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V is proportional to…
1/sqr of r
Kepler’s 3rd law
T2 = (4(pi)²/GMsun) (r³)
T² is proportional to…
r³!
v =…
v = 2(pi)r/T
Potential energy becoming less negative means there’s an ___ in it.
increase
Angular momentum is conserved when no ___ is on a planet, which means they move ___ when closer to the sun.
torque, faster
Angular momentum conservation in space equation:
r1v1 = r2v2
In the Fg equation, r stands for…
Distance between the centers of masses
Increase in speed means…
orbital radius decreases