The earthundergoes one complete rotation along
its axis in 24 hours.
For one complete rotation, the earth passes
through 360 degrees of longitude.
For every one-hour time, a point on the earth
moves through 15 degrees of longitude (360/24
hours = 15o
).
For every 4 minutes, a point on the earth passes
through 1 degree of longitude
4.
The earthrotates in an anti-clockwise direction
(From West to East).
Places on the East side of a given point on the earth
are ahead of time while those to the West side of
the same point always lag behind in time.
The most important result of the earth's rotation is the
daily pattern of DAYS and NIGHTS
7.
In 1878,Canadian Sir Sanford Fleming suggested a
system of worldwide time zones.
Fleming proposed that the globe be divided into 24
time zones, each 15 degrees of longitude in width.
Railroad companies in Canada and the United States
began using Fleming's time zones in 1883.
In 1884, an International Prime Meridian Conference in
Washington D.C. accepted it.
Each newcalendar day begins at midnight on the
International Date Line (Longitude 180o
).
Crossing the date line causes adjustments to clocks &
dates.
Traveling from West toward East (Hawaii to Japan)
one jumps into a new day on crossing the Date line.
From East towards West (Japan to Hawaii), one
looses a day after crossing the line
10.
The Impositionof Day/Night rhythm
The redirection of the flow paths of both air and
water that flows over the earth’s surface.
◦ Flows in the Northern Hemisphere – Right
◦ Flows in the Southern Hemisphere - Left
Rise and fall in Tidal Waves over the oceans.
11.
The earthrevolves around the Sun on its own
ORBIT (oval-shaped path).
Perihelion: A point on the orbit where the earth
is closest to the sun - January 3rd
Aphelion: A point where the sun is farthest away
from the SUN - July 4th.
On its orbit round the sun, the earth moves
through a plane called the PLANE OF THE
ECLIPTIC.
13.
The earth'saxis is inclined to the orbit at an angle of
23.50
Inclination of the earth’s axis during the movement
round the Sun results in the following:
1. different positions of the noon Sun
2. different positions of Sun rise and sun set
3. different length of days & nights in a year
4. different shadow lengths during the seasons
14.
March 21is Spring Equinox and…
September 21 is Autumnal Equinox.
On these days, the noon Sun is points directly on the
equator so…
ALL PLACES on the earth’s surface receive
approximately 12 hours of daylight and 12 hours of
darkness.
June 21st
(Summer
Solstice)
Places in the Arctic circle
points directly toward the
sun so the Northern
Hemisphere receive more
sunlight (hence longer days
and shorter nights)
On this day, places in the
Southern Hemisphere
receive less sunlight (so
shorter days and longer
nights).
17.
In summerthe earth’s axis lean toward the sun so the
energy we receive from the sun is more direct
The sun also remains in the sky for longer periods and
as such the earth’s surface absorbs more solar energy
The high temperatures produce summer conditions.
18.
December 21st
(Winter
Solstice)
On this day, the Sun moves
into the Southern
Hemisphere and places
there receive more
sunlight and experience
longer days and shorter
nights.
The Northern
hemisphere receive less
sunlight (so shorter days
and longer nights).
19.
Because theearth’s axis point to the same direction
toward the North Star, the Northern hemisphere
leans back on the Sun during winter
The Sun is lower in the sky and its energy is more
widely distributed
The Sun is also visible for a much shorter time giving
off little energy so temperature goes down producing
winter conditions