Lec 3 Flashcards
(52 cards)
constellation
a region of the sky with well-defined borders
-the patterns of stars help us locate constellations
north celestial pole
point directly over Earth’s North Pole
south celestial pole
point directly over earth’s south pole
celestial equator
projection of earths equator into space, makes a complete circle around celestial sphere
ecliptic
the path that the Sun follows as it appears to circle around the celestial sphere once each year
-crosses the celestial equator at 23.5 deg (tilt of earth’s axis)
local sky
the sky as seen from where you are standing, appears to take the shape of a hemisphere or dome
(explains why ppl of ancient cultures imagined we live on a flat earth)
horizon
boundary between Earth and sky
zenith
point directly overhead
meridian
imaginary half circle stretching from the horizon due south, thru zenith, to the horizon due north
azimuth
direction
-helps to pinpoint the position of any object in the local sky by stating its direction along the horizon, which’s degrees cw from due north and its ALTITUDE above horizon
angular size
the angle an object appears to span in your field of view
e.g. moon and sun are 0.5deg
-also depends on distance
angular distance
b/w a pair of objects in the sky is the angle that appears to separate them
circumpolar
when stars near the north celestial pole remain perpetually above the horizon, circling (ccw) around the north celestial pole each day
when a stars daily circle is entirely above your horizon
stars near the south celestial pole…
never rise above the horizon at all
latitude
measure north-south position
0 deg at the equator, increases to 90degN at North pole and 90degS at south pole
affects the constellations we see because it affects the locations of the horizon and zenith relative to celestial sphere
longitude
measures east-west position
-passes through prime meridian
the altitude of the celestial pole in your sky is equal to..
your latitude
zodiac
made up by constellations along the ecliptic
what determines how we can see constellations at night?
the sun’s apparent location
what causes seasons?
the tilt of Earth’s axis causes sunlight to fall differently on
Earth at different times of year
Step 1
–tilt of Earth’s axis, which remains pointed in same direction in space (toward Polaris) throughout yr
–as a result, the orientation of the axis relative to the Sun
changes over the course of each orbit: The Northern Hemisphere is tipped toward the Sun in June and away from the Sun in December, while the reverse is true for the Southern Hemisphere.
That is why the two hemispheres experience opposite seasons
the changing angle
of sunlight on the two hemispheres leads directly to seasons
how does the tilt of the sunlight affect the seasons?
the axis tilt causes sunlight to strike the Northern Hemisphere at a steeper
angle and the Southern Hemisphere at a shallower angle
the steeper sunlight angle makes it summer in the N hemisphere for 2 reasons
1) steeper angle means more concentrated sunlight, which tends to make it warmer
2) as Earth rotates each day, you’ll see that the steeper angle also means the Sun follows a longer and higher path through the sky, giving the Northern Hemisphere more hours of daylight during which it is warmed by the Sun
how does the angle tilt of the sun cause winter?
The shallower sunlight angle makes it winter there because sunlight is less concentrated and the Sun follows a shorter, lower path through the sky
june solstice
called the summer solstice in the Northern Hemisphere, occurs around June 21 and is the moment when the Northern Hemisphere is tipped most directly
toward the Sun and receives the most direct sunlight
december solstice
called the winter solstice in the Northern Hemisphere, occurs around December 21 and is the moment when the Northern Hemisphere receives the least direct sunlight