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the study of the Universe in which humans live
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smallest measurable unit of time
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| How many constellations today? |
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88; 40 new, 48 are from classical age by Babylonians, Egyptians, Mesopotamians, and Greeks.
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what used to define a group of stars, now defines a section/area of sky with clear boundaries
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Groupings of stars, smaller than a constellation. For example: The Big Dipper is an asterism of the constellation Ursa Major.
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Daily motion of the sun, moon, planets and stars
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means "around the pole"; stars that circle the pole and never set
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radius: 23.5deg; due to the fact that the earth is not a perfect sphere. It's top-like motion. Moves reference marks such as celestial poles.
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first appeared in writings of Ptolemy; 1st mag. to 6th mag. 1 mag= 2.5 factor in brightness.
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inversely related to the square of its distance. If a star is twice as distance, 2^2 is 4...1/4 the luminosity of the first star.
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Astronomical Unit; average distance between the earth and sun. (1.5 x 10^11 km
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first to calculate circum. of earth
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Measured relative sizes of earth/moon/sun; was far off, but established that the sun was far away and larger than earth
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geocentric model; traced out the ecliptic
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anytime the sun crosses the celestial equator, even amount of sunlight per day.
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March 21st, our calendar's zero
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Point where the sun is furthest north or south
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furthest from the sun (July 6th)
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closest to the sun (Jan 3rd)
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| An effect of the tilt of the earth's axis |
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it causes sunlight to be more/less direct, which causes our seasons!
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orbital period of the moon relative to the stars. 27.3 days
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orbital period relative to the sun; time between successive new moons, 29.5 days (has to catch up to the sun, who has moved a degree a day across the sky.
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defined to be 24 hours. rotates 361 degrees to meet back to the sun after moving across its revolution.
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relative to the stars, 23 hr. 56min.
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only occurs when the line of nodes points toward the sun.
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| Tilt between earth and lunar orbital plane: |
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| Amount of eclipses in a year |
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min. 2 and max. 7 in one year
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observer sees partial covering of the sun; surrounds the umbra
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observer sees the sun completely covered, darkest portion of shadow
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beyond the apex of the umbra, observer sees partial covering of the sun because the object covering is not large enough; only solar eclipses
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occurs when the earth casts its shadow onto the moon; seen by everyone who can see the moon; separated by six months
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| Length of Totality during Total Solar Eclipse |
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no more than about 7 minutes
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| Length of partial coverage from a Solar Eclipse |
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gas being projected off and back down to the Sun and above the Chromosphere
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The ring of white light emission during total solar eclipse
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caused by mountains and valleys on Moon's surface; little rim of sun shining through on the edges
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a partial eclipse where it can only be seen through the antiumbra, where there is an annulus, or ring.
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an eclipse cycle that has a period of about 18 years, 11 days, and 8 hours.
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geocentric, used epicycles, was used for 1400 years, very accurate
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heliocentric, still used perfect circular motion, not as accurate as Ptolemy's model
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circle about which an epicycle travels
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point about which the epicycle seems to make uniform circular motion about the deferent
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circle about which planet travels, used to explain motions like retrograde motion
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Copernican's writing over heliocentricity
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