reasons for seasons (recap) - ucsbsiegel/geog3a/l04_g3a_011005.pdf · reasons for seasons (recap)...

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Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism Sphericity

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Page 1: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

Reasons for Seasons (recap)Revolution (around the sun)

Rotation (on its axis)

Earth’s Tilt

Axial parallelism

Sphericity

Page 2: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

The Earth’s tiltperpendicular to plane of

equator

Q: do these planes form great circles?

Page 3: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism
Page 4: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

Arctic Circle as viewed from above the plane of the ecliptic

Credit: www.physicalgeography.net

24 hrs day

24 hrs night

the parallel of the Arctic Circle is set by Earth’s tilt

Page 5: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

equinox June 21

the circle of illumination divides the earth equally into day and night halves - it forms a great circle-

note that 1/2 of earth is always in the light

Page 6: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

March of the Seasons

Page 7: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

earthyear.mov

Page 8: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism
Page 9: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

Earth’s Modern Atmosphere

Chapter 3

Page 10: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

note: relative size of atmosphere not to scale

The atmos-“spheres”

Page 11: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

How much atmosphere is there?

How thick is the atmosphere?The atmosphere is incredibly thin - if Earth were the size of a 12” globe, 99% of its atmosphere would be

about as thick as the paint on this globe!

the total mass of the atmosphere is 5.3x1018 kgBUT mass ocean = 1.4x1021 kg

& mass Earth = 6x1024 kg

The atmosphere is crucial to lifeanalogous to a cellular membrane, regulating

what can enter (such as filtering UV rays)

Page 12: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

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air is a mixture of nitrogen and

oxygen with some trace

gases

What is air?

average density of air is 1.3 kg/m3

Page 13: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

Evolution of the Atmospherethe present composition of the atmosphere represents

the net sum of many processes (biological and chemical) operating over 100’s of millions of years

if Earth were lifeless, its atmospheric composition

would be very different (for example, no oxygen)

Page 14: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

*Probable early atmosphere: CH4, H2, H2O, NH3

*Early Evolution H2 is lost H2O photochemically disassociates H2 is lost CH4 + O2 CO2 + H2O NH3 + O2 N2 + H2O CO2 reacts to form CaCO 3

*3.5 by: N2, CO2, H2O (mostly N2) Photosynthesis and oxygen Fe is oxidized, last banded iron

*2 by to present: evolution of the modern atmosphere

Earth’s atmosphere in the distant past

Page 15: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

Stomatapores on leafs

Troughton and Donaldson 1972

atmospheric oxygen (O2) is produced by photosynthesis

6CO2 + 12H2O C6H12O6 + 6H2O + 6O2light

CO2

O2

From World Book © 2002 World Book, Inc., 233 N. Michigan Avenue, Suite 2000, Chicago, IL 60601. All rights reserved. World Book illustration by James Teason

carbon dioxide + light => sugars + oxygen

phytoplankton in oceans

www.ekologija.net/ zajednicki/phytoplankton.jpg

Page 16: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

most atmospheric nitrogen (N2) is produced by volcanoes

Page 17: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

the other relatively abundant gas, argon (Ar), is inert (not reactive)

and not involved in biological processes

- produced by radioactive decay of 40K

atmospheric carbon dioxide (CO2) is produced and released by terrestrial photosynthesis and

respiration, as well as air-sea gas exchange

atmospheric water vapor (H2O) varies tremendously (from <1 - 4%

by volume) and is affected by evaporation and condensation

Page 18: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

air density decreases with height in the atmosphere because of gravity

Page 19: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

pressure decreases rapidly with altitude

Credit: http://www.physicalgeography.net

elevation of Mt. Everest

~30% of sea level

elevation where jets typically fly

~20% of sea level

average tropopause elevation

~10% of sea level

Page 20: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

the atmosphere has several layers

with distinct properties and

functions

think of these layers as

concentric shells orsphereswe can

characterize vertical profiles

according to three criteria

Page 21: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

Troposphere

StratosphereTropopause

over 99% of the atmosphere is contained in the troposphere and

stratosphere

Layers classified by temperature

Page 22: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

the tropopause elevation (and thus the thickness of the troposphere) varies with latitude

the tropical tropopause is twice as high as the polar tropopause because of vigorous

surface heating at low latitudes

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Page 23: Reasons for Seasons (recap) - UCSBsiegel/GEOG3A/L04_G3A_011005.pdf · Reasons for Seasons (recap) Revolution (around the sun) Rotation (on its axis) Earth’s Tilt Axial parallelism

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90% of atmospheric

mass ~5x10^18

kg

why does T decrease

with height in troposphere?

why does T increase with height in the stratosphere

?