http://www.sciencedaily.com/releases/2009/05/090506131512.htm
Science News
Ocean Carbon: Dent In Iron Fertilization Hypothesis Previously
Proposed To Address Climate Change

ScienceDaily (May 6, 2009) — Oceanographers Jim Bishop and Todd Wood
of the U.S. Department of Energy’s Lawrence Berkeley National
Laboratory have measured the fate of carbon particles originating in
plankton blooms in the Southern Ocean, using data that deep-diving
Carbon Explorer floats collected around the clock for well over a
year. Their study reveals that most of the carbon from lush plankton
blooms never reaches the deep ocean.

The surprising discovery deals a blow to the simplest version of the
Iron Hypothesis, whose adherents believe global warming can be slowed
or even reversed by fertilizing plankton with iron in regions that are
iron-poor but rich in other nutrients like nitrogen, silicon, and
phosphorus. The Southern Ocean is one of the most important such
regions.

“Just adding iron to the ocean hasn’t been demonstrated as a good plan
for storing atmospheric carbon,” says Bishop, a member of Berkeley
Lab’s Earth Sciences Division and a professor of Earth and planetary
sciences at the University of California at Berkeley. “What counts is
the carbon that reaches the deep sea, and a lot of the carbon tied up
in plankton blooms appears not to sink very fast or very far.”

The reasons, while complex, are most likely due to the seasonal
feeding behavior of planktonic animal life, and specifically to the
effects of the dark Antarctic winter on plant and animal growth and
the mixing of surface and deep waters by winter storms. Phytoplankton
blooms in the spring may indicate that much of the zooplankton
(animal) population essential for carbon sedimentation has starved
during the winter.

The Carbon Explorers involved in the study were launched in January,
2002, as part of the Southern Ocean Iron Experiment (SOFeX), a
collaboration led by scientists from Moss Landing Marine Laboratory
and the Monterey Bay Aquarium Research Institute. SOFeX was meant to
test the Iron Hypothesis in waters between New Zealand and Antarctica
during the Antarctic summer. The Berkeley Lab Carbon Explorers were
originally intended to monitor the iron-fertilization experiment for
60 days, but they continued to report by satellite throughout the
Antarctic fall and winter and on into the following year.

“We would never have made these surprising observations if the
autonomous Carbon Explorer floats hadn’t been recording data 24 hours
a day, seven days a week, at depths down to 800 meters or more, for
over a year after the experiment’s original iron signature had
disappeared,” Bishop says.

He explains that “assumptions about the biological pump – the way
ocean life circulates carbon – are mostly based on averaging
measurements that have been made from ships, at intervals widely
separated in time. Cost, not to mention the environment, would have
made continuous ship-based observations impossible in this case.
Luckily one Carbon Explorer float costs only about as much as a single
day of ship time.”

The Iron Hypothesis, science and speculation

In the 1980s, oceanographer John Martin of the Moss Landing Marine
Laboratories, who died in 1993, proposed that iron added to regions of
the ocean that are otherwise rich in nutrients but poor in iron (so-
called high-nutrient, low-chlorophyl, or HNLC, regions) can stimulate
the growth of phytoplankton – a bold scientific hypothesis that has
since been proven correct.

Martin went further, however, when he suggested that artificial iron
fertilization of the oceans could change the climate. “Give me half a
tankerful of iron and I’ll give you an Ice Age,” he boasted in 1988.

In testing the Iron Hypothesis, SOFeX’s investigators acknowledged
that matters were not quite that simple, and that the crucial question
was not whether plankton blooms could be induced but whether the
carbon they captured was removed to the deep sea.

The SOFeX research vessels fertilized and measured two regions of
ocean, one in an HNLC region at latitude 55 degrees south and another
at 66 degrees south. Carbon Explorers were launched at both these
sites; a third Carbon Explorer was launched well outside the iron-
fertilized region at 55°S as a control. Berkeley Lab scientists Todd
Wood, Christopher Guay, and Phoebe Lam were members of the expedition,
while Bishop monitored and communicated with the Carbon Explorers from
Berkeley over a computer link to communications satellites.

One question was whether the relatively silicate-poor waters of the
more northerly 55° region would allow plankton known as diatoms to
form silicon skeletons. If large diatoms could not grow in this HNLC
region, the SOFeX researchers theorized, enhanced carbon sinking would
not occur. Partly for this reason, most of the effort by the ships was
at 66°S, where silicon wasn’t considered a limiting factor.

To the researchers’ surprise, the iron-augmented region at 55°N did
form a vigorous plankton bloom. Dubbed the North Patch, Carbon
Explorers tracked this bloom throughout the Antarctic summer,
measuring carbon particles, including waste from grazing zooplankton
and other aggregates, sinking beneath the bloom and carrying 10 to 20
percent of the fixed carbon out of the surface layer – at least to
below 100 meters. The initial results of the SOFeX experiment,
published in Science in April, 2004, seemed to support the Iron
Hypothesis in an unexpected way.

But the Carbon Explorers didn’t stop after 60 days. The two North
Patch floats operated for over 14 months, diving, recording, and
surfacing to report data in the world’s stormiest waters, traveling
almost to South America before falling silent. The Carbon Explorer
launched at 66° south lasted 18 months, spending much of its first
winter recording at 800 meters depth and surfacing at weekly intervals
to report, although occasionally prevented by bumping into the
underside of the sea ice. The Carbon Explorer data accumulated,
awaiting analysis.

