Although some researchers
have raised concerns about possible negative effects of rising CO2 on ocean
surface pH, there are several lines of evidence demonstrating marine ecosystems
are far more sensitive to fluxes of carbon dioxide from ocean depths and the
biosphere’s response than from invasions of atmospheric CO2. There is also
ample evidence that lower pH does not inhibit photosynthesis or lower ocean
productivity (Mackey
2015). On the contrary, rising CO2 makes photosynthesis less costly. Furthermore in contrast to
researchers arguing rising atmospheric CO2 will inhibit calcification,
increased photosynthesis not only increases calcification, paradoxically the
process of calcification produces CO2
and drops pH to levels lower than predicted by climate change models. A
combination of warmer tropical waters and coral reef biology results in
out-gassing of CO2 from the ocean to the atmosphere, making coral reefs
relatively insensitive to the effects of atmospheric CO2 on ocean pH.
Sixty million years ago
proxy evidence indicates ocean surface pH hovered around 7.4. If surface pH was
in equilibrium with the atmosphere, then CO2 concentrations would have hovered
around 2000 ppm, but there is no consensus that CO2 reached those levels.
However as will be discussed, there are biological processes that do lower
surface pH to that extent, despite much lower atmospheric CO2 concentrations.
Over the next 40 million
years corresponding with the rearrangement of the continents and ocean
currents, the formation of the Antarctic Circumpolar Current and initiation
of Antarctic glaciers, the evolutionary expansion of diatoms and their
increasing abundance (diatoms are the most efficient algae for exporting carbon
to ocean depths), ocean carbonate chemistry was greatly altered. As a result
ocean surface pH gradually rose above pH 8. Then for our last 20 million years,
ocean surface pH has fluctuated within this new equilibrium between 8.4 and
8.1, as seen in Figure 1 below (Pearson
and Palmer 2000). For the past 400,000 years, pH rose to about 8.35 during
the depths of each ice age. Then during each warm interglacial period, when
both land and marine productivity increased, pH fell to ~8.1 (Honisch
2005).
60 million years of ocean pH |
Although it is commonly
assumed atmospheric CO2 and ocean surface pH are in equilibrium, studies
examining various time frames from daily and seasonal pH fluctuations (Kline
2015) to the millennial scale transitions from the last ice age to our warm
interglacial (Martinez-Boti
2015), demonstrate surface ocean pH has rarely been in chemical equilibrium
with atmospheric CO2. Because oceans contain over 50 times as much CO2 as the
atmosphere, surface pH is more sensitive to changes in the rates of upwelling
of low-pH, carbon-rich deep waters. It is the response of photosynthesizing
organisms and the food webs they support that largely determines how much
carbon is sequestered in the surface layers and then sent to deeper waters (the
biological pump).
As discussed in an
earlier essay, the “biological pump” modulates how much
CO2 is sequestered and how much CO2 will out-gas to the atmosphere. It has been
estimated
that without the biological pump, pre-industrial atmospheric CO2 would have out
gassed and raised atmospheric CO2 to 500 ppm, instead of the observed 280 ppm.
Ironically the processes that build coral reefs also increase surface CO2
concentrations and lower regional pH to levels lower than expected by
equilibrium with atmospheric CO2. This biological control of the earth’s
chemistry is the essence of Gaia theory.
Gaia theory stimulated great
scientific interest (as well as controversy) since the 1970s, and
stimulated more extensive investigations into how the biosphere affects the
earth’s chemistry. Gaia’s founding scientist James Lovelock formulated Gaia
theory while working for NASA seeking chemical signatures of life on other
planets. For example, due to living organisms our atmosphere maintains about a
21% concentration of oxygen. Without photosynthesizing organisms, the
atmosphere would contain extremely low amounts of oxygen. Thus Lovelock argued,
“if life has merely a passive role in
cycling the gases of the air, then the concentrations will be set by equilibrium
chemistry; in fact they most certainly are not.” Shedding the mystical
connotations that many “New Age” adherents attributed to Gaia, several
universities have now created departments studying Gaia’s effects, but under
less anthropomorphic titles such as Earth System Sciences or Biogeochemistry.
