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Science
4th quarter
7 moon phases
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Moon
Does not produce
light
,
reflects
the sun's light
Moon
's rotation and orbit
1. Moon
rotates
on its own axis
2. Time for moon to
rotate
on axis equals time for moon to orbit
Earth
3.
Earth
orbits around the
sun
Moon
's position relative to Earth and sun
Determines the different
moon phases
New
moon
Barely visible,
Earth
and moon aligned, sun and earth on
opposite
sides of moon
Waxing
crescent moon
Moon
begins to become
visible
again after new moon
First
quarter moon
Moon reaches
first
quarter of orbit around earth, looks like
half-moon
Waxing
gibbous moon
Visibility of moon getting bigger, bigger than
semicircle
but smaller than
full moon
Full
moon
Moon is on
opposite
side of Earth
Waning
gibbous moon
Amount of moon visible begins to
decrease
, more than
half
still visible
Third
quarter moon
Opposite
view of first quarter, looks like
half moon
Waning
crescent
moon
Less than half of moon still visible
Lunar
eclipse
Sun, Earth, and Moon align so Moon passes into Earth's shadow
In total
lunar
eclipse
, entire Moon falls within umbra (darkest part of Earth's shadow)
Moon turns reddish hue, sometimes called "Blood Moon"
Lunar
eclipses
occur when the Sun, Earth, and Moon align so the Moon passes into Earth's shadow
In a total
lunar
eclipse
, the entire Moon falls within the darkest part of Earth's shadow, called the umbra
When the Moon is within the umbra, it will turn a reddish hue.
Lunar
eclipses
are sometimes called "Blood Moons" because of this phenomenon
Solar
eclipses
are caused by the Moon coming exactly between the Earth and the Sun, blocking all but a small shadow of the Sun's light to the Earth
Lunar eclipses are caused by the
Earth
coming directly between the
Sun
and the Moon, casting a shadow on the Moon
Solar and lunar eclipses do not occur every month because the
Moon's
orbit is tilted to the
Earth's plane of orbit around the Sun
The
moon
is always half-lit by the sun
The
moon
phases
are caused by observing the half-lit moon at different times during its orbit of the Earth
Solar
eclipses
can only be observed by a small number of people because of the small size of the shadow
Lunar
eclipses
can be observed by everyone on the night-side of the Earth