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deliver westward acceleration to the mean flow.
Furthermore, the stronger tropical upwelling dur-
ing Boreal winter slows down the QBO’s descent,
allowing more time for the extratropical waves to
impact during this particular phase.
Of course, it is also possible that our current
numerical models can not properly represent the
processes disrupting the QBO. To investigate
this, the foregoing RMS analysis that was applied
to the observational record was applied to his-
torical global climate model runs so as to identify
possible analogous events (Fig. 4, A to C). Among
the available models that produce a QBO inter-
nally, only one rarely produced behavior similar
totheobserveddisruption, withanexampleshown
in Fig. 4D. The extreme profiles resemble those
observed during 2016 with a thin layer of west-
ward wind appearing within an otherwise east-
ward QBO phase.
What will happen next? The recent disruption
of the QBO is a rare event that occurs in the
northern winter. The forecast initialized after
the disruption (Fig. 3B) suggests that the QBO
will return to more regular phase progression
over the coming year. The westward jet that
suddenly appeared in the lower stratosphere is
predicted to amplify in the summer of 2016 and
progress downward with time. Eastward flow then
descends from the 20-hPa level and dominates
the lower stratospheric flow toward the end of
2016, returning the QBO to its typical behavior.
We then expect regular and predictable QBO
cycling to continue from 2017, as occurs in the
available climate models (Fig. 4D). Nonetheless,
as the climate warms in the future, climate models
that simulate these events suggest that similar dis-
ruptions will occur up to three times every 100 years
for the more extreme of the standard climate
change scenarios. This is consistent with a pro-
jected strengthening of the Brewer-Dobson cir-
culation due to increasing stratospheric wave
activity (14) and the recently observed weakening
of the QBO amplitude in the lower stratosphere
(21) under climate change. However, robustly
modeling how the QBO and its underlying pro-
cesses and external influences will change in
the future remains elusive.
There is a further outcome of the 2016 dis-
ruption of the QBO. After an eastward QBO at
the onset of the 2015–2016 winter, the QBO at the
onset of the coming winter of 2016–2017 was
expected to be westward. The disruption of early
2016 means that an eastward QBO phase is now
again expected in the lower stratosphere. Because
of the expected QBO influence on the Atlantic jet
stream, this increases the risk of a strong jet,
winter storms, and heavy rainfall over northern
Europe in the coming winter (22, 23).
Note added in proof: A similar finding was pub-
lished by Newman et al. (24) during the final re-
vision period of the present study.
REFERENCES AND NOTES
1. R. A. Ebdon, Q. J. R. Meteorol. Soc. 86, 540–542 (1960).
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3. M. P. Baldwin et al., Rev. Geophys. 39, 179–229 (2001).
4. J. M. Wallace, Rev. Geophys. 11, 191 (1973).
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6. U. Niemeier et al., Atmos. Chem. Phys. 9, 9043–9057 (2009).
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8. J. A. Anstey, T. G. Shepherd, Q. J. R. Meteorol. Soc. 140, 1–21
(2014).
9. J. Kidston et al., Nat. Geosci. 8, 433–440 (2015).
10. A. A. Scaife et al., Geophys. Res. Lett. 41, 1752–1758 (2014).
11. B. Naujokat, J. Atmos. Sci. 43, 1873–1877 (1986).
12. R. S. Lindzen, J. R. Holton, J. Atmos. Sci. 25, 1095–1107 (1968).
13. J. R. Holton, R. S. Lindzen, J. Atmos. Sci. 29, 1076–1080(1972).
14. N. Butchart, Rev. Geophys. 52, 157–184 (2014).
15. A. R. Plumb, R. C. Bell, Q. J. R. Meteorol. Soc. 108, 335–352
(1982).
16. R. E. Dickinson, J. Atmos. Sci. 25, 984–1002 (1968).
17. T. J. Dunkerton, Atmos.-Ocean 21, 55–68 (1983).
18. K. Hamilton, A. Hertzog, F. Vial, G. Stenchikov, J. Atmos. Sci.
61, 383–402 (2004).
