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EARTH , SUN, and Moon Interactions. Understanding Climate and Weather What? Why and How?. Guide Questions . Why do we have night and day? What is a day/year? How does sunlight hit the Earth’s surface? (equator, poles) Why is it warmer at the equator and colder at the poles?

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EARTH , SUN, and Moon Interactions

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Earth sun and moon interactions

EARTH , SUN, andMoonInteractions


Earth sun and moon interactions

Understanding Climate and Weather

What?Why and How?


Earth sun and moon interactions

Guide Questions

  • Why do we have night and day?

  • What is a day/year?

  • How does sunlight hit the Earth’s surface? (equator, poles)

  • Why is it warmer at the equator and colder at the poles?

  • Why are there seasons?


Earth sun and moon interactions

What causes Night and Day?


Earth sun and moon interactions

Length of Day:

http://www.youtube.com/watch?v=dCyTNpcDTUM&feature=related


Earth sun and moon interactions

DAY AND YEAR


Earth sun and moon interactions

DAY AND YEAR

Rotationearth’s spinning on its axis

1,600 km/hr (rate of spin at any point along the equator)

Revolutionmovement of earth

around the sun


Leap year

Leap Year

  • It actually takes the Earth a little longer than a year to travel around the Sun — 365 days, 5 hours, 48 minutes, and 46 seconds, to be exact.

  • It was the ancient Egyptians who first figured out that the solar year and the man-made calendar year didn't always match up.

  • It was the Romans who first designated February 29 as leap day

  • That extra day was added to February because February used to be thelast month of the year

http://www.chiff.com/a/leap-year.htm


When do we have leap years

When do we have leap years?

  • a leap day happens in years only divisible by four, i.e., 1996, 2000, 2004

  • Another stipulation ruled that no year divisible by 100 would have a leap year, except if it was divisible by 400. Thus, 1900 was not a leap year ... but 2000 was! Go figure.


Leap years

Leap Years

  • When was the last leap year?

    2008

  • When is the next?

    2012


Number of daylight hours

Number of Daylight Hours

  • Every part of Earth gets about the same number of hours of daylight per year

    • half a year of full daylight

  • BUT, not received the same way

    • EQUATOR: it is delivered evenly -- exactly half a day, every single day, throughout the year.

    • POLES: it is delivered all at once -- half a year of daylight, and then half a year of darkness.

    • MIDLATITUDES: it is delivered in greater or lesser amounts, throughout the year -- some days having more than half a day of daylight, but others, half a year later, having less than half a day, and the average, throughout the year, being half a day of daylight per day


Amount of sunshine

AMOUNT OF SUNSHINE

  • However, although the different regions receive the same number of hours of daylight, they do NOT receive the same amount of sunshine

  • the amount of sunshine which is received over a certain amount of the ground depends upon how high the Sun is in the sky (the angle of the sun’s rays)


Earth sun and moon interactions

When sunlight shines from overhead (on left), one square foot of sunlight falls on one square foot of ground. When it shines at a shallow angle (on right), each square foot of sunlight spreads out over many feet of ground.

http://cseligman.com/text/sky/climate.htm


Earth sun and moon interactions

Geography basics

http://www.youtube.com/watch?v=95TtXYjOEv4

9 mins


Earth sun and moon interactions

March Equinox

June Solstice

December Solstice

Sun

September Equinox


Earth motions precession

Earth Motions: PRECESSION

  • Precession – Earth’s axis maintains approximately the same angle of tilt, but the direction in which the axis points continually changes.

  • Currently, the axis points toward Polaris.

  • In the year 14,000, it will point toward Vega.

  • By 28,000, it will point toward Polaris again.


Seasons

SEASONS

  • We have seasons because:

    • The Earth’s axis is tilted 23.5o, so different locations receive different amounts of direct sunlight throughout the year.

    • http://www.youtube.com/watch?v=000-3JYM0NI&feature=related


Solstice

SOLSTICE

http://members.shaw.ca/len92/geography.htm


Earth sun and moon interactions

Peralta Colleges, Physical Geography


Earth sun and moon interactions

FACTORS THAT AFFECT CLIMATE

  • Axis or tilt of the Earth

  • Latitude

  • Elevation

  • Precipitation

  • Currents (wind, water)


Earth sun and moon interactions

The latitude and longitude system

Longitude lines run north-south and meet at the North and South Poles; also called meridians.

Latitude lines run east-west and don't meet; also called parallels.


Latitude

Latitude

  • The latitude of a country is its angle above or below the equator.

  • For example

    • North Pole - 90° North

    • South Pole - 90° South

    • Paris, France - 48° North

    • Sydney, Australia - 34° South


Latitude1

Latitude

Paris

48°

Equator


Latitude2

Latitude

  • Some important lines of latitude include

    • The Equator – 0°

    • The Tropic of Cancer – 23.5° N

    • The Tropic of Capricorn – 23.5° S

    • The Arctic Circle – 66.5° N

    • The Antarctic Circle – 66.5° S


Longitude

Longitude

The longitude of a country is how far around the earth it lies from London.

For example

Manila - 120° East

New York - 74° West

The time zones follow lines of longitude that are every 15° away from London


Longitude1

Longitude

London

New York


Earth sun and moon interactions

TIME ZONES

Time zones: Every 15˚, changes by 1 hour


Earth sun and moon interactions

  • Climate change due to a country’s location

  • Latitude effect on seasonal change

  • day-light hours

  • precipitation levels (rainfall and snowfall)

  • average (and max, min) temperatures

  • crop growth

  • tourism

  • ecosystems

  • cultural changes due to climate differences (e.g. S.A.D also known as winter blues)


Earth sun and moon interactions

http://www.youtube.com/watch?v=5r3OufiIp5Y


Earth sun and moon interactions

Peralta Colleges, Physical Geography


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