Section 2.7: Applications of Satellites

Satellites are artificial objects placed in orbit around celestial bodies for various practical purposes. Their applications span communications, navigation, observation, and scientific research.

Communication Satellites:

Used for transmitting television, radio, internet, and phone signals globally. Often placed in geostationary orbit for constant coverage of a region.

Navigation Satellites:

GPS satellites enable precise location tracking and navigation for civilian and military use. Typically in medium Earth orbit (MEO).

Weather and Earth Observation Satellites:

Used to monitor climate, predict weather, track storms, and collect environmental data. Often placed in low Earth orbit (LEO) for higher resolution imaging.

Scientific Satellites:

Satellites for astronomy, astrophysics, and space exploration. Examples include Hubble Space Telescope and probes studying other planets.

Example 1

A communication satellite orbits Earth at 3.6×10^7 m (geostationary). Calculate the required orbital period to remain stationary relative to Earth's surface.

Orbital period for geostationary orbit: T = 24 hours = 86400 s (by definition of geostationary orbit).

Example 2

A GPS satellite orbits at 2×10^7 m. Find its approximate orbital speed assuming circular orbit.

v = √(GM/r) ≈ √(6.674×10^-11 * 5.972×10^24 / 2×10^7) ≈ 3.45×10^3 m/s

Practice Problems

  1. Calculate the orbital period of a LEO satellite at 500 km above Earth.
  2. Find the speed of a geostationary satellite at 3.6×10^7 m.
  3. Determine the altitude for a satellite to orbit Earth with period 12 hours.
  4. A weather satellite takes images of the equator every 90 minutes. Find its orbital radius.
  5. Compare velocities of LEO and MEO satellites.
  6. Compute the centripetal acceleration of a GPS satellite.
  7. Explain why communication satellites are placed in geostationary orbit.
  8. Estimate the orbital speed of a scientific satellite at 1×10^6 m above Earth.
  9. Calculate the orbital period of a satellite around Mars at radius 2×10^6 m.
  10. Explain advantages of satellites in sun-synchronous orbits for Earth observation.