Calculating Period of Hubble Telescope Orbit

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SUMMARY

The Hubble Space Telescope orbits Earth at an altitude of 615 km, resulting in an orbital radius of approximately 7000 km when combined with Earth's radius. The period of the telescope's orbit can be calculated using Kepler's Third Law, specifically the formula P² = (4π²r³)/(GM), where G is the gravitational constant (6.67259 x 10^-11) and M is Earth's mass (5.9742 x 10^24 kg). The calculated period is approximately 84.43 minutes, aligning with typical low Earth orbit (LEO) durations.

PREREQUISITES
  • Understanding of Kepler's Third Law of planetary motion
  • Familiarity with gravitational constant (G) and Earth's mass
  • Basic knowledge of orbital mechanics
  • Ability to perform unit conversions and calculations in physics
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  • Learn about gravitational forces and their impact on satellite orbits
  • Study the calculations involved in determining orbital periods for various altitudes
  • Explore the physics of low Earth orbit (LEO) satellites and their operational parameters
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Astronomy students, aerospace engineers, and anyone interested in satellite dynamics and orbital mechanics will benefit from this discussion.

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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