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56 Cards in this Set

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basic ideas about universe's formation
-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.
basic ideas about character of universe
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
spiral galaxies like our own Milky Way
-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
conservation of angular momentum: equation
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
basic ideas about contents of universe
-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
planets are the leftovers of ___
star formation
why is the solar system almost entirely in one plane?
pre-stellar cloud collapsed, flattened out as it spun faster due to angular momentum
T Tauri wind
"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."
Constellations
Historically: figures associated with star patterns
Today: sky divided into sections roughly associated with the historical figures
Star names
Bright stars usually have many
the magnitude system
-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.
what causes the apparent rotation of the celestial sphere?
the rotation of the earth causes this illusion.
North and south celestial poles (NCP and SCP)
"the points on the CELESTIAL SPHERE directly above the N and S poles of the earth"
Celestial equator (CE)
a circle around THE CELESTIAL SPHERE above the earth's equator, 90 degrees from the NCP and SCP. Just like the Earth's equator
Zenith
-point on THE SKY directly overhead
Meridian
the semicircle in THE SKY extending from N. Horizon, through the zenith, to the S horizon
Horizon
Point on THE SKY which divides the earth and the sky
circumpolar stars
stars that never set as seen from a particular location
Where is the NCP at the earth's N pole?
directly overhead
Where is the NCP at the earth's equator?
on the N horizon
Where is the NCP and CE as seen from a latitude in between the north pole and the equator, like Grinnell?
Altitude of the NCP above the N horizon is equal to the observer's latitude. (CE is 90 degrees from NCP)
declination
the N/S coordinate measured in degrees (+ and -) from the celestial equator. Like latitude on the earth
Right Ascension
The E/W coordinate in the CELESTIAL SPHERE measured in hours (0-24). Like longitude on the earth.
sketches of NCP, observer, CE, horizon, etc. only show stars on the ___
meridian
a star's location above the horizon (in degrees) is ___.
its altitude (a)
precession
-"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
the ecliptic
path of the sun on the celestial sphere
tilt of sun from celestial equator
23.5 degrees, same as tilt of earth's axis relative to its orbit
appearance of sun on celestial sphere and on flat star chart
sine wave-esque
vernal equinox
sun on CE going N, first day of spring, about March 21
summer solstice
sun at maximum declination (+23.5), first day of summer, about June 21
Autumnal equinox
sun on CE going S, first day of fall, about September 21
winter solstice
sun at minimum declination (-23.5), first day of winter, about December 21
why is summer warmer than winter?
sun is up longer, gets higher in the sky
solar day
-time for the sun to return to the meridian.
-about 4 minutes longer than sidereal day
sidereal day
-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
why do planets tend to follow the ecliptic?
because the solar system is on the same plane, more or less.
retrograde loops
loops planets make in their motion along the ecliptic
the ecliptic and constellations
ecliptic more or less passes through
planet speeds vary with ___ and ___
individual planet, time
motion of the moon in the sky
-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
What would the moon's motion be like if it did not move in its orbit?
E-->W
Which way does the moon actually move in the sky and why?
-E-->W
-the earth rotates faster than the moon orbits
New moon
near sun in sky, invisible
1st quarter moon
90 degrees east of sun in sky, half visible
full moon
opposite sun in sky, fully visible
3rd quarter moon
90 degrees west of sun in sky, half visible
solar eclipse
-moon passes between sun and earth, casting shadow on earth.
-full solar eclipses rare: moon's shadow on earth is small
lunar eclipse
-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
Ptolemaic model of the universe
-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)
why not Ptolemaic model?
-stellar parallax unaccounted for
copernican model
-earth, other planets orbit the sun (heliocentric)
-retrograde loop, other phenomena understood as apparent rather than real
-religious consequences
Kepler's first law
-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
Kepler's second law
-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!
Kepler's third law
-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
evidence for the Copernican model
-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