19. J. S. Kinnersley, S. Pawson, J. Atmos. Sci. 53, 1937–1949 (1996).
20. C. MacLachlan et al., Q. J. R. Meteorol. Soc. 141, 1072–1084
(2015).
21. Y. Kawatani, K. Hamilton, Nature 497, 478–481 (2013).
22. R. A. Ebdon, Aust. Meteorol. Mag. 104, 282–285 (1975).
23. C. Huntingford et al., Nat. Clim. Change 4, 769–777 (2014).
24. P. A. Newman, L. Coy, S. Pawson, L. R. Lait, Geophys. Res. Lett.
10.1002/2016GL070373 (2016).
25. D. P. Dee et al., Q. J. R. Meteorol. Soc. 137, 553–597 (2011).
26. D. G. Andrews, M. E. McIntyre, J. Atmos. Sci. 33, 2031–2048
(1976).
27. NCAS British Atmospheric Data Centre, European Centre for
Medium-Range Weather Forecasts: ECMWF operational
analysis: Assimilated Data (2006); http://catalogue.ceda.ac.
uk/uuid/c46248046f6ce34fc7660a36d9b10a71.
28. E. P. Gerber et al., Bull. Am. Meteorol. Soc. 93, 845–859 (2012).
ACKNOWLEDGMENTS
We thank the European Centre for Medium-Range Weather
Forecasts for providing ERA-Interim and Operational Analysis data
(www.ecmwf.int/en/forecasts) and the Freie Universität Berlin for
providing radiosonde data (www.geo.fu-berlin.de/en/met/ag/
strat/produkte/qbo). The CMIP5 data was obtained from the
British Atmospheric Data Centre (browse.ceda.ac.uk/browse/
badc/cmip5). A summary of data used in the study is listed in
table S1. S.M.O. was supported by UK Natural Environment Research
Council grants NE/M005828/1 and NE/P006779/1. A.A.S., J.R.K.,
and N.B. were supported by the Joint UK Business, Energy and
Industrial Strategy/Defra Met Office Hadley Centre Climate
Programme (GA01101). A.A.S. and J.R.K. were additionally supported
by the EU Seventh Framework Programme SPECS (Seasonal-to-
decadal climate Prediction for the improvement of European Climate
Services) project. We acknowledge the scientific guidance of the
World Climate Research Programme for helping motivate this work,
coordinated under the framework of the Stratosphere-troposphere
Processes and their Role in Climate (SPARC) QBOi activity led by
S.M.O., J.A.A., N.B., and K.H. The analysis of observations and
reanalyses was performed by K.H., C.Z., S.M.O., J.A.A., and N.B.
J.R.K. and A.A.S. provided the analysis of the seasonal forecasts, and
V.S. identified analogous events in global climate model output.
A.A.S. first alerted us to the disruption of the QBO in observational
data. All authors were equally involved in the interpretation of the
results and preparation of the manuscript.
SUPPLEMENTARY MATERIALS
www.sciencemag.org/content/353/6306/1424/suppl/DC1
Table S1
2 July 2016; accepted 29 August 2016
10.1126/science.aah4156
ATMOSPHERIC OXYGEN
A Pleistocene ice core record of
atmospheric O2 concentrations
D. A. Stolper,1
* M. L. Bender,1,2
G. B. Dreyfus,1,3
† Y. Yan,1
J. A. Higgins1
The history of atmospheric O2 partial pressures (PO2) is inextricably linked to the
coevolution of life and Earth’s biogeochemical cycles. Reconstructions of past PO2
rely on models and proxies but often markedly disagree. We present a record of PO2
reconstructed using O2/N2 ratios from ancient air trapped in ice. This record
indicates that PO2 declined by 7 per mil (0.7%) over the past 800,000 years, requiring
that O2 sinks were ~2% larger than sources. This decline is consistent with changes
in burial and weathering fluxes of organic carbon and pyrite driven by either
Neogene cooling or increasing Pleistocene erosion rates. The 800,000-year record of
steady average carbon dioxide partial pressures (PCO2) but declining PO2 provides
distinctive evidence that a silicate weathering feedback stabilizes PCO2 on million-year
time scales.