Unfortunately Gaia is
often misrepresented as a conscious super-being deserving of religious
devotion, with some adherents even advocating Gaia should replace the earth’s
major religions. Gaia’s deification was resented both in established religious
circles, and by Gaia’s scientific proponents like Dr. Lynn Margulis. She
stressed Gaia is simply “an emergent property of interactions among
organisms". Or as one of her graduate students suggested, Gaia is simply
“symbiosis as seen from space”.
Gaia theory also weighed
in on climate change debates and was advocated by Al Gore and climate
scientists such as Stephen Schneider. While basic Gaia theory simply argues a
variety of biological interactions provide negative feedbacks from which a
degree of self-regulating homeostasis emerges, those with a more alarmist view
of the earth’s changing climate argued those self regulating processes had been
pushed to a disastrous tipping point by rising CO2. In contrast climate skeptics like world-renowned physicist
Freeman Dyson also embraced the concepts of Gaia as a “great force for good”
uniting people to save natural habitat and endangered species. But Dyson also
bemoaned, “I am horrified to see the environmental movement hijacked by a bunch
of climate fanatics, who have captured the attention of the public with scare
stories.”
Despite Lovelock’s belief
that life regulates earth’s chemistry via a variety of negative feedbacks, his
logic was at first swayed by those CO2 scare stories. In a more fearful state
of mind Lovelock published books like “The Revenge of Gaia” and in newspaper
interviews predicted fast-approaching, global-warming doom stating, “Billions
of us will die” and only the “few breeding pairs of people that survive will be
in the Arctic”.
More recently however Lovelock
recanted stating, “I was 'alarmist'
about climate change & so was Gore!” 'The problem is we don't know what
the climate is doing. We thought we knew 20 years ago”.
Putting politics and
religion aside, the Gaia perspective provides a valuable framework that
incorporates the biosphere as a critical active player in global climate and
chemical cycles. And only from that framework can we fully
account for oscillations in the oceans’ pH on daily, annual, decadal and
millennial timeframes.
pH in a
Lifeless World
Global climate models,
such as used by Caldeira
and Wickett 2005, estimated that ocean pH has dropped by (0.09 pH) from 8.2
to ~ 8.1 since preindustrial times due to rising anthropogenic carbon dioxide
emissions. They then predicted a further pH drop of 0.3 to 0.4 by 2100 as
emissions increase. This claim has been cut and pasted into nearly every
journal article that hypothesizes an impending catastrophe driven by “ocean
acidification”. However an average pH of 8.1 is typical for interglacial
periods such as the one we are now experiencing. But more importantly Caldeira and Wickett’s modeling
experiments only examined geochemical processes and erroneously assumed 1)
ocean surface CO2 is in equilibrium with the atmosphere; and 2) the biosphere
was a neutral participant. Caldeira’s
model was based on their non-Gaia assumption that ocean surface pH is “affected
only by air-sea fluxes and directly injected carbon.” Indeed, if sequestration of CO2 by
photosynthesis is immediately offset by the release of CO2 in the surface
layers via respiration, then such an assumption may hold some validity. However
that is never the case. And according
to the IPCC if
there were no biological pump transporting carbon to the ocean depths, oceans
would now be experiencing an 8.0 pH.
