L5 physics and gravity

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36 Terms

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speed

rate at which object moves, distance/time in m/s

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velocity

speed AND direction e.g. 10 m/s due east

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Galileo showed that g is

same for all falling objects regardless of mass

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momentum changed by

a net force, usually meaning an acceleration

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angular momentum

rotational momentum of a spinning or orbiting object

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what is needed to change an object’s angular momentum

a torque

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mass

a measure of amount of matter in an object

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weight

the force that a scale exerts upon an object

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why are astronauts weightless in space

there is gravity and in a continued state of free fall

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what did newton do

extrapolated physical laws of Earth to heavens, laws of motion and gravity, experiments with light, invention of calculus

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newton’s first law of motion

an object moves at constant velocity unless a net force acts to change its speed or direction

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newton’s second law of motion

force = mass x acceleration = rate of change in momentum

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newton’s third law of motion

for every force there is always an equal and opposite reaction force

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conservation of momentum

objects continue at constant velocity, total momentum of interacting objects cannot change unless an external force is acting on them + they exchange momentum through equal and opposite forces

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conservation of angular momentum

figure skater bringing arms in makes them go faster

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types of energy

kinetic = motion, radiative = light, potential = stored

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conservation of energy

energy can transfer between objects or change forms, but cannot be created or destroyed

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thermal energy

the collective KE of many particles, depending on both temperature and density

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temperature

measure of the average KE of many particles in a substance

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on Earth, gravitational potential energy depends on 

object’s mass, strength of gravity, and height above the ground

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object/gas cloud and gravitational potential energy

has more when it is spread out than when it contracts, which converts it to thermal energy

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mass energy relationship

E = mc² - small mass, big energy

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concentrated energy can spontaneously 

turn into particles

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universal law of gravitation

every mass attracts every other mass with Fg = Gm1m2/d²

G is gravitational constant, d is distance between them

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types of orbital paths

bound (ellipses) and unbound (parabola, hyperbola) e..g extra-solarsystem comet that just leaves

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center of mass and orbits

because of angular momentum conservation, orbiting objects orbit around their combined center of mass

<p>because of angular momentum conservation, orbiting objects orbit around their combined center of mass</p>
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gain or loss of orbital energy from

gravitational encounter, friction or atmospheric drag

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escape velocity

if an object gains enough orbital energy, it may escape (change from bound to unbound orbit

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angular momentum equation

mass x velocity x radius

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total mass of a system from orbits/ newton and kepler’s third law

M1 + M2 = 4π²a³/Gp² (p = orbital period, a = avg orbital distance between centers)

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total orbital energy is

constant ; gravitational potential + kinetic energies

<p>constant ; gravitational potential + kinetic energies</p>
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causation of tides

Moon’s gravity pulls harder on near side of Earth than on far side

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tidal friction

gradually slows Earth’s rotation and makes Moon get farther, caused Moon’s tidal locking - removal of energy from the system

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spring tide

new moon and full moon, tidal forces of Sun and Moon work together to create lowest lows and highest highs

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neap tide

first and third quarters, Sun and Moon work against each other, highest lows and lowest highs

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relationship between gravitational acceleration and mass

DOES NOT EXIST