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Transcript
Daniel Fischbach
Physics 203-001 – Earth In Space
6/22/17
Created on: 10/27/04
Topic: Climate
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Weather is study of short term changes in the atmosphere (seconds to days)
Meteorology – study of weather
Climate is study of long term changes in the atmosphere (decades to millions of years)
Climatology – study of climate
Climate = Temperature and precipitation
Equatorial latitudes are hot and polar latitudes are cold (smallest temperature ranges) while
mid latitudes go through the seasons (biggest temperature ranges, because of seasons)
Daily temperature mean (average)
o Mean = (High + Low) / 2
o Monthly temperature mean: Average of the averages
o Yearly temperature mean: Average of the averages of the averages
Daily temperature range (difference)
o Range = High – Low
o Monthly temperature range: Difference of the highest mean and lowest mean (days)
o Yearly temperature range: Difference of the highest mean and lowest mean (months)
Earth moves about 1 million miles to/from the Sun per year because of the orbit
Earth is 93 million miles from the Sun
Earth is closest to the sun in winter and farthest from the sun during summer
Tilt of the earth causes the seasons
/ is the direction of the tilt
NH is tilted most toward the Sun – longest day of the year and shortest night (Summer
Solstice – June 21st)
NH is tilted most away from the sun – longest night of the year and shortest day (Winter
Solstice – December 21st)
Day and night are =
o Autumnal Equinox – September 21st
o Vernal Equinox – March 21st
Temperature ranges in the SH are small compared to the NH
Mild winters and summers in the SH because of the amount of water
Severe ice age every 100,000 years or so
o Severe ice age is explained by orbit – orbit changes every 100,000 to an ellipse
o Earth’s climate is between Ice Ages
Minor ice age every 25,000-50,000 years
Caused by changes in Earth’s tilt and orbit around the Sun (Milankovitch theory of
intermediate timescale changes in climate)
The Earth does 3 things:
o Rotates – spinning around an axis
o Precesses – spinning of an axis around another axis (\| | |/ | \| )
 26,000 years to precess once
 The North Star changes with axis rotation
o Nutates – hopping of the axis
 41,000 years to nutate once (could cause climate changes)
148071321
Instructor: Libarid A. Maljian
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