|
|
|
Changes in solar heating driven by changes in
Earth’s orbit are the major cause of cyclic climate changes over time
scales of tens to hundreds of thousands of years (23k years, 41k years, and
100k years) . |
|
Earth’s orbit and its cyclic variations: tilt
variations, eccentricity variations, and precession of the orbit. |
|
How do orbital variations drive the strength of
tropical monsoons? |
|
How do orbital variations control the size of
northern hemisphere ice sheets? |
|
What controls orbital-scale fluctuations of
atmospheric greenhouse gases? |
|
What is the origin of the 100,000-year climate
cycle of the last 0.9 Myr (ice sheets melt rapidly every 100,000 years)? |
|
|
|
|
First, Earth spins around on its axis once every
day è The Tilt. |
|
Second,
Earth revolves around the Sun once a year è The
shape of the Orbit. |
|
Both the tilt and the shape of the orbit have
changed over time and produce three types of orbital variations: |
|
(1)
obliquity variations |
|
(2)
eccentricity variations |
|
(3)
precession of the spin axis. |
|
|
|
|
|
|
Variations in the eccentricity of the orbit cause changes in the annually averaged
amount of sunlight hitting Earth. |
|
Variations in the tilt (obliquity variations and
the precession of the tilt) do not affect the averaged amount of solar
radiation to the Earth. |
|
The tilt variations affect seasons. |
|
|
|
|
At present-day, the axis is tilted at an angle
of 23.5°, referred to as Earth’s “obliquity”, or “tilt”. |
|
The Sun moves back and forth through the year
between 23.5°N and 23.5°S. |
|
Earth’s 23.5° tilt also defines the 66.5°
latitude of the Artic and Antarctic circles. No sunlight reaches latitudes
higher than this in winter day. |
|
The tilt produces seasons!! |
|
|
|
|
Assume the Earth has a perfectly circular orbit
around the Sun. |
|
With no tilt, incoming solar radiation is always
directed straight at the equator throughout the year. |
|
With no tilt, no seasonal changes occur in solar
radiation received at any latitude. |
|
As a result, solstices and equinoxes do not even
exit è NO SEASONS! |
|
|
|
|
|
|
Earth’s orbit is not a perfect circle: it has a
slightly eccentric or elliptical shape. |
|
This noncircular shape is the result of the
gravitational pull on Earth from the Sun, the moon, other planets and their
moons. |
|
The distance to the Sun changes with Earth’s
position in its orbit. |
|
This changing distance has a direct effect on
the amount of solar energy Earth receives. |
|
|
|
|
The position in which the Earth is closest to
the Sun is called “perihelion”. |
|
Perihelion means “near the Sun” in Greek. |
|
The position in which the Earth is farthest to
the Sun is called “aphelion”. |
|
Aphelion means “away from the Sun” in Greek. |
|
|
|
|
Seasons |
|
Solstices: mark the longest and shortest days of the years (June 21
and December 21 in the northern hemisphere, the reverse in the southern) |
|
Equinoxes: the length of night and day become equal in each
hemisphere. |
|
At the present-day orbit, the winter and summer
solstices differ from the aphelion and perihelion by about 13 days. |
|
|
|
|
The seasonal temperature contrast is referred to
the range of temperature extremes between summer and winter. |
|
The combination of an eccentric orbit and a
tilted spin axis means that the seasonal temperature contrast is different
in the Southern and Northern Hemispheres. |
|
The Southern Hemisphere experiences a larger
seasonal temperature contrast than the Northern Hemisphere. |
|
|
|
|
Over time, the tilt angle varies in a narrow
range (22.2° ~ 24.5°). |
|
These variations are caused by the gravitational
tug of large planets, such as Jupiter. |
|
The present-day value of the tile is decreasing. |
|
Cyclic changes in the tilt angle occur at a
period of 41,000 years. |
|
Changes in tilt cause long-term variations in
seasonal solar insolation received on Earth. |
|
The main effect of tilt changes is to amplify or
suppress the seasons: increase tilt amplifies seasonal differences,
decreased tilt reduces them. |
|
|
|
|
|
