Astronomical Control of Solar Radiation
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Transcript Astronomical Control of Solar Radiation
Climate Cooling
Proxy evidence
indicates an erratic
cooling
Over both poles
and mid latitudes
Roughly equal
cooling in first and
second half of
interval
Tectonic Scale Cooling Mechanism?
Lower volcanic CO2 emissions
Increased weathering
Increased ocean heat
transport
Tectonic changes
Atlantic widened and Pacific
narrowed
India and Australia
separated from Antarctica
India and Australia moved to
lower latitudes
India collided with Eurasia
Key oceanic gateways open
and closed
BLAG Hypothesis
Depends of global spreading
rates
55-15 mya general decrease
in spreading
Produce cooling
15 mya to today spreading
increased
Produce warming
Consistent with record prior
to 15 mya
Inconsistent with record
from 15 mya to present
Cannot alone explain cooling
Uplift Weathering Hypothesis
To explain cooling, 3 criteria must be met
High elevation terrain today must be
unusually large
High terrain must cause unusual amount of
rock fragmentation
Fragmentation and exposure must enhance
chemical weathering
Elevation on Earth
Most high elevation caused by subduction of
oceanic crust and volcanism
Mountain ranges associates with subduction
common throughout geologic time
Deep-seated heating and volcanism
East African plateau
• Mechanism of uplift not unique to last 55
my
Existence of uplifted terrains like the Tibetan
Plateau
Not common through geologic time
Conclude – amount of high elevation terrain is
unusually large during last 55 my
Physical Weathering High
Does the amount of
high elevation terrain
result in unusual
physical weathering?
Most likely given 10
fold increase of
sediment to the Indian
Ocean
Steep terrain along
southern Himalayan
margin
Presence of
powerful South
Asian monsoon
Chemical Weathering
Global chemical weathering rates difficult to
determine
Dissolved ions in rivers clue
Today concentration modified by human activity
Difficult to distinguish ions from hydrolysis and
dissolution
Only hydrolysis important on long term
Lots of rivers contribute ions to ocean
Chemical weathering rates in past very difficult to
quantify
Need chemical indicator of hydrolysis
Isotopes of strontium and osmium
Strontium Isotopes
87Sr/86Sr
for carbonate rocks
has been measured throughout
the Phanerozoic
Curve reflects relative
contributions of Sr to the
ocean
Continental weathering
Hydrothermal activity along
mid-oceanic ridges
General decrease in Early
Phanerozoic due to increasing
activity along mid-ocean ridges
Late Cenozoic increase in 87Sr
due to increased rates of
continental weathering by
glaciation
87Sr/86Sr
& Chemical Weathering
Increase in 87Sr/86Sr in
Cenozoic could be
Increase in chemical
weathering
Delivers more Sr and
more radiogenic Sr to
ocean
Rock type being
weathered is more
radiogenic
No change in rate of
chemical weathering
No unique solution
Osmium Isotopes
Radiogenic Os formed from Re
Re enriched in certain phases
Organic-rich shales
Weathering of organic-rich shales
Certain minerals in granitic rocks
Hydrolysis reactions!
Os residence time in ocean short
Rivers draining the Himalayans not particularly rich
in Os nor in radiogenic Os
Available evidence indicates Himalayans not a
source for strongly radiogenic osmium
Infer Chemical Weathering Rates
Tibetan-Himalayan complex very large and at high
elevation
Steep slopes receive lots of rainfall
Heavy rains produce high suspended load
Probably also provide high dissolved load
BLAG or Uplift Weathering?
No “proof” of either hypothesis exists
BLAG explains well cooling from 55-15 mya
Uplift weathering supported by conditions
in Tibetan-Himalayan Complex
Would a combination of the two hypotheses
explain best global cooling over last 55 my?
Did Himalayan uplift balance increased CO2
from enhanced spreading?