Relationship between Atmospheric CO2 and Ocean pH |
As seen in the graph
above from Cohen
and Happer models that suggest ocean pH should have declined over
the past 150 years as atmospheric CO2 concentrations rose are supported by an abiotic chemical analysis. Modulated by
ocean alkalinity, at 400 ppm atmospheric CO2, surface seawater declines to pH
8.2 or 8.1 (blue curve). For
un-buffered rainwater (or river outflows without buffering) pH drops to 5.5
(red dashed curve). However even without any modulating biological effects, the
graph suggests a degree of chemical homeostasis where increasing CO2 concentrations have an increasingly smaller effect on
ocean pH. For example when CO2 concentrations increase from 0 to 100 ppm,
pH rapidly drops from over 11.0 to 8.7. In contrast a quadrupling of
atmospheric CO2 since pre-industrial times (~250 to 1000 ppm) would only lower
ocean surface pH from 8.3 to 7.9 (blue curve). Counter-intuitively the
different dissolved CO2 species exert strong buffering effects. Furthermore far
from being catastrophic, not only is a pH range between 8.4 and 7.7 experienced
daily in thriving coral reefs, that range appears to be an optimal balance that
supports both photosynthesis and calcification!
Extreme views by researchers
like Hoegh-Guldberg (2014)
have speculated 95% of the coral will be lost by 2050, and he argues our
current high levels of CO2 are creating conditions coral have not experienced
for millions of years. Yet in terms of pH (and
temperature) such “scientific” claims are pure nonsense. First a modeled
average surface pH tells us very little about the pH that directly affects
marine organisms locally. Due to the counteracting effects of photosynthesis,
respiration and calcification, coral reefs can experience a pH hovering around
8.5 or higher during the day followed by a low pH of 7.8 or lower at night. Kline
2015 acknowledged, “As with many
other reefs, the nighttime pH minima on the reef flat were far lower than pH
values predicted for the open ocean by 2100.” Elsewhere researchers
concluded that in addition to atmospheric pH, the complex interactions
controlling pH especially in coastal zones, make detection of any trends
towards acidification “not trivial
and the attribution of these changes to
anthropogenic CO2 emissions is even more problematic.” (Duarte
2013)
Why More
Acidic Conditions Benefit Photosynthesis
Shallow-water
reef-building corals are able to thrive in low-nutrient tropical waters via
their symbiosis with a genus of photosynthesizing algae (discussed
here.) In order to sustain photosynthesis, corals actively pump hydrogen
ions (H+) into the vesicles encapsulating their algal symbionts. This lowers
its internal pH to truly acidic levels between pH 4 and 5 (Barott 2015). This
increases H+ concentrations up to 10,000 times greater than any theoretical
contributions to surface waters by atmospheric CO2. If coral do not acidify
their symbionts’ surroundings, the limiting supply of CO2 would dramatically decrease the rate of photosynthesis.
Why does an acidic
environment benefit photosynthesis?
To understand the
benefits of corals’ purposeful acidification, we must first review how CO2
reacts when dissolved in water. Dissolved CO2 can take 3 forms (or “species”)
collectively referred to as Dissolved Inorganic Carbon
(henceforth DIC):
1) Carbonic acid (H2CO3),
2) Bicarbonate ion (HCO3-)
after losing one H+
3) Carbonate ion (CO3-2)
after losing a second H+ .
When CO2 first
dissolves, a small proportion bonds to water molecules and forms a weak
carbonic acid (H2CO3). But the bond is weak causing
carbonic acid to convert back and forth with its CO2 form so rapidly, most
researchers treat these two forms as the same chemical species. Carbonic acid is a weak acid, and weak
acids are critical buffering agents for most living organisms precisely because
its species can rapidly and reversibly change form. Carbonic acid and
phosphoric acid are the 2 most critical buffering agents for maintaining a
narrow pH range in humans and other animals. In the form of carbonic acid,
water’s 2 H+ ions can more easily detach to form bicarbonate and carbonate ions
when pH rises. Buffering happens because those added H+ ions counteract a
rising pH. (Higher pH means lower H+ concentrations.) Conversely when pH falls
(Lower pH means higher H+ concentrations), the excess H+ ions recombine with
and are sequestered by any existing carbonate and bicarbonate ions to
counteract the falling pH.
Figure 2 illustrates how
changes in pH alter the species composition of DIC. For example during
photosynthesis CO2 is consumed causing pH to rise. Between pH 7.0 and 8.6, over
90% of the dissolved CO2 naturally converts to bicarbonate ions (HCO3-).
But bicarbonate ions cannot be directly used in photosynthesis.