The degree to which the orbit is elliptical is
called the eccentricity. |
|
The eccentricity is defined as the ratio of the
distance between the center of the ellipse to either focus to the distance
from the center to the edge of the ellipse along the major axis. |
|
The smaller the eccentricity, the more circular
the ellipse is. |
|
|
|
|
|
|
Today’s eccentricity is 0.0167, lies well toward
the lower end of the variation range of Earth’s eccentricity (closer to
circular). |
|
The long-term variations in orbital eccentricity
are concentrated at two periods: 100,000 years and 413,000 years. |
|
The eccentricity variations differ from the
other two orbital variations (obliquity variations and the precessional
variations) in one important aspect: Eccentricity variations cause changes
in the annually averaged amount of sunlight hitting Earth. |
|
|
|
|
There are two kinds of precession: (1) the
precession of the spin axis and (2) the precession of the ellipse. |
|
Earth’s wobbling motion is called the axial
precession. It is caused by the
gravitational pull of the Sun and Moon. |
|
Axial precession is a slow turning of Earth’s
axis of rotation through a circular path, with a full turn every 25,700
years. |
|
|
|
|
The precession of the ellipse is known as the
elliptical shape of Earth’s orbit rotates itself at a slower rate than the
wobbling motion of the axial precession. |
|
|
|
|
The combined effects of these two precessions
cause the solstices and equinoxes to move around Earth’s orbit, completing
one full 360° orbit around the Sun every 23,000 years. |
|
|
|
|
Small variations in received insolation do occur
in connection with Earth’s eccentric orbit about the Sun, but these appear
only as changes in the total energy received by the entire Earth, not
as seasonal variations. |
|
Compared to the changes in seasonal insolation
of 10% or more that occur at the tilt and precession cycles, these annual
eccentricity changes are smaller by a factor of 50 or more. |
|
|
|
|
The hemispheric and seasonal patterns of
insolation changes for tilt and precession are fundamentally different. |
|
Insolation changes at high latitudes caused by
change in the tilt are in phase between the hemisphere from a seasonal
perspective. |
|
For the case of increased tilt, summer
insolation maxima in the northern hemisphere occur at the same time in the
41,000-year cycle as summer insolation maxima in the southern hemisphere. |
|
|
|
|
For the precessional changes that dominant low
and middle latitudes, the relative sense phasing between seasons and
between hemispheres is exactly reversed from of tilt. |
|
The Earth-Sun distance is the major control on
precessional changes in insolation. |
|
A precessional-cycle insolation maximum
occurring at June 21 (or December 21) will be simultaneous everywhere on
the Earth, a summer season in one hemisphere and a winter season in another
hemisphere. |
|
|
|
|
|
|
The 23,000-year cycle of precissional change
dominants the insolation changes at low and middle latitudes. |
|
The 41,000-year cycle of tilt change dominants
the insolation changes at higher latitudes. |
|
Eccentricity changes (the 1000,000 or
413,000-year cycles) is not a significant influence on seasonal insolation
chanes. |
|
|
|
|
What controls the size of Ice Sheets in the
Northern Hemisphere? |
|
è The
summer insolation (The Milankovitch Theory). |
|
|
|
|
Milankovitch suggested that the critical factor
for Northern Hemisphere continental glaciation was the amount of summertime
insolation at high northern latitudes. |
|
Low summer insolation occurs during times when
Earth’s orbital tilt is small. |
|
Low summer insolation also results from the fact
that the northern hemisphere’s summer solstice occurs when Earth is
farthest from the Sun and when the orbit is highly eccentric. |
|
|
|
|
Continental ice sheets exist because the overall
rate at which snow and ice accumulates equals or exceeds the overall rate
of ice loss or ablation. |
|
Temperature is the main factor that determine
whether ice sheets are in a regime of net ablation (negative mass balance)
