Potential Causes of Climate Change ENVS 110
Dec 19, 2015
planetary temperatures
100 1000 10000
Average D istance from Sun (10 6 km )
note logarithm ic scale !
-400
-200
0
200
400
600
Ave
rage
Pla
net
ary
Tem
pera
ture
(°C
)
M ercury
Venus
Earth
M ars
Jup ite r Saturn
U ranus N eptune
eccentricity:the influence of elliptical orbits
http://astroprofspage.com/archives/1024
Note: for the Earth this difference is quite small – about 3%
• changes in the shape of the earth’s orbit
• affects how solarradiation is distributedthroughout the year
http://www.homepage.montana.edu/~geol445/hyperglac/time1/milankov.htm
• axial tilt orobliquity
• determines howmuch sunlight reaches the northern and southern hemispheres during summer / winter
• influences the severity of the seasons
Milankovitch (over) simplified
• changes in orbital parameters change the way solar radiation is distributed across the earth
• it changes the absolute amount of solar radiation a little
(due to Kepler’s second law)
• so why don’t the effects just average out?
Important Greenhouse Gasses
Water vapor H2O 0.1 ppm – 40,000 ppm
Carbon Dioxide CO2 370 ppm
Methane CH4 1.7 ppm
Nitrous Oxide N2O 0.3 ppm
Ozone O3 0.01 ppm (at surface)
Freon – 11 CCl3F 0.00026 ppm
Freon – 12 CCCl2F2 0.0054 ppm
Data from Kump et al., 2004
The Greenhouse Effect
• Atmosphere transparent to visible light
• Atmosphere opaque to long wavelength radiation (infrared)
1600 1700 1800 1900 2000
Year
1363
1364
1365
1366
1367
mea
n a
nnua
l sol
ar ir
radi
ance
(W
/ m
2 )
data from :Lean, J.. 2004. Solar Irradiance Reconstruction.IG BP PAG ES/W orld Data Center for Paleoclim atology Data Contribution Series # 2004-035.NO AA/NG DC Paleoclim atology Program , Boulder CO , USA.
total solar irradiance 1610 - 2000
The Reverend Robert WalkerSkating on Duddingston Loch
attributed to Henry Raeburn, 1790's
Pieter Brueghel the Younger. Winter Landscape, 1621
little ice age
London Bridge Frost Fair Luke Clenell, 1814