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rotation
The action of spinning an object around an axis
1 rotation equals
1 day or 24 hours
revolution
1 full orbit around the sun
1 revolution equals
1 year
the tilt of the earth
causes seasons
23.5 degrees
why the tilt of the earth causes seasons
sunlight hits the earth more directly on the part facing the sun
longer days
northern vs southern hemisphere
when it is summer in the northern hemisphere, it is winter in the southern hemisphere
when 1 part of the earth is pointed towards the sun, the other is pointed away
Summer in the northern hemisphere
is winter in the southern hemisphere
spring and fall
in these seasons, the northern and southern hemisphere receive equal amounts of sunlight
change of daylight hours
change of daylight hours throughout the year
is greatest at the poles
least near the equator
aka near the equator the days don’t get as short in winter
which part of the earth is it summer
depends on the part of the earth that is tilted towards the sun
apparent size
size as seen from earth
the moon and sun have similar apparent sizes
phases of the moon
the very predictable pattern of what the moon looks like from the earth
two major features of the moon
highlands and maria
highlands
lighter, raised areas of the moon
has a lot of craters from impacts with asteroids
maria
latin for sea
darker, low areas formed by lava cooling down
Has less craters due to being younger rock
tidal locking
when one side of the moon always faces the earth
time for 1 orbit = time for 1 rotation
near side of the moon
the side of the moon that is always facing us on earth
far side of the moon
the side of the moon that is always facing away from us on earth
not any darker than the near side
has almost no maria
manned missions to the moon
are more expensive and can’t go to all the places that robots can go to
tides per day
each day has 2 high tides and 2 low tides
high tide
when the water level at the coast is higher than normal
low tide
when the water level at the coast is lower than normal
how long tides are separated by
6 hours
tidal force
a difference in gravitation pull from 1 side of a celestial object to another
bulge
the squeezing of the earth and moon as a result of tidal forces
spring tide
when the tidal force from the moon and sun line up and enhance one another.
extra high high tide and low low tide (big change in water level)
neap tide
when the tidal force from the moon and sun don’t line up and cancel each other out.
low high tide and high low tide (little change in water level)
proxigean tide
when a spring tide occurs while the moon is close in it’s elliptical orbit.
MAXIMUM TIDES
solar eclipse
the earth passes into the shadow of the moon, blocking the sun from our view
totality is only visible by a small area on earth
lunar eclipse
the moon passes into the shadow of the earth, blocking light from reaching the moon
visible by everyone on earth
totality
the darkest part of the shadow of an eclipse. For a solar eclipse, it is small and moves across the earth
only time it’s safe to take off your eclipse glasses
how many days is the orbit of the moon
27 days
corona
the layer of the sun that is visible during a total solar eclipse
photosphere
the layer of the sun that is blocked during a total solar eclipse
who can see a lunar eclipse
everyone on earth facing the moon
who can see a total solar eclipse
only people in the path of the moon’s shadow
eye protection
is required during a solar eclipse
don’t stare at the sun
new moon
phase of the moon where the we only see the dark side
occurs during a solar eclipse
waxing
growing or getting larger
waning
means getting smaller
gibbous
means rounded
refers to a shape larger than a crescent
quarter moons
half moons
quarter refers to completing the moon completing a quarter of its rotation/orbit
full moon
phase of the moon where we only see the bright side
occurs during a lunar eclipse
new moon and full moon
phases of the moon that cause spring tides
first quarter and third quarter
the phases of the moon that cause neap tides