Chapter 2 Flashcards
phase of the moon between waxing crescent and waxing gibbous
first quarter
phase between third quarter and new moon
waning crescent
full moon is sets
sun rise
new moon is rises
sun rise
moon is setting at midnight
first quarter
astronomers see stars right next to the sun
with space telescopes
constellations that the Sun passes through
zodiac
meridional altitude
height of the Sun in the sky at noontime
On the equator, the Sun will reach its highest point in the sky
the summer solstice
phase between waning crescent and waxing crescent
new moon
On an equinox, the Sun sets
due west
Over the course of the year, the right ascension of the Sun
increases
calculate the peak altitude of the Sun in the sky
by using the observer’s latitude and the sun’s declination
On the summer solstice, the Sun sets
North of West
moon is rising at midnight
third quarter
Over the course of the year, the Sun’s declination
increases and decreases
moon is setting at noon
third quarter
Your noontime shadow will be the longest on
winter solstice
The longest day of the year in Michigan is
the summer solstice
The length of the day on an equinox
12 hours
On the winter solstice, the Sun will rise
South of East
Lunar eclipse
earth’s shadow falls on the moon
Cycles of the moon
New->waxing crescent->first quarter->waxing gibbous->full->waning gibbous->third quarter->waning crescent
full moon
100% bright
1st and 3rd quarter
50% bright
waxing
brightness if increasing
waning
brightness is decreasing
gibbous
moon is more than 50% bright
crescent
moon is less than 50% bright
synodic month
29.5 days, amount of time it takes to complete one cycle of phases
Horizon diagram
tool we can use to show what an observers sky looks like
nadir
opposite point directly point below the observer
celestial meridian
imaginary line that runs in the sky from north to the south
time of day
position of the sun in the sky
phase of the moon
how far the moon is from the sun
SOHO
tool used to take pictures of the sun
meridional altitude
changes in the height of the sun
meridian
north-south line of the observers in the horizon coordinate system
tilt of axis
causes the seasons
no eclipse every new and full moon
because of ecliptic plane
solar eclipse
moon blocks ar view of the sun