T
he importance of O2 to biological and geo-
chemical processes has led to a long-standing
interest in reconstructing past atmospheric
O2 partial pressures (PO2, reported at stan-
dard temperature and pressure) (1–12). How-
ever, there is no consensus on the history of
Phanerozoic PO2, with reconstructions disagree-
ing by as much as 0.2 atm, the present-day pres-
sure of O2 in the atmosphere (e.g., 7, 10). Even
over the past million years, it is not known whether
atmospheric O2 concentrations varied or whether
the O2 cycle was in steady state (Fig. 1A). Knowl-
edge of PO2 over the past million years could
provide new insights into the O2 cycle on geologic
time scales and serve as a test for models and
proxies of past PO2. Here we present a primary
record of PO2 over the past 800,000 years, recon-
structed using measured O2/N2 ratios of ancient air
trapped in polar ice.
O2/N2 ratios of this kind have been extensively
used to date ice cores on the basis of the corre-
lation between O2/N2 and local summertime
SCIENCE sciencemag.org 23 SEPTEMBER 2016 • VOL 353 ISSUE 6306 1427
1
Department of Geosciences, Princeton University, Princeton,
NJ 08544, USA. 2
Institute of Oceanology, Shanghai Jiao Tong
University, Shanghai 200240, China. 3
Laboratoire des Sciences
du Climat et de l'Environnement, Gif-sur-Yvettte, France.
*Corresponding author. Email: dstolper@princeton.edu
†Present address: U.S. Department of Energy, Washington, DC
20585, USA.
RESEARCH | REPORTS
onSeptember22,2016http://science.sciencemag.org/Downloadedfrom
insolation (13–17). Despite being directly tied to
atmosphericcompositions,O2/N2 ratioshavenever
before been used to reconstruct past PO2. Landais
et al. (16) and Bazin et al. (17), while using O2/N2
ratios for ice core dating, noted a decline in O2/N2
values with time (i.e., toward the present). They
suggested that this decline could be due to sec-
ular changes in air entrapment processes, gas
loss during core storage, or changes in atmospheric
O2/N2, but they did not evaluate these hypotheses.
Given the potential for O2/N2 ratios to directly
constrain Pleistocene PO2, we present compiled
O2/N2 measurements from multiple ice core re-
cords and evaluate their geochemical implications.
We compiled published O2/N2 ice core records
from Greenland [Greenland Ice Sheet Project 2
(GISP2) (18)] and Antarctica [Vostok (13), Dome
F (14), and Dome C (17); table S1], along with
previously unpublished Antarctic Ar/N2 records
[Vostok and Dome C; table S2]. The data were
treated as follows [see (19) for more details]. (i)
Measured ratios were corrected for gravitational
fractionations and are reported using d notation
dO2=N2 ¼ 1000Â
½O2Š=½N2Šsample
½O2Š=½N2Špreanthropogenic atmosphere
−1
!
ð1Þ
dAr=N2 ¼ 1000Â
½ArŠ=½N2Šsample
½ArŠ=½N2Šmodern atmosphere
−1
!
ð2Þ
where brackets denote concentrations. A decrease
indO2/N2 of1permil(‰)equatestoa0.1%decrease
in PO2 relative to the preanthropogenic atmosphere
(i.e., the modern atmosphere corrected for fossil
fuel combustion). We define the preanthropogenic
atmosphere as having dO2/N2 = 0‰ and dAr/N2 =
0‰. (ii) Only analyses of bubble-free ice with
clathrates were considered. (iii) The portions of
the dO2/N2 and dAr/N2 signals linked to insola-
tion (13–17) were removed (figs. S1 and S2). (iv)
We corrected for differences in bubble close-off
fractionations between ice cores and interlabo-
ratory offsets by assuming that, in the absence of
such effects, trapped gases of a given age share
identical atmospheric O2/N2 and Ar/N2 values
(figs. S3 and S4).
The fully corrected data are plotted versus ice
age in Figs. 1B (dO2/N2) and 2A (dAr/N2). dΟ2/N2
values decrease by 8.4‰ per million years (±0.2,
1s), consistent with the observations of Landais
et al. (16) and Bazin et al. (17). dAr/N2 values in-
crease by 1.6‰ per million years (±0.2, 1s), which
is discussed below.
