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EARTH , SUN, and Moon Interactions
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EARTH , SUN, and Moon Interactions

Feb 23, 2016

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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? - PowerPoint PPT Presentation
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Page 1: EARTH  ,  SUN,  and Moon Interactions

EARTH , SUN, and Moon Interactions

Page 2: EARTH  ,  SUN,  and Moon Interactions

Understanding Climate and Weather

What? Why and How?

Page 3: EARTH  ,  SUN,  and Moon Interactions

Guide Questions 1.Why do we have night and day?

2.What is a day/year?

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

4.Why is it warmer at the equator and colder at the poles?

5.Why are there seasons?

Page 4: EARTH  ,  SUN,  and Moon Interactions

What causes Night and Day?

Page 5: EARTH  ,  SUN,  and Moon Interactions
Page 6: EARTH  ,  SUN,  and Moon Interactions

Length of Day:

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

Page 7: EARTH  ,  SUN,  and Moon Interactions

DAY AND YEAR

Page 8: EARTH  ,  SUN,  and Moon Interactions

DAY AND YEARRotation earth’s spinning on its axis

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

Revolution movement of earth

around the sun

Page 9: EARTH  ,  SUN,  and Moon Interactions

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

Page 10: EARTH  ,  SUN,  and Moon Interactions

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.

Page 11: EARTH  ,  SUN,  and Moon Interactions

Leap Years•When was the last leap

year?2008

•When is the next?2012

Page 12: EARTH  ,  SUN,  and Moon Interactions

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.

– MID LATITUDES: 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

Page 13: EARTH  ,  SUN,  and Moon Interactions

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)

Page 14: EARTH  ,  SUN,  and Moon Interactions
Page 15: 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

Page 16: EARTH  ,  SUN,  and Moon Interactions

http://www.youtube.com/watch?v=95TtXYjOEv49 mins

Geography basics

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Page 18: EARTH  ,  SUN,  and Moon Interactions

June Solstice

September Equinox

December Solstice

March Equinox

Sun

Page 19: EARTH  ,  SUN,  and Moon Interactions
Page 20: EARTH  ,  SUN,  and Moon Interactions

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.

Page 21: EARTH  ,  SUN,  and Moon Interactions

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

Page 22: EARTH  ,  SUN,  and Moon Interactions

SOLSTICE

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

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Page 24: EARTH  ,  SUN,  and Moon Interactions

Peralta Colleges, Physical Geography

Page 25: EARTH  ,  SUN,  and Moon Interactions

FACTORS THAT AFFECT CLIMATE

1.Axis or tilt of the Earth

2.Latitude

3.Elevation

4.Precipitation

5.Currents (wind, water)

Page 26: 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.

Page 27: EARTH  ,  SUN,  and Moon Interactions

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

Page 28: EARTH  ,  SUN,  and Moon Interactions

Latitude

Equator

Paris

48°

Page 29: EARTH  ,  SUN,  and Moon Interactions

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

Page 30: EARTH  ,  SUN,  and Moon Interactions

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

Page 31: EARTH  ,  SUN,  and Moon Interactions

Longitude

London

New York

Page 32: EARTH  ,  SUN,  and Moon Interactions

Time zones: Every 15˚, changes by 1 hour

TIME ZONES

Page 33: 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)

Page 34: EARTH  ,  SUN,  and Moon Interactions

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

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Peralta Colleges, Physical Geography

Page 36: EARTH  ,  SUN,  and Moon Interactions