Photosynthesizing organisms can only use CO2. Thus if photosynthesis
drives pH to 8.2 or higher, the requisite CO2 species approach zero. In
addition to competing for a dwindling supply of CO2, photosynthesis consumes
the limited supplies of nutrients. Thus photosynthesis creates negative
feedbacks that inhibit additional photosynthesis.
The relationship between pH and proportion of CO2 species |
To overcome the limiting
supply of CO2, organisms like coral concentrate bicarbonate ions in
compartments into which they pump H+ ions and lower the pH. As seen in Figure
2, at pH 5 or lower, 90% of the DIC converts to CO2. Once bicarbonate ions are
imported and concentrated, the conversion to CO2 is also accelerated by the
ubiquitous enzyme carbonic anhydrase. However bicarbonate ions cannot simply
diffuse into a cell or pass through internal membranes. The ions must be
pumped. However pumping and concentrating those ions requires transporters and
an expenditure of energy. In contrast whenever surrounding waters experience a
lower pH, it makes CO2 more available so that the energy expenditures drop
because CO2 freely diffuses into cells and through membranes.
The same carbonate
chemistry reactions that provide more CO2 for photosynthesis also explain how
some pharmaceutical antacids work and how DIC buffers ocean pH. Bicarbonate is
a common ingredient in antacids like Alka-seltzer. When H+ ions increase due to
acid indigestion, ingested bicarbonate ions rapidly bond to H+ to form CO2 gas,
which can then be carried away by the blood or by a good belch. Likewise when
ocean concentrations of H+ ions increase, they more readily bond to the
bicarbonate and carbonate ions to minimize the drop in pH and form more CO2,
which can be quickly utilized during photosynthesis.
However below pH 7.0,
nearly all carbonate ions (CO3-2)
will be converted to bicarbonate (HCO3-), so that
carbonate ions no longer serve as buffering agents. (CO3-2 + H+ forms HCO3- ).
However in coral reefs, that loss of buffering capacity at lower pH is
counteracted to a degree by increased dissolution of calcium carbonate
minerals. Dissolution of calcium carbonates counter-intuitively absorbs CO2 and
releases carbonate ions to increase the water’s buffering capacity, thus
exerting a negative feedback that tries to raise pH (Morse 2007).
Nonetheless the concept that a lower pH reduces the concentration of carbonate
ions evoked climate fears amongst some researchers who incorrectly believed calcifying organisms require carbonate
ions. But research shows no such
requirement. All calcifiers use the more abundant bicarbonate ions and
bicarbonate ions will be plentiful even if pH unrealistically fell to 6.0
Outside of coral reefs,
other marine ecosystems also benefit from lower pH. For example diatoms now
account for 40% of the world’s ocean primary productivity and flourish in
upwelling waters that bring abundant CO2 and DIC from the ocean’s dark depths
into sunlit surface regions. Although this upwelling deceases surface pH and
provides more CO2, diatoms still rely on bicarbonate transporters and carbonic
anhydrase to ensure an adequate supply of CO2 for photosynthesis. Hopkinson et al. (2011)
calculated a doubling of ambient CO2 levels would save diatoms ~20% of the
energy they expended on importing bicarbonates. Globally different
photosynthesizing organisms have demonstrated a variety of responses to rising
CO2 but altogether there appears to be few negative effects on photosynthesis
due to elevated CO2 and depending on the species small to large benefits (Mackey 2015).
The Omega Myth
In a lifeless ocean when
carbonate ions rise to a certain concentration, they react with ever-present
calcium ions to form calcium carbonate minerals like aragonite and calcite.
Those minerals are used to make shells, skeletons and reefs. If carbonate ion
concentrations are lower, calcium carbonate minerals are more likely to
dissolve. When there is a balance between formation and dissolution of those
minerals, the water is said to be saturated with respect to that mineral, and
saturation is represented by the omega symbol (W).
