Calculating Period of Hubble Telescope Orbit

AI Thread Summary
The Hubble Space Telescope orbits Earth at an altitude of 615 km, requiring the total orbital radius to be calculated as the Earth's radius plus this altitude, approximately 7000 km. The initial attempt to calculate the period mistakenly used the acceleration due to gravity at Earth's surface, which is not appropriate for orbital calculations. Kepler's third law is discussed as a method to determine the orbital period, with the correct formula involving the mass of Earth and gravitational constant. After clarifications, the period of the Hubble's orbit is determined to be approximately 1.61 hours or 96.85 minutes, aligning with typical low Earth orbit durations. The final consensus suggests using the radius of Earth for simplified calculations, resulting in a period of about 84.43 minutes.
cstout
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Homework Statement


The Hubble Space Telescope orbits Earth 615 km above Earth's surface. What is the period of the telescope's orbit?


Homework Equations


T = 2(pi)r/v


The Attempt at a Solution



T = 2(pi)(6.37x10^6)/9.8
 
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Remember the radius of the orbit is measured from the centre of the earth.
 
Isn't 6.37 × 106 m the radius of the earth, or do I use another measurement.
 
cstout said:
Isn't 6.37 × 106 m the radius of the earth, or do I use another measurement.

So, the radius of the orbit is radius of earth? That means the satellite is orbiting in surface, right?
 
it orbit 615km above the Earths surface
 
The orbital radius is the distance from the centre of the Earth to the satelite.
Hence the radius of the Earth PLUS the altitude = approx 7000km.
 
Remember to express total distance (Earth's radium + orbital distance) in meters to mantain a coherence among unities.
 
And since you aren't given the speed you also need Kepler's 3rd law to work out the period. Not sure where you got the 9.8 from in your original equation - but it's wrong!
 
how would you use Kepler's 3rd law in relation to this question though, you aren't given some of the information needed.
 
  • #10
Nope - you have everything you need. What information do you think you need for Kepler's 3rd Law that you aren't given?

And by the way, mgb_phys - I'll be cstout was using the value for the approximate acceleration due to gravity at the Earth's surface, i.e. 9.8 m/s^2, which you'd just have to call a pretty bad guess.
 
  • #11
Remember the simplified form of the law doesn't need the mass of the orbital body
, you can assume that G(M+m) is pretty much equal to GM. Hubble only weighs about 10tons!
 
  • #12
Ok, I finally got it, the answer is 1.61 hrs. Thanks for the help
 
  • #13
That sounds about right, 90 minutes is pretty typical for LEO
 
  • #14
Try using this formula: 4(pi)² r³/(M+m)G = P²

Where:
r = radius between the centers of mass of both bodies measured in meters
M = the larger mass in kilograms (5.9742 X 10^24 for the earth)
m = the smaller mass in kilograms (this mass is usually so much smaller than the
larger mass that it can almost always be disregarded)
G = 6.67259 X 10-¹¹
P = the period of orbit in seconds

This formula yields an answer of approx. 5,811 seconds, which is about 96.85 minutes.
 
Last edited:
  • #15
I don't think so..

Since the radius,r of the telescope is just about 10% of the radius of the Earth.
Then it can be ignored..

Just use R for the radius of Earth.

Hence, Period of revolution of telescope
= 2Pi Square root R/g

=84.43min
 
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