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56 Cards in this Set
- Front
- Back
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basic ideas about universe's formation
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-big bang created space and time, not just energy and matter, roughly 14 billion years ago.
-denser regions of Big Bang collapsed under gravity, formed galaxies. Smaller clumps probs coalesced to form larger clumps. -conservation of angular momentum: as the system gets smaller, it has to rotate faster to conserve angular momentum. Reason galaxies spin faster as they get smaller. |
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basic ideas about character of universe
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plays according to rules (Eienstein's General Theory of Relativity) that are very different from our everyday experience
-space is "warped" by the presence of matter |
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spiral galaxies like our own Milky Way
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-flat swirling disk of material divided up, apparently, into spiral arms
-bright central nucleus -halo of globular clusters -nature of rotation suggests black hole at center |
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conservation of angular momentum: equation
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L=mvr
-angular momentum L for localized mass m moving with a velocity v in a circular orbit of radius r -remains constant in the absence of external torques |
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basic ideas about contents of universe
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-gas, dust, dark matter
-stars: fusion from weight of overlying material compresses center of the star-->center material (mostly Hydrogen) is ionized (electrons separated from protons), then protons can combine to make heavier nuclei. large energy release |
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planets are the leftovers of ___
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star formation
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why is the solar system almost entirely in one plane?
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pre-stellar cloud collapsed, flattened out as it spun faster due to angular momentum
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T Tauri wind
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"after the sun lit up a strong "wind" of particles swept light elements out of the inner solar system, leaving small planets composed of relatively heavy elements."
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Constellations
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Historically: figures associated with star patterns
Today: sky divided into sections roughly associated with the historical figures |
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Star names
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Bright stars usually have many
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the magnitude system
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-Brightest stars (roughly)--1st magnitude
-Faintest naked eye stars (roughly)-- 6th magnitude -difference in 5 magnitudes corresponds to a factor of 100 in intensity, so each magnitude corresponds to a factor of about 2.5. |
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what causes the apparent rotation of the celestial sphere?
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the rotation of the earth causes this illusion.
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North and south celestial poles (NCP and SCP)
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"the points on the CELESTIAL SPHERE directly above the N and S poles of the earth"
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Celestial equator (CE)
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a circle around THE CELESTIAL SPHERE above the earth's equator, 90 degrees from the NCP and SCP. Just like the Earth's equator
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Zenith
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-point on THE SKY directly overhead
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Meridian
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the semicircle in THE SKY extending from N. Horizon, through the zenith, to the S horizon
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Horizon
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Point on THE SKY which divides the earth and the sky
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circumpolar stars
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stars that never set as seen from a particular location
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Where is the NCP at the earth's N pole?
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directly overhead
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Where is the NCP at the earth's equator?
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on the N horizon
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Where is the NCP and CE as seen from a latitude in between the north pole and the equator, like Grinnell?
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Altitude of the NCP above the N horizon is equal to the observer's latitude. (CE is 90 degrees from NCP)
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declination
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the N/S coordinate measured in degrees (+ and -) from the celestial equator. Like latitude on the earth
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Right Ascension
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The E/W coordinate in the CELESTIAL SPHERE measured in hours (0-24). Like longitude on the earth.
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sketches of NCP, observer, CE, horizon, etc. only show stars on the ___
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meridian
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a star's location above the horizon (in degrees) is ___.
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its altitude (a)
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precession
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-"the direction of the earth's axis of rotation wobbles slightly over time (one revolution in 26,000 years). This is called precession of the equinoxes, or just precession"
-means declination, right ascension of stars changes slightly over time -that polaris is the "pole star" is only a temporary coincidence |
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the ecliptic
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path of the sun on the celestial sphere
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tilt of sun from celestial equator
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23.5 degrees, same as tilt of earth's axis relative to its orbit
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appearance of sun on celestial sphere and on flat star chart
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sine wave-esque
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vernal equinox
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sun on CE going N, first day of spring, about March 21
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summer solstice
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sun at maximum declination (+23.5), first day of summer, about June 21
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Autumnal equinox
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sun on CE going S, first day of fall, about September 21
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winter solstice
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sun at minimum declination (-23.5), first day of winter, about December 21
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why is summer warmer than winter?
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sun is up longer, gets higher in the sky
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solar day
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-time for the sun to return to the meridian.
-about 4 minutes longer than sidereal day |
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sidereal day
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-time for a star to return to the meridian
-about 4 minutes shorter than solar day -for this reason stars rise about 4 minutes earlier each night |
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why do planets tend to follow the ecliptic?
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because the solar system is on the same plane, more or less.
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retrograde loops
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loops planets make in their motion along the ecliptic
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the ecliptic and constellations
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ecliptic more or less passes through
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planet speeds vary with ___ and ___
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individual planet, time
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motion of the moon in the sky
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-approximately follows ecliptic because moon's orbit is only slightly inclined to the earth's orbit
-takes about one month to go around the earth, so takes about one month to go around the ecliptic |
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What would the moon's motion be like if it did not move in its orbit?
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E-->W
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Which way does the moon actually move in the sky and why?
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-E-->W
-the earth rotates faster than the moon orbits |
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New moon
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near sun in sky, invisible
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1st quarter moon
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90 degrees east of sun in sky, half visible
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full moon
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opposite sun in sky, fully visible
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3rd quarter moon
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90 degrees west of sun in sky, half visible
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solar eclipse
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-moon passes between sun and earth, casting shadow on earth.
-full solar eclipses rare: moon's shadow on earth is small |
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lunar eclipse
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-moon passes directly behind the earth relative to the sun, so earth's shadow falls on the moon.
-everyone who can see the moon at that time can see the eclipse |
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Ptolemaic model of the universe
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-earth at the center (geocentric), other objects rotate around
-sun, moon, planets revolve on epicycles (small orbits) that are attached to the main orbit (deferent) |
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why not Ptolemaic model?
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-stellar parallax unaccounted for
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copernican model
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-earth, other planets orbit the sun (heliocentric)
-retrograde loop, other phenomena understood as apparent rather than real -religious consequences |
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Kepler's first law
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-planets move in elliptical orbits with the sun at one focus of the ellipse
-for the planets in our solar system, these ellipses are almost circles |
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Kepler's second law
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-the sun-planet line sweeps out equal areas in equal times.
-means that a specific planet moves faster when it is closer to the sun -*reflects conservation of angular momentum! |
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Kepler's third law
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-P[squared] is proportional to r[cubed]
-but actually an equality if P is measured in years where p is the period and r is the radius of the orbit -means planets with smaller orbits move more rapidly |
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evidence for the Copernican model
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-retrograde loops are explained
-kepler's laws of planetary motion work -correct phases of the inner planets are observed -observations of jupiter's (and other planets') moons-->earth not the unique center of revolution -stellar parallax is observed -aberration of starlight is observed (shift in star positions resulting from the finite speed of light) -space probes get where they are supposed to go |