The oceans are currently oversaturated with respect to calcium carbonate
minerals, but some researchers became fearful that a falling pH could lower the
supply of carbonate ions, and eventually drive the ocean’s saturation point so
low that calcium carbonate minerals will dissolve faster than they form.
However biologically controlled calcification reveals that simple metrics of
chemical equilibriums and saturation points do not accurately demonstrate the
biologically controlled calcification process. In that regard several
researchers have now published evidence demonstrating the “Omega
Myth”.
First biologically
controlled calcification does NOT depend on, or directly utilize seawater
carbonate ions. Nor does calcification depend on observed saturation states of
the oceans (Maranon
2016). Transporters are required
for carbonate ions to cross any membrane, but no carbonate transporters have
ever been detected. Instead, as with photosynthesis, calcifiers actively uptake
the more abundant bicarbonate ions and concentrate them in compartments. Most
calcifying organisms have evolved mechanisms to “up-regulate” their internal pH
by pumping H+ ions out of the compartment and raising internal pH. In addition
pumping H+ ions out of the
calcifying compartments is beneficial because it maintains an electrical gradient
that facilitates importing calcium ions (Ca++) into the calcifying compartment.
With a higher internal pH, bicarbonate sheds an H+ and converts into carbonate
ions and when concentrated in the presence of concentrated Ca++, calcium
carbonate minerals readily form.
Although in some species
photosynthesis and calcification compete for bicarbonate ions, photosynthesis
generally benefits calcification by providing energy, and by raising external
pH, which lowers the cost of pumping internal H+ ions to the surrounding
waters. In addition on a per molecule basis, the cost of calcification requires
less than 1% of the energy produced by photosynthesis (McCulloch
2012). Accordingly numerous studies have reported that greater rates of
photosynthesis correlate with greater rates of calcification. The same holds
true for other calcifying organisms. For example across the tropical ocean, the
ratio of net calcification to net photosynthesis for coccolithophores remained
constant despite regions of widely varying surface pH and calcite saturation
levels (Maranon
2016).
Past hypotheses arguing
calcification was dependent on carbonate ion concentration, or aragonite and
calcite saturation levels, were most likely misled by the fact that higher
carbonate ion concentrations are a daily “side effect” of photosynthesis. It is
the rate of photosynthesis and the energy it provides that typically controls
calcification rates. And as reported in the discussion on the coral adaptive
bleaching hypothesis, coral are always shifting and shuffling their
symbionts to maximize photosynthesis to best adapt to changing local
microclimates. The bigger threat to coral photosynthesis is heavy sediment
loads from disturbed landscapes that can block the sun and suffocate polyps.
How Calcification Lowers pH more than Atmospheric
CO2
Strangely enough, although
some researchers fret higher CO2 concentrations will reduce calcification, it
is the very process of calcification that results in the “alkalinity pump.” Calcification
removes buffering bicarbonate and carbonate ions from the surface and pumps
them to the deep. Calcification also releases CO2 in the surface waters and in
combination with less buffering capacity, lowers pH to a much greater extent
than possible by surface exchanges with rising atmospheric CO2.
Assuming the modeled
background pH of 8.1, and if all else is equal, we would expect pH to rise
during the day due to photosynthesis and then fall back to pH 8.1 at night due
to respiration. As seen in the graph below for daily (diel) pH values on Heron
Island in the Great Barrier Reef (from
Kline 2015), coral reefs rarely spend any time at Caldeira’s modeled pH
value of 8.1. When photosynthesis and carbonate dissolution outweigh
respiration and calcification, surface pH can rise to 8.4 or higher as would be
expected. Furthermore when surface pH is above 8.1, the concentration of
surface CO2 is lower than atmospheric CO2, and this difference allows CO2 to
diffuse into the ocean. However
any absorbed CO2 is quickly sequestered into organic molecules via
photosynthesis during which surface pH remains high and never comes into
equilibrium with atmospheric CO2 during the day.
