13
s 1360 Planet Earth g Earth’s Hydrosphere metric height changes on rivers & lakes (with strong seasonal cycle & dependence on precip) metric height changes in oceans (Steric plus mass sea level change > climate predi tellite imaging of extent & thickness of sea ice (Arctic sea ice in a “new normal”; likely to be ice free in 5-15 years) osphere 13 October 2008 Read for Wed: 351-363

Honors 1360 Planet Earth Last time: Measuring Earth’s Hydrosphere Obs : Altimetric height changes on rivers & lakes (with strong seasonal cycle & dependence

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Honors 1360 Planet Earth

Last time:Measuring Earth’s Hydrosphere

Obs: Altimetric height changes on rivers & lakes (with strong seasonal cycle & dependence on precip)

Obs: Altimetric height changes in oceans (Steric plus mass sea level change > climate predictions!)

Obs: Satellite imaging of extent & thickness of sea ice (Arctic sea ice in a “new normal”; likely to be ice free in 5-15 years)

Today:• The Cryosphere

13 October 2008

Read for Wed: 351-363

Example IV: Satellite Gravity to Measure Mass Change:

Example IV: Satellite Gravity to Measure Mass Change:

The Cryosphere:

Frozen water at or near the Earth’s surface

Includes snow, alpine glaciers, ice caps (Greenland and Antarctica), sea ice (e.g. North Pole)

Earth is currently (past 12,000 to 15,000 years) in an interglacial period of a ~1.8 to 2.5 million year epoch of glaciation

Evidence for this in our back yard…

Pleistocene LakeBonneville Shorelines!

Deltaic Lake Deposits!

U-Shaped Glacial Valleys!

Cirques!

Moraines and Tills!

Pleistocene Ice Caps and Sea Level

From Surface Landforms (e.g., Moraines) & Sediment Record

Glacial Moraine on an Active Alpine Glacier, Swiss Alps

Also much wetter climate: Pleistocene Lakes evidencedby shoreline landforms,

salt flats.

Glacial-Interglacial Cycles Through Pliocene-Pleistocene

These are Natural cycles of climatic variation!

40,000–100,000 year cycles → Changes in Earth Insolation?

Milankovitch cycles: Variations in

(1) Eccentricity (“ellipticity”) of Earth orbit around the sun (T = 100,000 years)

(2) Obliquity (tilt of Earth’s spin axis relative to plane of orbit) (T = 41,000 years)

(3) Precession (changes in orientation of the spin axis) (T = 26,000 years)

The important factor: How much insolation does high latitude (particularly northern!) receive in summer?

Planetary orbits are ellipses with Sun at one focus:

Current Earth distance to Sun changes by ~3.4%Recall S = S0(R/R0)2

1.0342 = 1.069 (i.e. ~7% total change over a year!)

Min-Max distance varies between 0% to 12%

N

SJan 3Jul 4

Tilt of the Earth gives us seasons:

Precession determines what season in the year we are closest(Now, northern hemisphere has less insolation in summer,

more in winter, and a shorter winter than southern hemisphere)

• Glaciers form on continents• At latitudes 40-80º, very sensitive to seasonality • Right now, a very large fraction of continental area is in that range of northern hemisphere!