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37 Cards in this Set
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- Back
- 3rd side (hint)
ptolemaic model
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each planet moves on a small circle whose center moved around the earth on a larger circle
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copernicus
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known for his sun centered model and published a book about it
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tycho
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he was an eccentric genius who observed a nova "new star" and concluded that the sun orbits earth while all other planets orbit the sun.
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Kepler
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discovered planets orbits was an ellipse and 3 laws of planetary motion
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keplers 1st law of planetary motion
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the orbit of each planet about the sun is an ellipse with the sun at one focus.
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keplers 2nd law of planetary motion
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the line that connects the planet to the sun sweeps out equal areas in equal time.
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keplers 3rd law of planetary motion
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more distant planets orbit the sun at slower average speeds obeying the precise mathematical relationship
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copernican model
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sun at center
no epicycles circular orbits |
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tycho brahes model
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combined ptolemaic and copernican models
tracked the position of the stars |
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eccentricity
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it is a measure of how weird the planets are moving.
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sir Isaac newton
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taught himself everything
used mathematics to explain motion invented calculus first to point a teloscope in the sky wrote first physics textbook |
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newton's laws of universal gravitation
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we feel weight because gravity is pulling us down.
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theory
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is not something that remains true but a large body of evidence must be able to back it up.
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radiative energy
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energy carried by light
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law of conservation of energy
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energy cannot appear or disappear. objects can gain or lose energy only by exchanging energy with other objects.
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conserving energy with other planets
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thermal energy
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measures the total kinetic energy of all the randomly moving particles.
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Kelvin
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Kelvin does not have negative temperatures and it starts at the coldest at absolute zero which is 0 Kelvin
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gravitational potential energy
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depends on its mass and how far it can fall as a result of gravity. an object has more gravitational potential energy when it is higher and less when it's lower.
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bound orbits
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objects go around and around another object and gravity creates a bond that holds the objects together.
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unbound orbits
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paths that bring an object close to another object just once. for example a comet.
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speed of light
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300,000 kilometers per second
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photons
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pieces light comes in that has a precise wavelength,frequency, and energy.
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infrared light
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light with wave lengths somewhat longer than red light.
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radio waves
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longest wave length light.
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not sound but light waves
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emission line spectrum
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when a thin and low density gas is involved it does not produce a continuous spectrum but it consists of bright emission lines against a black background.
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continuous spectrum
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spectrum of an ordinary light bulb that spans a broad range of wavelengths.
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absorption line spectrum
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with the gas between the light bulb and us we see most of the continuous light but the cloud of gas absorbs specific wavelengths and so the spectrum also shows dark absorption lines.
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emitted light
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anything with a temperature above absolute zero.
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blueshift
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objects that are coming towards us has shorter wavelengths
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redshift
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if an object is moving away from us it has longer wavelengths.
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adaptive optics
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which eliminates much of the blurring caused by our atmosphere by cancelling out the atmospheric distortions.
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interferometry
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allows two or more individual telescopes to achieve an angular resolution of a much larger telescope.
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moons circling Jupiter
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lo, europa, ganymede, callisto
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Hubble space telescope
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observes ultraviolet or infrared wavelengths that don't reach the ground.
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galileo
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perfected telescope that was used in astronomy
found support for copernican model used observations vs pure thought Venus had full set of phases moon has mountains and sun spots that was not a perfect sphere discovered 4 new planets circling Jupiter galileo got house arrest for testing Aristotles belief |
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perihelion
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close part of the sun
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apehelion
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farthest part of the sun
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