Daily Changes in pH on Heron Island Great Barrier Reef |
Conversely without
photosynthesis, nighttime respiration and calcification increase surface CO2
concentrations and lower pH. Reefs benefit because those processes replenish
the depleted CO2 required for photosynthesis on the following day. Furthermore
if more organic molecules are formed and sequestered than subsequently
respired, we would expect surface pH to remain above 8.1. Indeed photosynthesis
produces a large reservoir of dissolved and particulate organic molecules that
may persist for decades, centuries, and millennia. When those stored molecules
eventually return to the surface, pH can be lowered due to respiration of
ancient carbon, independent of atmospheric CO2. Other organic molecules are
also formed that resist decomposition for millions of years. And molecules like
DMS are out-gassed to the atmosphere where they serve as cloud condensation
nuclei and inhibit further warming of ocean surface temperatures.
Thus due to long-term
sequestration of CO2 that exceeds respiration we would expect surface pH to
remain above 8.1 for the short term. However due to the release of CO2 during
calcification, reef pH drops far below 8.1. Calcification infuses the surface
waters with an excess of CO2 largely driving the nighttime pH down as low as
7.7. Furthermore at a pH below
8.1, CO2 concentrations in the ocean’s surface rise higher than the
atmosphere’s, and this results in nighttime out-gassing of CO2. Instead of CO2
invading the ocean and affecting coral, overall measurements show coral reefs
are net sources of CO2 from the ocean to the atmosphere. Similar dynamics from
calcifying coccolithophores likewise promotes CO2 fluxes from the open ocean,
and inhibits uptake from the atmosphere. Again as Gaia predicts, biological
processes control carbonate chemistry and when or where atmospheric CO2 enters
or leaves the ocean.
Although studies in the
waters around Hawaii (Dore 2009)
reported an increasing trend in DIC that was “indistinguishable” from what
rising atmospheric CO2 predicts researchers observed, “Air-sea CO2
fluxes, while variable, did not appear to exert an influence on surface pH
variability. For example, low fluxes of CO2 into
the sea from 1998–2002 corresponded with low pH and relatively high fluxes
during 2003–2005 were coincident with high pH; the opposite pattern would be
expected if variability in the atmospheric CO2 invasion was the
primary driver of anomalous DIC accumulation.” However that observed pattern is exactly what we would expect
to arise from biological effects.
Furthermore oscillating
decadal trends in wind strength can further magnify biological effects causing
pH to trend independently of atmospheric CO2. CO2 generated by calcification
does not completely outgas and thus changes in the rate at which reefs are
flushed with open ocean water will modulate how calcification affects surface
pH. In contrast to Caldeira’s “lifeless” pH models that suggest pH has dropped
from 8.2 to 8.1 since preindustrial times, a study of pH since 1700 AD on
Flinder’s Reef in the Great Barrier Reef concluded pH has oscillated between
8.15 and 7.9 every 50 years. During a positive Pacific Decadal Oscillation and
El Nino years, trade winds slowed and reduced the flushing rate of the reef. As
a result there was a build up of CO2 released from calcification and average pH
dropped pH to 7.9. When winds increased during a negative PDO and more La
Ninas, the reef was flushed and pH rose to 8.15. Several studies have linked
changes in pH driven with multidecadal oscillations.
For example examining
surface pH in the Sargasso Sea Goodkin
2015 reported, “from 1950 to 1996, when
surface ocean pHs are predicted to decline
more rapidly due to anthropogenic CO2 emissions,
pH at Bermuda increases in response
to a declining AMO.” They concluded, “ocean pH does not simply reflect atmospheric CO2 trends but
rather that circulation/biogeochemical changes account for >90% of pH
variability in the Sargasso Sea and more variability in the last century than
would be predicted from anthropogenic uptake of CO2 alone.”
Similarly Yeakel
2016 reported Bermuda reefs experienced a drop in pH in association with a
negative NAO that caused westerly winds to move further south and generate a
deeper winter mixed layer just to the north of the Bermuda reefs. Deeper mixing
brought more DIC to the surface layers and promoted greater plankton blooms.
