Slide 20
For a satellite to be in a particular orbit, a particular velocity is required or a given height above Earth ‘r0+h’.
Telecommunications satellites remain above one given point on the Earth’s surface, so are called geostationary.
Spy Satellites move in a polar orbit so that they can perform sweeps of the surface.
Slide 21
Formulae for calculating satellite orbits
ω = 2πf;
v = ωr;
a = ω2r
a=v2/r → v2=ar
v=2πr/T
g=GM/r2
V=-GM/r
Slide 22
References:
Giancoli , Physics: Principles with Applications, 6th edition
http://kilby.sac.on.ca/physics/sph4u/3-Fields/GravEnergy.htm
http://www.antonine-education.co.uk/Pages/Physics_4/Fields/FLD_02/Fields_page_2.htm
http://www.physicsclassroom.com/class/circles/u6l3c.cfm
http://hyperphysics.phy-astr.gsu.edu/hbase/gpot.html
http://blog.superprincipia.com/2012/01/16/a-theory-of-gravity-for-the-21st-century-the-gravitational-force-and-potential-energy-in-consideration-with-special-relativity-general-relativity/