Kepler's Laws, specifically focusing on the relationship defined by T^2/R^3. The original poster presents a calculation that yields a period significantly shorter than expected for such satellites.

Discussion Character

  • Exploratory, Assumption checking, Conceptual clarification

Approaches and Questions Raised

  • Participants question the validity of the constant used in the calculations, with some suggesting that it may pertain to orbits around the sun rather than Earth. Others express confusion regarding the units and values provided in the homework materials.

Discussion Status

There is an ongoing exploration of the correct constant to use for calculations related to Earth orbits. Some participants have acknowledged their misunderstandings and are seeking clarification on the appropriate values and units.

Contextual Notes

Participants note discrepancies in the provided constants and suggest that there may be errors in the homework documents. The original poster's calculation contrasts sharply with known values for satellite periods, indicating a potential misunderstanding of the constants involved.

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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