The resulting organic particles and zooplankton that fed on the blooms, then
circulated over the Bermuda reef. The resulting increase in respiration and calcification
caused an “acidification event”.
Thus to reliably
distinguish multidecadal trends in pH driven by ocean oscillations, upwelling
and deeper surface mixing versus trends due to rising atmospheric CO2, it will
require 60 to 100 years of observation; far longer than any data series to
date.
Ocean Surface
pH is More Sensitive to Ventilated CO2 Stored at Ocean Depths
Published estimates of
anthropogenic CO2 now stored in the upper ocean layers and affecting pH has
been based on “the assumption that ocean circulation and the biological pump
have operated in a steady state since preindustrial times” (Sabine
2010). The problem is such assumptions are faulty and misleading. The
biological pump and ocean circulation are not in a steady state. Regional
upwelling has increased since the Little Ice Age (Gutiérrez 2009) and during
the past 3 decades (Varela
2015). Multidecadal changes in hurricane
frequency and intensity affect upwelling. Changes in surface winds due to El
Nino and La Nina, the North Atlantic Oscillation and Pacific Decadal
Oscillation affect upwelling (Ishii 2002).
Coastal and equatorial upwelling bring an enormous amount of DIC to the
surface, with subsequent transport to the gyres of the open ocean, causing
declines in open ocean surface pH at rates that are much faster than possibly
attributed to atmospheric diffusion.
While 50% of the
sequestered carbon formed during photosynthesis is respired before sinking into
the dark depths, a tremendous pool of dissolved organic carbon has been created
that may not be respired for decades, centuries or millennia and slowly
contributes to the pool of DIC at various depths and locations (Giorgiou
2002). This further complicates any attribution of trends in surface pH.
For example upwelling of stored CO2 is believed to have been the main driver of
the rise in atmospheric CO2 and the fall in ocean surface pH during the
transition from the glacial maximum to our interglacial.
As discussed in the
article on natural
cycles of ocean “acidification”, and illustrated in the graph below by Martinez-Boti, over the past 15,000 years proxy data (thick
lines) has determined surface pH has rarely been in equilibrium with
expectations (green line) based on models driven by atmospheric CO2. As
illustrated, surface pH was more sensitive to the upwelling of subsurface DIC.
The venting of stored carbon led to a drop in average regional pH from the 8.3
during glacial times to a pH fluctuating between 8.1 and 8.2 during our current
interglacial.
Difference between ocean surface pH and modeled pH from atmospheric CO2 |
The mechanisms that
lowered surface pH to 8.3-8.4 during the Last Ice Age is a matter of
considerable debate, but clearly more carbon was being sequestered at depth and
less carbon was being pumped to the surface. Several authors have reported less
upwelling during the Ice Age. While colder temperatures and less upwelling
would reduce rates of photosynthesis, colder temperatures also reduce rates of
respiration and calcification. A lower rate of respiration would allow more
organic carbon to sink to deeper depths before being completely consumed. Sinking
to deeper depths prevents a quick return to the surface during winter mixing or
mild upwelling.
It has also been
speculated that the loss of coral reefs during the last Ice Age contributed to
the higher pH. Research
has estimated that during the cold nadir of each ice age, coral reef extent was
reduced by 80% and carbonate production was reduced by 73% relative to today.
Lower calcification rates would reduce the alkalinity pump, reduce surface CO2
and increase the buffering capacity of surface waters. Conversely the growth of
coral reefs as the earth warmed and sea levels rose would contribute to rising
CO2 concentrations and falling pH. Vecsei 2004
concluded, “The pattern of reef growth that emerges suggests that emission of CO2 resulting from carbonate
production was important particularly during the late stages of
deglaciation.”
Overall observations of
the effects of photosynthesis and calcification reveal coral reefs are not
victims of a fall of pH from 8.2 to 8.1 pH as suggested by Caldeira
and Wickett 2005, Doney
2009
or Hoegh-Guldberg (2014).
On the contrary as Gaia theory would suggest, coral reefs are actively
regulating surface pH.