or net accumulation (positive mass balance). |
|
The boundary between the upper area of positive
mass balance and the lower area of net loss of ice mass is called the equilibrium
line. |
|
|
|
|
Continental ice sheets exist because the overall
rate at which snow and ice accumulates equals or exceeds the overall rate
of ice loss or ablation. |
|
It is the summer insolation that determines the ice sheets grow and
shrink. |
|
Low (cold) summer insolation is the critical
factor that cools the climate enough to allow snow and ice to persist from
one winter to the next. |
|
Winter insolation is not important to ice sheet
sizes, because (1) the temperatures are always cold in winter and (2) the
Sun at high latitudes are low in the sky, regardless of ongoing orbital
changes. |
|
|
|
|
The Milankovitch theory proposes that high
summer isolation results in net melting of ice sheets, while low summer
insolation results in net accumulation of ice sheets. |
|
|
|
|
(1) Insolation control of ice sheet size |
|
(2) Initial lag of ice volume behind insolation |
|
(3) Subsequent lag of bedrock depression and
rebound behind ice sheet growth and decay |
|
|
|
|
During high summer insolation, the equilibrium
line is driven north. The continents lie in a regime of net albation. |
|
During low summer insolation, the equilibrium
line is driven south. The continents lie in a regime of net accumulation. |
|
|
|
|
Under the most favorable condition (ice
accumulates 0.3 meters each year), a full-size ice sheet 3000 meters thick
would take 10,000 years to form. |
|
At the 41,000-year cycle of orbital tilt, ice
sheets lag behind changes in summer insolation by about 10,000 years. |
|
At the 23,000-year cycle of orbital precession,
ice sheet lags behind summer insolation by about 6,000 years. |
|
The lag times are both about one quarter of the
periods of the cycles. |
|
|
|
|
As ice sheets grow, the pressure of their weight
on the underlyingion bedrock becomes significant. |
|
Due to the different densities of ice and rock,
a ice sheet of 3000m thickness is roughly equivalent to the weight of 1000m
of solid rock. |
|
The initial sinking would be elastic and
immediate. |
|
The bedrock later respond more slowly and sinks
half of the remaining distance toward the eventual equilibrium every 3000
years. |
|
The total time to reach the final depression
depth is about 15,000 years. |
|
|
|
|
A full cycle of ice sheet growth and decay
incorporates both the delayed response of the ice sheets to summer
insolation forcing as well as the delayed response of bedrock to the ice
sheet load. |
|
As a results of the delays, the maximum size of
ice sheets does not happen at the time of the lowest summer insolation. |
|
|
|
|
The long-term evolution of ice sheets reflects
the interaction of two factors: changes in summer insolation that drive
shorter-term changes in ice sheet mass balance and a much more gradual
global cooling represented by a slowly changing glaciation threshold. |
|
Ice sheets accumulate when summer insolation
falls below a critical glaciation threshold and melt when it rises above
it. |
|
|
|
|
|
This figures shows a North Atlantic Ocean
sediment core holds a 3 Myr d18O record of ice volume and
deep-water temperature changes. |
|
There were no major ice sheets before 2.75 Myr
ago. |
|
After that, small ice sheets grew and melted at
cycles of 41,000 and 23,000 years until 0.9 Myr ago. |
|
After 0.9 Myr ago, large ice sheet grew and
melted at a cycle of 100,000 years. |
|
|
|
|
A closer look of the last 150,000 years of the d18O
record shows 23,000-year and 41,000-year cycles. |
|
|
|
|
|
|
Methane (CH4) levels have fluctuated mainly at
the 23,000-year orbit rthym of precession. |
|
è These
changes may be linked to fluctuations in the strength of monsoon in
Southeast Asia. |
|
During glaciations, atmospheric CO2 values have
repeatedly dropped by 30% from the levels typical of warm interglaciations. |
|
è Most of
the explanation for lower glacial CO2 appears to be tied to a transfer of
carbon into the deep ocean. |
