How can we describe the position of celestial objects?

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Astronomy—_____________________________________________________________
Celestial objects—_________________________________________________________
Examples: _______________________________________________________________
How can we describe the position of celestial objects?
____________________—angle measured from North (0°) clockwise to East (90°), South
(180°), West (270°) and back to North (360°).
____________________—angle above the horizon between 0° (horizon) to 90° (overhead—
also called the zenith).
What is the Sun’s Apparent Path Across the Sky?
Distinguish between Apparent and Real:
_____________________ The Earth actually rotates and the daily path of the sun through the
sky is caused by Earth’s rotation.
_____________________ We describe the Sun as rising and setting because it looks real, even
though we know the Earth is moving.
Does the Sun’s Path Depend on the Observer’s Location?
The path of the sun through the sky changes with ________________________. Since the
earth is a sphere, the cycle of day and night changes most at the poles and is most constant at
the equator. People at the equator experience approximately __________ hours of daylight
every day and the noon sun is high in the sky and directly overhead for half of the year.
Changes from season to season are hardly noticeable.
As you move _____________ or _____________ of the tropics (23.5°N and 23.5°S), the noon
sun is never directly overhead. You also notice distinct _____________________ and changes
in the length of __________________________.
How Does the Sun’s Apparent Path Change with the Seasons
___________________________________—in New York State the sun rises due ___________
at about 6am and sets due _____________ at about 6pm, giving _________ hours of daylight.
The sun reaches its highest point at solar noon when it is in the southern sky at an altitude of
48°.
_______________________________________—in New York State the sun rises in the
_____________________________at 4:30 am and sets in the _______________________ at
7:30pm providing _________hours of daylight. The sun reaches its highest point at noon
when it is near 72° altitude.
_________________________________________—in New York State the sun rises in the
__________________________at about 7:30 am and sets in the _____________________ at
about 4:30 pm providing just _________ hours of daylight. The sun reaches its highest point
at noon in the southern sky near an altitude of 24°.
Variation in Intensity and Angle of Insolation
When sunlight strikes the surface at an angle of 90° or ____________________________, it
has _____________________________ intensity (heat) because the insolation is concentrated
in the smallest possible area. As the angle __________________________ from 90° to 0°, the
amount of insolation is spread over a greater and greater area and the intensity
____________________________.
The intensity of insolation is greatest at the _______________________ and
_________________________________with increasing latitude. The intensity of insolation
also varies with the ____________________________. Since the maximum intensity
corresponds to the angle of incidence (90°), during the solstices, the maximum intensity shifts
from the Equator to the Tropic of Cancer (23.5°N) on June 21 and to the Tropic of Capricorn
(23.5°S) on December 21.
24.5° Dec 21
48° Mar 21/Sep 23
71.5° Jun 21
Maximum angles of incidence at 42°N in different seasons.
On any given day, the maximum intensity occurs at ___________________when the sun is
highest in the sky. Note the changes in the direction and the length of the shadows.
Relationship of Surface Temperature to Insolation/Seasonal and Daily Maximum
Temperatures
The hottest month of the year is August, not June and the hottest time of day is 3 pm not noon
due to heat build-up. In the summer, due to the higher angle/higher intensity of the sun, we
receive more insolation than we radiate so the earth heats up over the summer.
The same thing happens each day; during the afternoon, we receive more insolation than we
radiate. The opposite happens in the winter and at night.
Variation in the Duration of Insolation
Duration-- _______________________________________________________.
Duration of insolation varies with ____________________ and ______________________.
Only the Equator has _______ hours of daylight all year. At the Equinoxes,
_______________________________ on Earth experiences _________hours of daylight.
Variation in Insolation by Season
Latitude
Duration of
Insolation Summer
Solstice --June 21
Duration of
Insolation
Equinoxes—March
21/September 23
Duration of
Insolation Winter
Solstice—December
21
90°N
24 hrs
12 hrs
0 hrs
40°N
15 hrs
12 hrs
9 hrs
0°
12 hrs
12 hrs
12 hrs
90°S
0 hrs
12 hrs
24 hrs
The Seasons Are Caused by Earth’s Motion
Seasons are caused by:
1. ________________________________________________________________________
2. ________________________________________________________________________
3. ____________________________________________________________________
The Vertical Ray
The vertical ray migrates between 23°N (Tropic of Cancer) and 23°S (Tropic of
Capricorn).
How Do Earth’s Motions Affect the Appearance of Other Celestial Objects?
Constellations—__________________________________________________________
For example: The Big Dipper is called The Plow in Britain and the Great Bear (Ursa
Major) in ancient Greece.
Modern astronomers use the constellations to designate 88 regions of the night sky. This is a
convenient way to map the stars in our sky. This star map shows constellations visible at
about 40° N in March and April. If you find the Big Dipper high in the sky, you can use it to
locate other stars and constellations as shown by the arrows on the chart.
Why Do Stars Seem To Change Their Positions?
Earth’s rotation makes stars appear to move through the sky just as the sun appears to
move. In New York State, stars rise in the East and set in the West.
Yearly Apparent Motions
In addition to the apparent daily cycle of motion of stars through the sky, the stars
positions appear to change in a yearly cycle as the earth revolves around the sun.
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