Gravity | Orbitals | Kepler's Law Flashcards

1
Q

magnitude of the gravitational force on either particle

A

Fg

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2
Q

Every particle of matter in the universe attracts every other particle with a
force that is _______
to the “product of the masses of the particles”

A

Directly proportional

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3
Q

Every particle of matter in the universe attracts every other particle with a
force that is _______to the square of the distance between them.

A

Inversely proportional

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4
Q

The force is extremely small for bodies that are small enough to be brought into the
laboratory, but it can be measured with an instrument called

A

Torsion balance

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5
Q

Henry Cavendish used in 1798 to determine

A

Gravitational constant (G)

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6
Q

Is the most important force on the scale of planets, stars, and galaxies. It is
responsible for holding our earth together and for keeping the planets in orbit about the sun.

A

Gravitation

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7
Q

important on the cosmic scale because at a distance,
without any direct

A

Gravitational force

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8
Q

is the energy stored of an object because of its distance
above the surface of the Earth.

A

Gravitational Potential Energy

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9
Q

GPE formula

A

Eg = mgΔh

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10
Q

is the object’s change in gravitational potential energy in Joules

A

ΔEg

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11
Q

is the vertical displacement of the object in meters

A

Δh

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12
Q

the simplest case. It is also an important case, since many artificial
satellites have nearly circular orbits and the orbits of the planets around the sun are also fairly circular

A

Circular orbit

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13
Q

The only force acting on a satellite in circular orbit around the earth is

A

Earths Gravitational attraction

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14
Q

The first law explains
that all planets move in
elliptical orbits with the
sun at one focus.

A

Law of orbits

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15
Q

The second law describes a
line that connects a planet to
the sun and sweeps out
equal areas in equal times.
When a planet is near the
sun, it travels faster and
sweeps through a longer path
in a given time.

A

Law of areas

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16
Q

The third law mathematically expressed as the square of the period of any planet is
proportional to the cube of the semi-major axis of its orbit.

A

LAW OF PERIODS