Ch18 Gravitational fields Flashcards
What is newton’s law of gravitation
F=-GMm/r^2
- any 2 bodies attract each other with a force that is directly proportional to their product of mass and inversely proportional to the square distance between them
Speed of a satellite
- satellite orbiting the earth so
Fg=Fc
GMm/r^2 = mv^2/r
rearrange for V
Keplers first law
the orbit pf a planet is an ellipse with the sun at one of the 2 foci
Keplers second law
a line segment joining a planet and the sun sweeps equal area during equal time intervals
keplers third law
the square of the optica time period of is directly proportional to the cube of the optical distance
gravitational potential energy
the work done required to bring an object from infinity to a point in the gravitational field
E =-GMm/r
E = mgh
Escape velocity
KE converted to Eg
KE=Eg
1/2mv^2=GMm/r
rearrange for V