Orbital Velocity of Equatorial Satellite at 352,000 km

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Homework Help Overview

The problem involves determining the orbital velocity of a satellite in equatorial orbit at an altitude of 352,000 km above Earth. The context is rooted in orbital mechanics and gravitational principles.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss the definition of an equatorial orbit and its implications for orbital calculations. There is an exploration of Kepler's laws and how they relate to the satellite's period and radius. Questions arise regarding the correct interpretation of the variables in the equations and the relationship between altitude and orbital radius.

Discussion Status

Some participants have provided guidance on using Kepler's third law to relate the period and radius of the orbit. Others are attempting to apply the law but are encountering difficulties with their calculations and interpretations. Multiple approaches are being explored without a clear consensus on the correct method.

Contextual Notes

There is uncertainty regarding the definitions and relationships between the variables involved, particularly the distinction between altitude and orbital radius. Participants are also navigating the constraints of homework expectations and the need for precision in their calculations.

cortozld
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Homework Statement


An Earth's satelite is in equatorial orbit at 352,000 km above earth. What is the orbital velocity (m/s) of the satelite (4 sig figs)


Homework Equations


g1d1^2=g2d2^2 to find gravity at the height of the satellite


The Attempt at a Solution


I don't really know what an equatorial orbit is, i tried solving it as if it was a circular orbit but that didn't work. My guess was that equatorial means it goes around Earth once per year, but no idea...
 
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Equatorial orbit just means one above the equator.
The equation you are looking for is Kepler's third law - it will give you the period of the orbit.
Then from the distance you can work out the circumference and so the speed.


hint - you are given an altitude but the orbit depends on the radius, from the centre of the earth
 
so kepler's 3rd law is T1^2=R1^3
T2^2 R2^3

so T2 is the period, R1 is radius of earth, and R2 is radius of my orbit? what is T1 then?
 
Kepler's law is T^2 [tex]\propto[/tex] r^3

You should be able to find an equation in your textbook or on wikipedia involving G and the Earth's mass
 
so my equation will be T^2[tex] \propto[/tex] 358370000^3? I am getting a really low answer and according to my teacher it is wrong
 

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