The decline in dO2/N2 with time could result
from temporal changes in bubble entrapment
processes, effects of ice core storage, a decline in
PO2, or an increase in the partial pressure of atmo-
spheric N2 (PN2). We now evaluate these possi-
bilities in the context of the dO2/N2 record.
dO2/N2 values of gas extracted from ice are ~5
to10‰lowerthanthoseofambientair(13–18,20,21).
Additionally, dAr/N2 covaries with dO2/N2 along
slopes of 0.3 to 0.6 (fig. S5) (19, 21, 22). These
depletions and covariations have been attributed
to fractionations created during bubble close-off
on the basis of measurements and models of firn
air (20, 22) and the covariation of dO2/N2 and
dAr/N2 with local insolation (figs. S1 and S2)
(13–17, 19). If secular changes in bubble close-off
fractionations caused the decline in dO2/N2, then
dAr/N2 values should covary with dO2/N2 along
slopes of 0.3 to 0.6 and thus decline by 2.5 to 5.0‰
per million years. Instead, dAr/N2 increases with
time by 1.6‰ per million years (±0.2, 1s; Fig. 2A).
The increasing trend is largely due to a subset of
Vostok data from 330,000- to 370,000-year-old ice
that is lower in dAr/N2 by ~1‰ compared with
younger data. Exclusion of this subset yields an
increase in dAr/N2 with time of only 0.35‰ (±0.20,
1s), within the 2s error range of no change. Re-
gardless, whichever way the dAr/N2 are ana-
lyzed, they are inconsistent with the decline in
dO2/N2 being caused by bubble close-off pro-
cesses (Fig. 2A).
Ice core storage, under some conditions, causes
the dO2/N2 values of trapped gases to decline
(14–17). Thus, the second possibility that we con-
sider is that ice core storage lowered the dO2/N2
values so that the slope observed in Fig. 1 is an
artifact. For example, a change in dO2/N2 cor-
related with ice age but unrelated to atmospheric
compositions could result if the retention of O2
versus N2 during storage is a function of pre-
coring properties controlled by original ice depths
(e.g., in situ temperature, pressure, or clathrate
size). We evaluate this possibility by using three
approaches. (i) Gas loss during core storage causes
dAr/N2 todeclineathalftherateofdO2/N2 (21,23,24).
However, as discussed above, the dAr/N2 values
are not consistent with such a change (Fig. 2A).
(ii) Because some ice properties (e.g., temperature
and pressure) can vary linearly with ice depth,
we tested whether the Dome C dO2/N2 data are
better fit by a linear relationship when plotted
against ice age or depth. We note that only the
Dome C ice core’s age-depth relationship is suffi-
ciently curvilinear for this test to be useful. We
linearly regressed both age and depth against
1428 23 SEPTEMBER 2016 • VOL 353 ISSUE 6306 sciencemag.org SCIENCE
O2/N2(‰)
age (kyr)age (kyr)
-4
-2
0
2
4
6
8
10
-4
-2
0
2
4
6
8
10
0 600400200 800
Dome F
Vostok
Dome C
Best-fit line:
Slope = 8.4 ‰/myr (±0.2, 1 )
20.95
21.03
21.12
20.87
PO2(100xatm)
GISP2
-15
-10
-5
0
5
10
15
20
25
30
0 200 400 600 800000 200200200 400400400 600600600 800800800
Glasspool and Scott (2010) [11]
Falkowski et al. (2005) [7]
ice core data
best-fit line
Kump and Garrels (1986) [1]
Shackleton (1987) [2]
Berner and Canfield (1989) [3]
Derry and France-Lanord (1996) [4]
Tappert et al. (2013) [12]
Hansen and Wallmann (2003) [5]
Bergman et al. (2004) [6]
Arvidson et al. (2006) [8]
Berner (2006) [9]
Berner (2009) [10]
20.95
21.16
21.37
20.74
PO2(100xatm)
21.58
O2/N2(‰)
[2]
[9]
[7]
[6]
best-fit
line
[1]
[11]
[5]
[4]
[12]
[3]
[8]
[10]
Fig. 1. dO2/N2 and PO2 values versus age from ice cores and from model and proxy predictions. (A) Comparison of the ice core data with model and
proxy predictions (1–12). (B) dO2/N2 versus ice age from ice cores. dO2/N2 decreases by 8.4‰ per million years (±0.2, 1s). Gray bands are 95% confidence
intervals. Data are corrected for gravitational, interlaboratory, and bubble close-off fractionations (19). kyr, thousand years; myr, million years.
