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Constellation
a region of the sky
not scientfically significant
1603
system for naming stars with greek letters
magnitude
refers to brightness
0 is the brightest 6 is the dimmest
the larger the magnitude the dimmer the star
Star trails
shows the circular motion of the sky
everything rises in the east and sets in the west
stars remain in fixed postions
Archaeastronomy
study of how ancients viewed the universe
Many cultures around the world
observed the sky and marked important
alignments.
Ancient structures
stonehenge, carcol, mayan city, Tulum Mexico
Astronomy of greece
Derived from previous civilizations ( babylon and Egypt)
Greek astronomy is better known as written documents
First ones actually tried to understand the universe as far as we know
Pythagoras
noticed mathmatical patterns in nature
Thales of Miletus
Believed humans could understand the universe and how it works
Plato
believed we see a distorted shadow of perfect form
believed the perfect form was a circle
Aristotle
divided universe into two parts heaven and earth
Argued Earth not moving because he
saw no parallax
argued that
if the Earth were
moving we would
see the star
positions changing
Parallax
Change in postion in an object due to change in location of the observer
Ptolmaeus
explained retrograde motion by a system of wheels withing wheels
Eratosthenes
Measured the circumference of the earth 2500 years ago
Middle ages (europe)
Ancient greek writing perserved by Islamic nations for centuries
Copernicus
came up with Heliocentric model
Galileo Galilei
based on observations with a telescope
Moon was not perfect
Milky Way made up of
stars
Jupiter had moons
The heavens weren’t so
perfect anymore
Inquisition
waxing
describes increasing amounts of visible light reflecting off the moon
waning
describes decreasing amounts of visible light reflecting off the moon
Crescent
describes the moon when less than half of the visible moon surface is illuminated
Gibbous
more than half of the visible moon surface is illuminated
Umbra
full shadow
penumbra
partial shadow
First quarter
the waxing half moon that appears when the moon has traveled one quarter of its orbit around the earth
Third/last quarter
the waning half moon that appears when the moon has traveled three quarters of tis orbit around the earth
why does the moon shine?
reflects light
Luminous
produces its on light
ex. the sun
Illuminated
lit up by something
ex. sun lights up the moon
IMPORTANT
The full moon rises at sunset
the moon orbit is not a perfect circle
Solar eclipse
sun being eclipsed
Lunar eclipse
moon being eclipsed
Path of totality
moons shadow going across the earth
Celestial sphere
a giant sphere extending from the earth which celestial objects reside. describing what the sky looks like as we see it
Parts of a celestial sphere
north south east and west on the horizion. the north and south celestial poles and celestial equator are directly above earth’s counterparts.
Zenith
directly overhead of observer
Nadir
directly below observer
ecliptic
the apparent motion of the sun and planets across the sky
Right ascension
east and west
declination
north and south
telescope
can use equitorial mount
equinox
when the ecliptic and celestial equator intersect the sun crosses the celestial equator
solstice
when the sun is furthest from the celestial equator highest or lowest point in the sky
analemma
when you take a picture of the sun everyday for a year it traces out a certain shap the ends are solstices and intersection is equinox
altitude of the sun
further south in winter and further north in summer
angle of the sun
in the winter we are tilted away from the sun more than we are in the summer
axial tilt
tilt from the sun which causes the seasons
Tides
cyclic rise and fall of sea levels
caused by the combined effect of gravitation forces exerted by the moon, sun, and rotation of the earth
high tide
when water levels are highest
low tide
when water levels are the lowest
tidal range
the difference in height between high and low tide
typical tidal ranges in the open ocean are about 2 feet
coastal tidal ranges can greatly vary from 0 to 52 feet
Gravity and Inertia
work together to create the two major tidal bulges on earth
Inertia
the tendency of moving objects to continue moving in a straight line
Spring tides
occur during new and full moons
they occur twice a month
greatest tidal range
higher than normal high tides and lower than normal tides
sun moon and earth are aligned
when sun earth and moon are aligned the combined gravitational pull creates larger tidal bulges and lower low tides
Neap tides
occur during first and third quarter moon
occur twice a month
little tidal range
sun moon and earth are located at right angles to eachother
hightides are a little lower and low tides are a little higher than average
Semidiurnal tides
most coastal areas experience semidiurnal tides
two equal high tides and two equal low tides
Diurnal tides
only one high tide and one low tide per day
Mixed semidiurnal tides
two unequal hightides and two unequal low tides
diurnal inequality
the difference in height between high or low tides
ptolemaic system
considered the standard model of the universe until the copernican revolution