|
d18O is a comparison of ratios,
like the d13C values. |
| How is oxygen fractionated?
|
Physical processes:
 | Evaporation favours H216O (the lighter isotope). |
 | Precipitation condenses H218O preferentially (the
heavier isotope). Therefore atmospheric water vapour is enriched in 16O. |
 | Ice caps remove 16O-enriched water from the ocean/atmosphere
cycle. Therefore during times of extensive glaciation, the oceans are depleted in 16O
and enriched in 18O. Since glacial episodes correspond to periods of low sea level,
measuring d18O in seawater will
tell us about relative sea levels. |
|
Biological processes:
 | Formanifera and other marine organisms fractionate oxygen in the formation
of carbonate skeletons. |
|
| How is information about the oxygen isotope ratio in seawater preserved?
|
 | Carbonate skeletons secreted by formanifera reflect the 18O/16O
ratio in seawater. |
 | 18O/16O ratios in
carbonate skeletons are greater in cold than in warm water. So d 18O values of carbonate sediments preserve information about deep
ocean temperatures (and, by extension, about surface temperatures), and about
surface ocean temperatures at high latitudes. |
 | Different formaniferan species fractionate oxygen differently.
Therefore d18O values in carbonate
sediments are determined by a complex interplay of the species
concerned, water temperature, and the 18O/16O
ratio of the seawater.
Nevertheless, d18O values are
used to infer deep ocean temperatures and sea levels for the
Pleistocene. |
|
| Equations affecting the carbon
cycle |
| Carbonate weathering |
(TDE
Equation 3.6a)

Weathering
of carbonate minerals takes 1C from the atmosphere and 1C from the
carbonate mineral to form 2 molecules of bicarbonate in solution.
Precipitation of calcium carbonate from solution simply reverses the first
reaction, and returns 1C to the atmosphere. Overall the cycle is in balance,
with no net loss of C from the atmosphere. |
| Silicate weathering |
(TDE Equation 3.6b) (TDE
Equation 3.6a)
Weathering of silicate minerals removes 2C from the atmosphere to form
2 molecules of bicarbonate in solution. Precipitation of calcium
carbonate from solution is not the reverse of the first reaction.
Precipitation restores 1C to the atmosphere, leaving a net loss of 1C from
the atmosphere. Hence silicate weathering removes CO2
from the atmosphere.
Note that weathering of calcium silicates also draws down CO2,
as described in Origin of Earth and Life, p. 76:
where the carbonic acid on the left is formed by reaction of
atmospheric CO2 with water. |
| Organic carbon burial |
(OEL
Equation 1.4, aerobic photosynthesis)
(OEL Equation
4.7, respiration)
Burial of organic carbon blocks
the respiration reaction in the cycle above, causing a net drawdown of CO2
and allowing O2 to accumulate in the atmosphere. |
| Summary |
What causes the net loss of C from the atmosphere?
Net loss of C from the atmosphere arises from the fact that,
whereas the formation and weathering of carbonate rocks (CaCO3)
is a cycle in balance, silicate rocks are formed by geological
processes not involving atmospheric carbon. Silicate weathering
removes 2C from the atmosphere, and precipitation of carbonates
using HCO3 (aq) released by silicate weathering returns
only 1C to the atmosphere.
In effect, the formation and weathering of silicates links
processes in the mantle and crust to processes affecting the
atmosphere.
In conclusion:
 | Weathering & precipitation of carbonate rocks results in no net
gain or loss of CO2 from the atmosphere. |
 |
Weathering of silicates and precipitation of carbonates results
in a net loss of CO2 from the atmosphere.
|
|
- The sources of 87Sr and 86Sr in the
Earth. 86Sr is a primordial constituent of the Earth, acquired at the time
of accretion from the Primitive Solar Nebula. 87Sr is entirely
derived from the radioactive decay of 87Rb, which is a primordial
constituent of the Earth.
|
- Why the 87Sr/86Sr ratio in any rock increases over
time. 86Sr is a stable isotope and the amount does not
change, whereas the radioactive decay of 87Rb adds to the amount of 87Sr.
|
- Why the 87Sr/86Sr ratio in continental crust is higher than
that in oceanic crust, and the ratio in oceanic crust is higher than that in the
upper mantle. 87Rb is an incompatible
element. Partial melting which generates basaltic magma at mid-ocean ridges
depletes the upper mantle of 87Rb and enriches it in the oceanic
crust. Likewise, partial melting at subduction zones depletes 87Rb in
oceanic crust and enriches it in continental crust. So crustal rocks are
enriched in 87Rb, which is the source of 87Sr.
|
- Why the 87Sr/86Sr ratio in oceanic hydrothermal
fluids is lower than that in rivers. Hydrothermal systems in
the oceans sample basaltic oceanic crust, which, because it is the first
distillation of the upper mantle by partial melting, has a lower 87Sr/86Sr
ratio than the continental crust being sampled by rivers.
|
- With reference to Figure 6.20, how can 87Sr/86Sr ratios
be determined for the geological
past. By measuring the ratio in
marine carbonate rocks.
|
- What the ratios tell us about palaeoweathering.