Return to the Southern Ocean

In 2007 Bishop and Lam (who was now at the Woods Hole Oceanographic
Institution) published measurements from shipboard instruments
deployed during SOFeX which suggested that the rosy picture of
plankton blooms sending carbon to the deep ocean wasn’t so simple
after all. Carbon reaching the deep ocean depended partly on particle
size and weight; more important, there seemed to be much less
particulate matter reaching depth where the biomass was highest, e.g.,
in plankton blooms.

“This paper was criticized on the grounds that it was based on limited
shipboard observations,” says Bishop. “So Todd Wood and I turned to
the treasure-trove of virtually continuous observations in the records
of the Carbon Explorers.”

The Carbon Explorers’ records through the Antarctic summer and fall of
2002 and the winter and spring of 2003 (and in the case of the float
at 66° south, much longer) not only confirmed the limited shipboard
observations in greater detail but opened up a complex picture of life
in the Southern Ocean.

The Carbon Explorer at 66°S recorded data never before observed or
reported. During the SOFeX experiment, the float had measured the
demise of a plankton bloom rich in particulate organic carbon.
Particulate carbon levels were severely reduced with the onset of
perpetual darkness and sea ice formation, then modestly increased
again with the return of light and the melting of the ice. Strong
sedimentation – the sinking of large numbers of carbon particles to
the deep ocean – was never observed.

Data from the two floats deployed farther north at 55°S produced a
startling picture. As noted above, the Explorer launched inside the
original SOFeX iron-amended region, dubbed 55A, had recorded a long-
lasting bloom immediately following iron fertilization, with
sedimentation to 100 meters. Remarkably, 55A found an equally strong
bloom the next spring in the same region – long after the SOFeX iron
was gone – with equally strong sedimentation down to 100 meters.

And while it was unsurprising that the original control float, dubbed
55C, did not see a bloom, a bigger surprise came at depth: a rain of
particulate organic carbon at 800 meters down. Carbon Explorer 55C had
measured sedimentation beneath a region with no plankton bloom much
greater than the 55A float measured under the bloom itself.

To explain this counterintuitive “High Biomass, Low Export” result the
researchers considered a number of ideas. Perhaps current shears had
separated the plankton blooms from their sedimentation; or perhaps
there were “large rare particles” of organic carbon that the Carbon
Explorers had failed to observe; or perhaps differences in mixing of
surface and deep waters during winter storms had brought sequestered
iron back to the surface. The first two hypotheses were rejected, and
the third, even if true, would imply that iron-stimulated blooms still
lead to reduced carbon sedimentation at kilometer depths.

A fourth hypothesis, taking into account the lighting conditions that
encourage or limit the growth of microscopic plants and zooplankton,
emerged as the most convincing. Latitude 55°S is far enough north for
light to reach into the water year round (although in winter it is
much reduced). But mixing between near-surface and deeper waters can
carry phytoplankton too deep to grow – out of the light, beneath the
critical depth where growth is sufficient to meet the energy demands
of the whole plant and animal community. The latitudes where the
Explorers operated are infamously stormy; in wintertime the mixed
layer can reach 400 or 500 meters deep.

To survive the winter, zooplankton have to stay deep, where it’s too
dark for the phytoplankton they live on to survive. Storms and deep
mixing keep the zooplankton alive. “Mixing is the dumbwaiter that
brings food down,” says Bishop. “The question is whether the
dumbwaiter is empty or full.”

When mixing is consistently below the critical level, phytoplankton
are carried out of the light and can’t grow; the dumbwaiter stays
empty and the zooplankton starve. When mixing stops in the spring, the
fast growing phytoplankton rebound, but there aren’t enough surviving
zooplankton population to keep up with the growth and resulting bloom,
and also less production of the sinking carbon particles other
zooplankton species depend on. With fewer animals to intercept the
material as it falls between 100 and 800 meters, Carbon Explorer 55A
observed a low carbon export to the deep ocean beneath the lush bloom.

Continual deep mixing can starve zooplankton, but if the mixing is
regularly interrupted, more phytoplankton grow during the winter to
supply the zooplankton lurking at depth. In the region where Carbon
Explorer 55C spent the winter, storms were intermittent and mixing
below 400 meters was interrupted on a daily basis. When phytoplankton
growth began in the spring, the healthy zooplankton were there to “mow
the lawn,” as it were – probably accounting for the modest
phytoplankton growth near the surface, with increased carbon
sedimentation from the zooplankton.

Bishop says these observations point to an important lesson: “Iron is
not the only factor that determines phytoplankton growth in HNLC
regions. Light, mixing, and hungry zooplankton are fundamentally as
important as iron.”

The Iron Hypothesis isn’t wrong, but it’s much more subtle than
usually stated. Achieving optimum carbon sedimentation from plankton
growth may require the right “recipe” of iron and other trace
nutrients to grow the right kind of phytoplankton. Says Bishop, “You
can grow a lot of Brussels sprouts, but kids won’t eat it. The same
appears to be the case with diatom phytoplankton and zooplankton. It’s
the zooplankton community that determines carbon sedimentation.”

The new study brings one other important lesson: two Carbon Explorers
deployed under similar circumstances experienced subtle differences in
ocean physical conditions that resulted in very distinct biological
responses. A fleet of Carbon Explorers could yield essential data on
the workings of the ocean’s biological pump at far less cost than a
shipborne expedition, and answer questions that cannot be answered now
– such as how much man-made atmospheric carbon the ocean can absorb,
and how much longer we can depend on it to soak up our excesses – and
most important, how the biological carbon pump will respond to
changing ocean conditions.

Journal reference:

   1. James K. B. Bishop and Todd J. Wood. Year-round observations of
carbon biomass and flux variability in the Southern Ocean. Global
Biogeochemical Cycles, DOI: 10.1029/2008GB003206

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