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Gravity
the attractive force that exists between all objects
Kepler’s laws of Planetary Motion
plantes move in ellipses with the sun at one focus
a planet covers the same amount of space in the same amount of time no matter where it is in orbit
a planet’s orbital period is proportional to the size of it’s orbit (semi-major axis)
Newton’s Law of Universal Gravitation
grav. force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers
F = m1 x m2 / r²
What can r be replaced with in the formula?
“d”
Eccentricity
the deviation of a circular orbit