Ocean Heat Transport
Although it appears “cool tropics paradox” is
resolved
Several important tectonic events influenced
oceanic circulation
Opening or closing of critical gateways
Narrow passages linking major ocean basins
Change heat and salt balance
Two critical gateways
Opening of Drake Passage producing the
Antarctic Circumpolar Current
Appearance of the Isthmus of Panama stopped
equatorial flow between Atlantic and Pacific
Opening of Drake Passage
Opening the gap
between South America
and Antarctica 25-20
mya allowed start of
ACC
Prior to opening, flow
from north kept
Antarctica warm
Onset of ACC
proposed to initiate
glaciations on
Antarctica
Timing of Opening
Drake Passage opened 25-20 mya
Glaciations on Antarctica began 35 mya
Most intense glaciation 13 mya
Ocean GCM models
Indicate that opening of Drake Passage
had no effect on ocean/atmosphere
temperatures
Antarctica cold with or without ACC
Models crude
Smaller grid
Affect of ACC on other deep currents
Isthmus of Panama
Closure within last 10 my
Complete closure 4 mya
N. America glaciations 2.7 mya
Stopped westward flow of warm salty water
Redirecting flow in Atlantic into Gulf
Stream
Northward flow of salty water slow sea ice
formation
Reduced sea-ice cover made more moisture
available on land
Triggered growth of ice sheets
Results of Closure
Ocean GCM model results
Agree with redirection of west
flowing warm saline water into
Gulf Stream
Also stops return flow of low
salinity water into Atlantic from
Pacific
Further increase salinity of
Gulf Stream
GCM model predicts reduction in
sea ice in N. Atlantic
Did not affect atmospheric
moisture
However, warmed N. Atlantic
and increased summer
melting of snow and ice
Assessment of Gateway Changes
Illustrates fundamental disagreement
Stopping pole-ward flow enhanced glaciations
Starting pole-ward flow enhanced glaciations
Argument centers about role of latent heat
Warmer ocean releases more latent heat to
atmosphere
Supply moisture in atmosphere for ice sheet
growth
Appears that more sensible heat transferred
Promote melting and ablation of glacial ice
Ablation of glacial ice important
Importance of Gateways
Not satisfactory explanation for long-term
global temperature changes
Discrete events that affected circulation
One-time events cannot explain well
long-term temperature changes
Clearly affect circulation patterns
Closure of Isthmus of Panama
Increased rate of NADW formation
• Redirected dense water to north
– Easier to form bottom water
Brief Tectonic-Scale Change
Attempt to explain erratic nature of cooling
Volcanic aerosols
Formation of sulfuric acid droplets or
particles
Sulfate aerosols block incoming solar
radiation when in stratosphere
Burial of organic carbon
Brief intervals of enhanced burial
Reduction in atmospheric CO2
Earth’s Active Volcanoes
Most volcanoes associated with subduction
andesitic and relatively explosive
Explosive eruptions between 23.5°N and 23.5°S
have most effect on climate
Sulfate Aerosols
Aerosols that reach
stratosphere
Attain maximum
concentration within
months of eruption
Concentrations
decline
exponentially as
particles settle
Cooling effect follows
concentration
Documentation of Effect
Effect of sulfate aerosols difficult to
detect in geologic record
Crater size
Volume of volcanic ash deposits
Geographic area of ash fall deposit
Caveat is that sulfur content ash
content
Ice core records show ash deposits and a
record of sulfuric acid
Limited time resolution
Size of effect
Even massive eruptions that send sulfate
aerosols into stratosphere
Produce cooling for only a few years
Multiple eruptions required for significant
long-term cooling
Multiple large eruptions unlikely
Global cooling countered by increased CO2
Volcanic eruption also a source for CO2
CO2 residence time in atmosphere higher
Burial of Organic Matter
Changes in the rate of burial of organic
matter affect atmospheric CO2
Rate of burial of marine organic matter
sensitive to:
Changes in rates of production
Nutrient supply
• Change in upwelling
• Change in delivery of nutrients from
land
Changes in mode of preservation
Bottom water oxygenation
Cooling 13 mya
Organic carbon-rich sediments deposited
along California coast 13 mya
Coincided with global cooling
Strong winds enhanced upwelling
• Termed the Monterey Hypothesis
Timing of maximum organic carbon burial
lags maximum cooling rate by 3 my
Coastal deposition of organic-rich sediments
May be exposed during sea-level low stand
Organic matter oxidized, CO2 released
Future Research Directions
What is needed to better resolve
mechanisms underlying tectonic-scale
changes?
Detailed record of atmospheric CO2
Geochemical tracer for chemical
weathering
Better understanding of feedbacks in
climate system
More detailed ocean general circulation
models