Orbital Velocity of Equatorial Satellite at 352,000 km

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To determine the orbital velocity of a satellite at 352,000 km above Earth, understanding equatorial orbit is essential, as it refers to a satellite orbiting directly above the equator. The discussion highlights the use of Kepler's third law to find the orbital period and subsequently the velocity. The correct approach involves calculating the radius from the Earth's center and applying the relationship between period and radius. Participants express confusion over the calculations, particularly regarding the application of Kepler's law and the necessary constants. Ultimately, the conversation emphasizes the importance of using the correct radius and gravitational equations to achieve accurate results.
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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 \propto 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<br /> \propto 358370000^3? I am getting a really low answer and according to my teacher it is wrong
 
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