|
WHY? |
|
|
|
|
Air moves freely through snow and ice in the
upper 15 m of an ice sheet. |
|
Flow is increasingly restricted below this
level. |
|
Bubbles of old air are eventually sealed off
completely in ice 50 to 100 m below the surface. |
|
|
|
|
The best place on an ice sheet to take ice cores
is at the top. |
|
Ice cores can be dated by counting annually
deposited layer (or ice flow model). |
|
Annual layering is recorded in several
properties of ice cores, the most obvious of which are layers of dust
easily visible to the eye. |
|
Dust is usually deposited at the end of cold,
dry windy winters. |
|
One of the most famous ice core drilling is at a
site high on the Antarctic ice sheet, which is called the Vostok ice
record. |
|
|
|
|
|
|
|
The Vostok ice record shows a series of cyclic
variations in methane concentration, ranging between 350 to 700 ppb (part
per billion). |
|
Each Ch4 cycle takes about 23,000 years. |
|
This cycle length points to a likely connection
with changes in orbital procession. |
|
The orbital procession dominates insolation
changes at lower latitudes. |
|
|
|
|
|
|
On the 23,000-year cycle, methane variations
closely resemble the variations of monsoon strength. |
|
The peak values of methane match the expected
peaks in monsoon intensity not only in timing but also in amplitude. |
|
This match suggests a close connection between
CH4 concentrations and the monsoon on the 23,000-year climate cycle. |
|
By why? |
|
|
|
|
Monsoon circulations exit on Earth because the
land responds to seasonal changes in solar radiation more quickly than does
the ocean. |
|
Changes in insolation over orbital time scales
have driven major changes in the strength of the summer monsoons. |
|
Changes of 12% in the amount of insolation
received at low latitudes have caused large changes in heating of tropical
landmass and in the strength of summer monsoons at a cycle near 23,000 years in length. |
|
|
|
|
The 23,000-year cycle of orbital procession
increases (decreases) summer insolation and at the same time decreases
(increases) winter insolation at low and middle latitudes. |
|
Departures from the modern seasonal cycle of
solar radiation have driven stronger monsoon circulation in the past. |
|
Greater summer radiation intensified the wet
summer monsoon. |
|
Decreased winter insolation intensified the dry
winter monsoon. |
|
|
|
|
Orbital procession affects solar radiation at
low latitudes |
|
è solar
radiation affects the strength of low-latitude monsoons |
|
è monsoon
fluctuations changes the precipitation amounts in Southeast Asia |
|
è heavy
rainfalls increase the amount of standing water in bogs |
|
è decaying
vegetation used up any oxygen in the water and creates the oxygen-free
conditions needed to generate methane |
|
è the
extent of these boggy area must have expanded during wet monsoon maxima and
shrunk during dry monsoon minima. |
|
|
|
|
The longest orbital-scale record of CO2 changes
comes from the Vostok ice core drilling site. |
|
The CO2 record shows a series of regular
oscillation between CO2 values as high as 280-300 ppm and as low as 180-190
ppm over the last 400,000 years. |
|
Values at the high end of this range occur
within the present interglacial interval. |
|
These relative high CO2 values lasted for
several thousand years before the abrupt increase after 1800. |
|
The dominant period of CO2 variations is about
100,000 years. |
|
|
|
|
We have learned that the dominant cycle of ice
sheet variations over the last several hundred years has also been 100,000
years. |
|
This suggests that the 100,000-year variations
in atmospheric CO2 match those of ice sheets. |
|
Over the 400,000-year length of the ice core
record, the major cycles of CO2 change line up well with the ice volume
changes (indicated by d18O). |
|
The two signals share not only the 100,000-year
cycle but also its asymmetric shape: abrupt increases in CO2 during times
of rapid ice melting (i.e., warming) and slower decreases during times of
slower phases of ice volume buildup (cooling). |
|
