gravitational fields - theme D Flashcards

1
Q

Kepler’s first law of orbital motion

A

First law: each planet orbits the Sun along an elliptical path. The sun is located at a focus of the elliptical orbit

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2
Q

Kepler’s second law of orbital motion

A

second law: the imaginary line joining the Sun and a planet sweeps equal areas of space in equal time intervals as the planet follows its orbit

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3
Q

Kepler’s third law of orbital motion

A

third law: the square of the orbital period of a planet is directly proportional to the cube of the average distance of the planet to the sun = Tˆ2 = rˆ3 (r = distance)

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4
Q

Newton’s universal law of gravitation:

A

every object in the universe attracts every other object with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.

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5
Q

Newton’s universal law of gravitation equation

A

F=G(m1m2)/rˆ2

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6
Q

speed along the trajectory:

A

v= 2πr/T

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7
Q

centripetal force

A

mvˆ2/r

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8
Q

equation for orbital period:

A

T= ((4πˆ2rˆ3)/GM)ˆ1/2

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9
Q

gravitational field

A

any region of space where a mass experiences a gravitational force

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10
Q

gravitational fields act..

A

at a distance
infinite range

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11
Q

gravitational field strength

A

gravitational force per unit mass experienced at a point in a gravitational field

g=GM/rˆ2

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