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Solution

From [link] , the total energy of the Soyuz in the same orbit as the ISS is

E orbit = K orbit + U orbit = G m M E 2 r = ( 6.67 × 10 −11 N · m 2 /kg 2 ) ( 9000 kg ) ( 5.96 × 10 24 kg ) 2 ( 6.36 × 10 6 + 4.00 × 10 5 m ) = −2.65 × 10 11 J .

The total energy at Earth’s surface is

E surface = K surface + U surface = 0 G m M E r = ( 6.67 × 10 −11 N · m 2 /kg 2 ) ( 9000 kg ) ( 5.96 × 10 24 kg ) ( 6.36 × 10 6 m ) = −5.63 × 10 11 J .

The change in energy is Δ E = E orbit E surface = 2.98 × 10 11 J . To get the kinetic energy, we subtract the change in potential energy from [link] , Δ U = 3.32 × 10 10 J . That gives us K orbit = 2.98 × 10 11 3.32 × 10 10 = 2.65 × 10 11 J . As stated earlier, the kinetic energy of a circular orbit is always one-half the magnitude of the potential energy, and the same as the magnitude of the total energy. Our result confirms this.

The second approach is to use [link] to find the orbital speed of the Soyuz , which we did for the ISS in [link] .

v orbit = G M E r = ( 6.67 × 10 −11 N · m 2 /kg 2 ) ( 5.96 × 10 24 kg ) ( 6.36 × 10 6 + 4.00 × 10 5 m ) = 7.67 × 10 3 m/s.

So the kinetic energy of the Soyuz in orbit is

K orbit = 1 2 m v orbit 2 = 1 2 ( 9000 kg ) ( 7.67 × 10 3 m/s ) 2 = 2.65 × 10 11 J,

the same as in the previous method. The total energy is just

E orbit = K orbit + Δ U = 2.65 × 10 11 + 3.32 × 10 10 = 2.95 × 10 11 J.

Significance

The kinetic energy of the Soyuz is nearly eight times the change in its potential energy, or 90% of the total energy needed for the rendezvous with the ISS. And it is important to remember that this energy represents only the energy that must be given to the Soyuz . With our present rocket technology, the mass of the propulsion system (the rocket fuel, its container and combustion system) far exceeds that of the payload, and a tremendous amount of kinetic energy must be given to that mass. So the actual cost in energy is many times that of the change in energy of the payload itself.

Summary

  • Orbital velocities are determined by the mass of the body being orbited and the distance from the center of that body, and not by the mass of a much smaller orbiting object.
  • The period of the orbit is likewise independent of the orbiting object’s mass.
  • Bodies of comparable masses orbit about their common center of mass and their velocities and periods should be determined from Newton’s second law and law of gravitation.

Conceptual questions

One student argues that a satellite in orbit is in free fall because the satellite keeps falling toward Earth. Another says a satellite in orbit is not in free fall because the acceleration due to gravity is not 9.80 m/s 2 . With whom do you agree with and why?

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Many satellites are placed in geosynchronous orbits. What is special about these orbits? For a global communication network, how many of these satellites would be needed?

The period of the orbit must be 24 hours. But in addition, the satellite must be located in an equatorial orbit and orbiting in the same direction as Earth’s rotation. All three criteria must be met for the satellite to remain in one position relative to Earth’s surface. At least three satellites are needed, as two on opposite sides of Earth cannot communicate with each other. (This is not technically true, as a wavelength could be chosen that provides sufficient diffraction. But it would be totally impractical.)

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Source:  OpenStax, University physics volume 1. OpenStax CNX. Sep 19, 2016 Download for free at http://cnx.org/content/col12031/1.5
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