physics - gravitational fields (D.2)

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gravitational field definition

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13 Terms

1

gravitational field definition

a region of space in which an object experiences a force due to its mass

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2

field lines

show the direction a particle will travel if placed into a gravitational field; always point towards the mass responsible for them

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3

gravitational potential definition

work done per unit mass in moving a small test mass from a point of zero potential (infinity) to a point in the field

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4

kinetic energy formula

(GMm)/(2r)

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5

total energy formula

(-GMm)/(2r)

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6

kepler’s first law

planetary orbits are elliptical with a star at the focus

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7

kepler’s second law

the line connecting the orbiting object to the star sweeps out equal areas in equal times

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8

kepler’s third law

the square of the periodic orbital time of an orbiting object is directly proportional to the cube of the semimajor axis (radius) of its orbit

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9

gravitational potential difference definition

the work done in moving a mass between two points in a gravitational field

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10

polar orbit

satellites orbit over the earth’s poles in one plane, intersecting the earth’s center, with earth rotating underneath

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11

geosynchronous orbit

satellites stay in the same area of sky and typically follow a figure-of-eight orbit (orbit at a greater distance from earth than polar orbits)

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12

geostationary orbit

satellites orbit above the plane of the equator and will not appear to move when viewed from the surface

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13

a loss in the orbital energy -ΔE leads to a decrease in the orbital radius Δr that has two contributions:

  • a loss of gravitational potential energy -2ΔE

  • a gain in kinetic energy +ΔE

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