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Earth

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Chapter 25 Earth s Motions Rotation The spin of the Earth on its axis (rate of 15 /hr) Earth is tilted at an angle of 23.5 from perpendicular (90 ) . – PowerPoint PPT presentation

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Title: Earth


1
Chapter 25
  • Earths Motions

2
Rotation
  • The spin of the Earth on its axis (rate of
    15º/hr)
  • Earth is tilted at an angle of 23.5º from
    perpendicular (90º) . In other words, the tilt
    of the Earths axis is 23.5º off of the 90º it
    should be if it had a perpendicular tilt.
  • The Earths axis is always tilted in the same
    direction throughout its orbit (parallelism)

3
Remember, the ecliptic is the plane of the path
that the Earth takes around the Sun
4
Evidence of Movement
  • Foucault Pendulum- Changes its direction of swing
    over time
  • Coriolis Effect- The deflection of air and
    water to their right in the northern hemisphere
  • Sorry, Bart Simpson was incorrect. Water DOES
    deflect counterclockwise in the Northern
    Hemisphere and clockwise in the Southern
    Hemisphere, HOWEVER in toilets, the direction is
    caused by the force of the pump and direction it
    pumps the water in, not the CORIOLIS force!
  • In fact, YOU can determine the direction that
    water goes down the tub drain if you turn your
    hand in the water around the drain and spin the
    water either CW or CCW as it is draining out of
    the tub!!! Try it!!!!!

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6
Object moves to ITS LEFT
Object moves to ITS RIGHT
7
Solar Time
  • The measurement of time based on the apparent
    movement of the sun through the sky
  • Solar Noon is the time of day when the sun is at
    its highest altitude above the horizon.
    (Wherever the Sun Peaks in the sky)
  • Problem - solar noon does not occur at the same
    time for everyone (solar noon differs by approx.
    1 minute for every 12 miles east/west of a
    specific location)

8
  • To make up for this problem, time zones were
    established (each 15º longitude wide 1 hour of
    rotation)
  • Time zones begin at the Prime Meridian
  • Every 15 degrees EAST is 1 hour, every 15
    degrees WEST is 1 hour
  • Clock time is the average solar time

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10
Revolution
  • Movement of the Earth around the sun in its
    elliptical orbit
  • One complete revolution is 365.25 days (1 year)
  • In conjunction with AXIAL TILT, this causes a
    change in the seasons
  • If there was no tilt of the axis no seasonal
    changes
  • Evidence of movement Change in visible
    constellations throughout the year

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Solstices and Equinoxes
  • SOLSTICE extreme differences in daylight vs.
    darkness. The following values are applicable to
    the NORTHERN HEMISPHERE ONLY. REVERSE THESE
    VALUES FOR THE SOUTHERN HEMISPHERE
  • SUMMER 6/21/05 16 hours daylight/8 hrs
    darkness. The Sun is directly above the Tropic
    of Cancer. (23.5º N)
  • WINTER 12/21/05 8 hours daylight/16 hrs
    darkness. The Sun is directly above the Tropic
    of Capricorn. (23.5º S)
  • EQUINOX equal distances from the sun (equal
    daylight and darkness)
  • Autumn (Autumnal) 9/23/05, Spring (Vernal)
    (Verde/Vern means green) 3/20/05 12 hours
    daylight and 12 hours of darkness FOR THE ENTIRE
    EARTH NORTHERN AND SOUTHERN HEMISPHERES. The
    Sun is directly above the Equator.

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16
Nighttime on the Artic Circle during the Summer.
The sun never sets! It only gets as low as the
horizon and as high as it looks about an hour
before sunset!!!
17
The Suns Apparent Path Across the Sky
  • Because of the tilt of the Earth and the
    Revolution of the Earth around the Sun, the Sun
    appears to rise and set each day in a slightly
    different place on the horizon.
  • Also, Solar Noon (the highest point the Sun
    reaches in the sky) also varies slightly each
    day.
  • These are predictable apparent motions and are
    easiest to pick out on the Solstices and
    Equinoxes.

18
Suns Apparent Path from a Viewpoint in NYS
December 21
June 21
March 21 September 21
19
Solar Noon at The Equator
20
Causes of Seasons
  1. Earths revolution around the sun
  2. Tilt of the Earth on its axis
  3. Parallelism of the axis
  4. More daylight hours more insolation warmer
    time of year
  5. Less daylight hours less insolation cooler
    time of year
  6. Suns rays are more direct (perpendicular) to the
    Earths Surface in the Northern Hemisphere during
    our summer

21
Causes of Seasons
  • 6 explains why even though the Sun shines for 24
    hours a day for nearly 6 months a year at the
    North and South Poles, the temperature never gets
    above freezing!!!!
  • If the Suns rays dont hit the Earth at a
    perpendicular or near perpendicular angle, they
    arent all that powerful and warming!!!!

22
Direct solar rays
Less direct solar rays
23
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