WHY? |
|
|
|
|
How could CO2 vary by 30% or more over orbital
time scale? |
|
What factors can explain the observed 90-ppm dip
in CO2 level during glacial intervals from the levels observed in
interglacial intervals? |
|
|
|
|
Changes in the physical oceanographic
characteristics of the surface ocean – its temperature and salinity –
during glaciations might alter the chemical solubility of Co2. |
|
Because CO2 dissolves more readily in colder
seawater, atmospheric CO2 will drop by 9 ppm for each 1°C of ocean cooling. |
|
Because CO2 dissolves more easily in seawater
with a lower salinity, saltier glacial seawater will increase atmospheric
CO2 level. |
|
The effects of seawater temperature and salinity
work against each other! |
|
The net effect of the physical oceanographic
influences on atmospheric CO2 is to decrease CO2 by 11 ppm during
glaciations. |
|
This process only explains 10% of the CO2
changes on orbital scales. |
|
|
|
|
The large changes in atmospheric CO2 over
intervals of a few thousand years must involve rapid exchanges (compared to
the rate of exchange between the atmosphere and rock) among: the
atmosphere, vegetation and soil, surface and deep ocean. |
|
Not vegetation and soil: because vegetation
reduced during glaciations. |
|
Not surface ocean: because surface ocean
exchanges CO2 quickly (in a few years) with the atmosphere. |
|
The glacial carbon removed from the atmosphere,
from the vegetation, and from the surface ocean must have been stored in
the deep ocean. |
|
Carbon was exported to the deep ocean by higher
rates of photosynthesis and biological productivity. |
|
|
|
|
Carbon was exported from surface oceans to the
deep ocean during glaciations by higher rates of photosynthesis and
biological productivity. |
|
Photosynthesis and organic productivity occur in
the surface ocean because of sunlight and nutrients. |
|
Photosynthesis extracts CO2 from surface waters
and incorporates it in organic tissue (CH2O), some of which sinks to the
deep ocean. |
|
|
|
|
The pumping hypothesis asserts that greater
downward removal of carbon occurs because more nutrients become available
to stimulate greater removal of organic carbon from surface water by
photosynthesis. |
|
Large-scale changes in biological pumping of
carbon to the deep sea can occu only in relatively productive regions. |
|
The most productive regions in the world ocean
are in areas of upwelling along costal margins and near the equator and in
the high-latitude surface ocean around Antarctica. |
|
These are the two regions where significant more
organic carbon could have been pumped down into the deep ocean during
glaciations than today. |
|
|
|
|
|
|
Increased Upwelling |
|
Stronger glacial winds |
|
greater wind-driven upwelling of nutrient-rich
water along coast and near equator. |
|
Increased Nutrient Levels By Iron Fertilization |
|
Stronger glacial winds |
|
Dust rich in iron is blow to the ocean from arid
continental interiors |
|
Ions fertilize the surface ocean and stimulate
greater glacial photosynthesis and productivity. |
|
This fertilization effect stimulates the
productivity in mid-ocean regions far from costal upwelling. |
|
|
|
|
|
|
|
|
The deep-ocean circulation in the Antarctica
brings abundant nutrients up into the surface water, which is not fully
utilized by photosynthesis due to the brief summer seasons. |
|
During glacial intervals in the Antarctic
region, increased carbon pumping out of surface water could occur either
because |
|
(1)
nutrient-rich waters remained at the surface longer, or |
|
(2)
higher glacial nutrient levels stimulated more productivity. |
|
|
|
|
One of the major factors that determines CO2
levels in surface water of the world oceans is the amount of carbonate ion
CO3-2. |
|
These ions are produced when corrosive bottom
water dissolve CaCO3 on the seafloor. |
|
When these ions are later returned to surface
waters by ocean circulation, they can combine chemically with CO2 and
produce the bicarbonate ion HCO3-. |
|
Therefore, increasing the amount of CO3-2