They show
changes in the input of 87Sr to the oceans. This is argued (TDE p. 205)
to have been caused by changes in the rate of continental weathering, which in
turn may be a result of uplift of the Himalayas and the Tibetan Plateau. The
evidence from 87Sr/86Sr ratios must be supplemented by
independent evidence of other kinds (e.g. rates of ocean floor production).
|
| There are three orbital cycles which are thought to influence
climate by changing the incidence and distribution of solar radiation on the
Earth, viz.:
 | Eccentricity of the Earth’s orbit.
Periodicity of 110,000 years. Affects the total amount of solar radiation
reaching the Earth. An elliptical orbit exaggerates the seasons in the
hemisphere in which winter occurs at aphelion and summer at perihelion. |
 | Change in the angle of tilt of the Earth’s axis
(21.8° - 24.4° ).
Periodicity of 40,000 years. Changes the effective latitude of the Tropics.
Higher tilt gives warmer summers & colder winters. |
 | Precession of the equinoxes.
Periodicity of 22,000 years. Solstices and equinoxes move clockwise around the
orbit. Changes the position in the Earth’s orbit at which the seasons occur. |
The three cycles operate independently of
each other. They combine to produce variations in the intensity of the seasons
and the amount of solar radiation reaching the Earth. They are the principal
forcing factors controlling the glacial/interglacial cycles during the
Pleistocene Ice Age.
|
| Frequently
Asked Questions |
Answers |
| How far back in geological time can these
cycles be traced? |
About 1.6 Ma, into the
Pleistocene. |
| Did the Milankovitch cycles operate in the distant geological past? |
Probably. There is little direct evidence. Previous ice ages probably
experienced similar climate variations to that of the Pleistocene, though the
rock record does not resolve such small time cycles for the distant geological
past. |
|
Do the Milankovitch cycles operate only during ice ages?
|
No.
Their effects are most obvious during the Pleistocene Ice Age because the
advance and retreat of ice sheets leaves a strong signal. |
| In what ways have the signals of orbital forcing during the Pleistocene been
detected? |
 |
TDE Figure 5.14 - Variations in sea level and
the amount of ice in Northern Hemisphere ice caps, to 600,000 yrs. |
 | TDE Figure 5.15 - Global sea level record
to 1.6 Ma. |
 | TDE Figures 6.22 & 6.23 - Cyclical
changes in the Monsoons, especially as recorded in sediment records in the
Arabian Sea (% CaCO3, % terrigenous sediment, total sediment
accumulation, d 18O variations in
biogenic carbonates). |
|
| Frequently Asked Questions |
Answers |
| How is the Carbonate Compensation Depth (CCD) defined? |
The
CCD is the depth below which <20% of the sediment buried on the sea-bed
consists of carbonate material. |
| Is the CCD everywhere and always the same? |
No. The CCD is
determined by the concentration of dissolved carbonate [CO32-]
in ocean waters and the acidity of ocean waters. High levels of dissolved
carbonate will depress the CCD; high acidity will tend to raise it. |
| What processes will affect the CCD? |
 | High organic productivity in surface waters will depress the CCD, by
increasing the amount of carbonate material sinking through the water
column, thereby raising the concentration of dissolved carbonate. |
 | A high concentration of dissolved CO2 will increase acidity,
tending to raise the CCD. |
|
|
In what circumstances will marine limestones be deposited? |
Where
the sea bed is above the CCD. |
|
What happened concerning carbonate deposition during the Cretaceous (Ref Fig.
5.23, p. 173)? |
 | Before 100 Ma, shallow water carbonate factories caused the deposition of
limestones in shelf seas. |
 | In deeper water, carbonaceous rocks (e.g. the Gault Clay) were deposited
in anoxic conditions |
 | Increased hydrothermal activity (superplumes) raised CO2
concentrations in the atmosphere and oceans, contributing to global warming
and to anoxia in the oceans |
 | At about 100 Ma, deep water carbonate factories become established with
the evolution of coccolithophores. |
 | CCD is depressed by high surface productivity in deep water, leading to
deposition of more carbonate rocks. Much more efficient sink for CO2. |
 | Anoxic conditions give way to oxic conditions in deep water, which further
depresses the CCD |
|
| Is the Chalk a manifestation of
the deep sea carbonate factory? |
Yes and No! The Chalk was deposited in
shallow shelf seas, not deep sea basins. But it is composed of coccoliths, the
calcareous skeletons of the same planktonic plants which were responsible for
the deep sea carbonate factory – they flourished in the photic zone,
regardless of the water depth beneath them! |