Earth’s Motions Unit 4 I. Rotation 1. The earth spins on an axis 2.The axis of rotation is an...
Transcript of Earth’s Motions Unit 4 I. Rotation 1. The earth spins on an axis 2.The axis of rotation is an...
Earth’s Motions
Unit 4
I. Rotation
1. The earth spins on anaxis
2. The axis of rotation is animaginary line through the earth from north to south pole
•The earth rotates around this axis
•The axis is tilted23½º from vertical
3. The axis always points towardsPolarisThis is calledParallelism of the axis.
A. Results of Rotation
1. Sunrise and set2. Moonrise and set3. Planet rise and set4. Coriolis effect5. Motion of the foucault
pendulum6. Circumpolar motion of stars
7. Location of sunrise/setis due to the direction of rotation…the earth rotates fromwest to east orcounterclockwise
B. Rate of Rotation
1. Angular rate:360º 24 hours15º/hr
2. Velocity is dependent upon latitudeAs latitude increasesvelocity decreases
Equator 40,080 km
1670 km/hr
42º 31,200 km
1300 km/hr
60º 20,140 km
839 km/hr
90º 0 km 0 km/hr
Latitude CircumferenceRate ofRotation
C. Time, the Sun and Earth’s Rotation
•We use the apparent motion of the sun to tell time.
•Time is based upon the actual movement of the earth
•The earth’s rotation causes the apparent rise and set of the sun
•The apparent path of the sun is an arc
•Local solar noon is always the time at which the sun reaches its highest point in its arc–Solar noon in NYS is
never directly overhead!!
Z
II. Revolution
1. The earth travels around the sun
2. The orbit of the earth isan ellipse withthe sun at one of the foci
3. The direction of revolution is counterclockwise
A. Results of Revolution
1. Seasons2. Seasonal changes in
visible constellations3. Parallax4. Retrograde motion
B. Rate of Revolution
1. Angular rate:360º365.25 days~1º/day
2. Velocityradius of revolution is 1.5 x 108
therefore v=2(pi)r Tv = ~ 2,580,822 km/day
(1548493 mi/day)
•Comparative velocity:•The Earth travels fastest when we are closest to the sun andslowest when we are farthest from the sun
III. Seasons in the Northern Hemisphere
Seasons and seasonal changes are due to the revolution of the earth combined withthe tilt of the earth on its axisand parallelism of the axis
A. Summer1. Summer solstice2. June 21st
3. Northern hemisphere is tipped towards the sun
4. Earth is at its greatest distance from the sun (aphelion)
5. Altitude of solar noon is highest
6. Days are longest7. Shadows are shortest8. The sun appears smallest9. Sunrise occurs north of
east10.Sunset occurs north of
west
11.The zenith sun is found at 23½ºN…Tropic of Cancer
12.The north pole experiences 24 hours of daylight
13.The south pole experiences 24 hours of darkness
B. Fall
1. Autumnal equinox2. September 23rd
3. Neither hemisphere is tilted towards the sun
4. The distance to the sun is decreasing
5. The altitude of solar noon is decreasing
6. The length of day is decreasing
7. Shadow length is increasing
8. The sun is looking bigger
9. Sunrise occurs due east10.Sunset occurs due west11. Zenith sun is found at
the equator…0º12.We experience 12
hours of daylight and 12 hours of darkness
C. Winter1. Winter solstice2. December 21st
3. The northern hemisphere is tilted away from the sun
4. The earth is closest to the sun
5. The altitude of solar noon is lowest
6. The length of day is shortest
7. Shadow length is longest8. The sun appears biggest9. Sunrise occurs south of
east10.Sunset occurs south of
west
11. The zenith sun is found at the Tropic of Capricorn…23½ºS
12.The north pole experiences 24 hours of darkness
13.The south pole experiences 24 hours of daylight
D. Spring
1. Vernal equinox2. March 21st
3. Neither hemisphere is tilted towards the sun
4. The distance to the sun is increasing
5. The altitude of solar noon is increasing
6. The length of day is increasing
7. Shadow length is decreasing
8. The sun is looking smaller
9. Sunrise occurs due east10.Sunset occurs due west11.The zenith sun is found
at the equator…0º12.We experience 12
hours of daylight and 12 hours of darkness
Shadows in the northern hemisphere
A shadow castby an object at solar noon in NYS will always pointnorth
June
Sept
DecJanFeb
MarAp
MayJulyAug
OctNov
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IV. The Moon
A. Movements1. Revolution
The moon travels a path thatis an ellipse withthe earth at one of the foci(the other foci is called the barycenter)
Its period of revolution is27 1/3 days and is called asidereal month
2. The moon’s period of rotation is 27 1/3 days …its rotation is synchronous with its revolution
•Because of this synchronicity, the same side of the moon always faces the earth.
•Until we began exploring space, the far side of the moon remained unobserved.
B. Lunar Phenomena
1. Phases of the moon:the changing shape of the visible moon due to the revolution of the moon around the earth
•Because the earth is revolving around the sun as the moon revolves around the earth, one complete cycle of phases takes longer than one complete revolution
•One cycle of phases takes29½ days and is called asynodic month
waxing
waning
crescent
New moon
crescent
quarter
¾ or gibbous
Full moon
¾ or gibbousquarter
Waxing…when the visible portion of the moon is becoming larger
Waning…when the visible portion of the moon is becoming smaller
2. Eclipsesa. Terms:
i. Umbra: The darkest part of the shadow cast by the earth or the moon. The surface is completely blocked from view.
ii. Penumbra: The area of partial shadow surrounding the darkest part of the shadow cast by the earth or the moon. The surface is only partially blocked from view.
b. Lunar eclipse:when the moon is in the shadow of the earthThe moon must be in the full moon phase:S – E – M
c. Solar eclipse:when the earth is in the shadow of the moonThe moon must be in the new moon phase:S – M – E
d. We don’t experience eclipses with every new and full moon because the plane of the moon’s orbit is tilted 5º to the plane of the earth’s orbit
e. When the moon is at perigee and the sun is at aphelion, the surface of the sun is completely “blocked”When the moon is at apogee and the sun is at perihelion, we see an annular eclipse in which the sun is seen as a ring around the moon’s shadow
3. Tides•The cyclic rise and fall of ocean water on the earth.
•They are caused by the gravitational attraction between the moon and the earth’s waters…and, to a lesser degree, the sun and the earth
•Tidal events occur every6 hours
•The position of the moon affects the degree of the tides
a. S – E – M = Full MoonorS – M – E = New Moonthe sun and the moon work “together” to create extreme tides…Spring tidesvery high, high tides and very low, low tides
The sun and the moon work against each other to create minimal tides
b.
S E
M
Quarter Moon
or
M
ES
•These tides are calledneap tidesvery low, high tides andvery high, low tides
•Without the moon, the earth would still experience tides, but certainly not to the extent that we do with the moon’s influence.
4. Moonrise and Moonset
•Caused by therotation of the earth
•Occurs 50 minutes later each day because of the revolution of the moon