ions dissolved by and carried in deep water can have the effect of reducing
CO2 concentrations in surface water. |
|
|
|
|
The carbon isotope trend provides clear evidence
that there was a link between the size of northern hemisphere ice sheets
and the formation of deep water in the North Atlantic nearby. |
|
Less deep water formed in the North Atlantic
every time ice sheets grew larger at the 100,000-year cycle after 0.9 Myr
ago. |
|
More deep water formed when ice sheets were
small. |
|
|
|
|
The percentage of deep water originating in the
North Atlantic and flowing to the equator during the last 1.25 Myr has been
consistently lower during glaciations than during interglaciations. |
|
In general, southern-source waters (deep water
formed near Antarctica) dominated tropical Atlantic waters during
glaciations. Northern-source water (deep water formed in the North
Atlantic) dominated tropical Atlantic waters during interglaciations. |
|
|
|
|
Among the changes in the distribution of ocean
carbon that could reduce glacial levels of atmospheric CO2 are: |
|
(1)
fast downward organic carbon pumping in areas of costal or tropical
upwelling, |
|
(2)
similar processes in Antarctic, |
|
(3)
changes in the chemistry of Antarctic surface water toward higher CO3-2
content, |
|
(4)
changes in the chemistry of shallow subsurface water originating from
southern latitudes. |
|
|
|
|
After 0.9 Myr ago, the 41,000-year and
23,000-year cycles of ice volume change were overridden by larger and more
dominant fluctuations of ice sheets at a period of 100,000 years. |
|
The large 100,000-year cycle is not related to
any cycle of orbital variations. |
|
TWO QUESTIONS: |
|
(1)
Why did more ice accumulate after 0.9 Myr ago? |
|
(2)
Why did these large ice sheets melt rapidly every 100,000 years? |
|
|
|
|
Explanation 1: A result of the gradual
(tectonic-scale) cooling. |
|
Tectonic-scale cooling due to the decrease of CO2 |
|
è cooling
reach a threshold value 2.75 Myr ago |
|
è
moderate-size ice sheets can form in
northern hemisphere ice during major summer insolation minima and
disappeared completely during summer insolation maxima. |
|
è the
falling CO2 levels continued |
|
è cooling
reached another threshold value 0.9 Myr ago |
|
è that ice
sheets never completely disappeared during weak summer insolation maxima |
|
è ice
sheets began to grow larger and persist longer |
|
|
|
|
|
Explanation 2: Ice Slipping Effect (nothing to
do with climate changes) |
|
During
earlier glaciations (2.75 – 0.9 Myr ago), ice sheets may have been thin
because they slid on water saturated soil toward lower elevations and
warmer temperatures. |
|
During later glaciations (beginning from 0.9 Myr ago), after ice
sheets stripped off most of the underlying soil, their central regions
could grow higher because they no longer slid. |
|
|
|
|
Slow global cooling together with the less
sliding beneath ice sheets helped to create thicker and more extensive ice
sheets beginning 0.9 Myr ago. |
|
What cause the rapid melting every 100,000
years? |
|
Explanation: the 100,000-year eccentricity cycle |
|
The
100,000-year eccentricity orbital cycle only produces a trivial amount of
direct insolation changes. |
|
It
is the modulation of the 100,000-year cycle on the amplitude of the
23,000-year precession cycle that actually affect the rapid melting every
100,000 years. |
|
|
|
|
|
|
The pace of the 100,000-year variations in ice
sheet size is set by the external forcing from the eccentricity orbital
cycle. |
|
The amplitude of the 100,000-year cycle depends
in part on the internal interactions of the climate system. |
|
The large ice sheets themselves produced
internal interactions within the climate system that hastened their own
destruction every 100,000 years. |
|
The possible positive feedbacks to accelerate
ice sheet melting include: rising CO2 level during deglaciations, the
delayed in bedrock rebound provided warmer temperatures in the depressed
land surface for fast ice melting, and other ice-controlled processes in
wind, sea level, and deep ocean circulation. |
|