RESEARCH | REPORTS
onSeptember22,2016http://science.sciencemag.org/Downloadedfrom
dO2/N2 for ice older than ~400,000 years (i.e.,
deeper than 2600 m) and extrapolated the fits to
younger ages and shallower depths. The extrap-
olation forage(Fig. 2B)passesthrough the younger
data, whereas the extrapolation for depth (Fig. 2C)
misses the shallower data (by >4s). (iii) Repeat
dO2/N2 measurements of Vostok ice from the same
age interval (150,000 to 450,000 years ago) made
10 years apart (13, 15) differ onaverage by 6‰, with
longer storage leading to lower dO2/N2. Despite
this, regressing dO2/N2 against time yields statisti-
cally identical (within 1s) slopes of dO2/N2 versus
age for both data sets (fig. S6).
Collectively, the data and tests presented above
provide no support for the observed decrease in
dO2/N2 over time being an artifact of either bubble
close-off processes as they are currently under-
stood or ice core storage. Consequently, we hy-
pothesize and proceed with the interpretation
that the observed decline in dO2/N2 reflects changes
in PO2 or PN2. Because N2 has a billion-year at-
mosphericlifetime(25),welinkthedeclineindO2/N2
with time exclusively to a decline in PO2. Our
hypothesis is further supported by the observa-
tion that data from all four ice cores individually
exhibit the same general trends and magnitudes
of decreasing dO2/N2 with time (table S3), even
though each was drilled, stored, and analyzed
differently.
The question raised by this record is why PO2
has decreased by ~7‰ over the past 800,000 years.
Changes in PO2 require imbalances between
O2 sources [dominantly modern sedimentary
organic carbon (Corg) and pyrite burial] and sinks
(dominantly ancient sedimentary Corg and pyrite
oxidation) (26). Thus, a higher rate of oxidative
weathering relative to Corg and/or pyrite burial
over the past million years could
have caused the observed PO2 de-
cline. The ~2-million-year (+1.5/
–0.5 million years) (26) geological
residence time of O2, combined
with the decline in dO2/N2 of
8.4‰ per million years, indicates
that O2 sinks were 1.7% larger than
sources over the past 800,000 years
(27). We now explore possible causes
for this drawdown, examining first
the impact of changing erosion rates
and second the impact of global
cooling on PO2.
Global erosion rates influence
the amount of rock weathered (con-
suming O2) and sediment buried
(releasing O2). These rates have
been suggested to have increased
up to 100% in the Pleistocene rel-
ative to the Pliocene (28) [though
this is debated (29)]. Thus, the pos-
sibility exists that increased Pleisto-
cene sedimentary erosion and burial
rates affected PO2 levels. Indeed,
Torres et al. (30) modeled that in-
creasing erosion rates over the past
15 million years enhanced oxida-
tion of sedimentary pyrite rela-
tive to burial so that PO2 declined
on average by 9 to 25‰ per million years. This is
similar to the decline given by the ice core record
(8.4‰ per million years). We note that whether
increasing erosion rates cause PO2 to decline
(instead of increase) is unknown (31).
Large increases (e.g., 100%) in Pleistocene ero-
sion rates, if they did occur, likely would have
required processes that keep O2 sources and sinks
balanced within ~2% (the observed imbalance).
Such processes could include the proposed PO2-
dependent control of Corg burial fluxes on sedimen-
tary phosphorus burial rates (32). Alternatively,
sedimentary mineral surface area is known to
positively correlate with total sedimentary Corg and
pyrite content (33). Hedges and Kiel (33) pro-
posed that the total eroded and total buried min-
eral surface areas today are about equal. If this
was true in the past, the conservation of eroded
versus newly generated mineral surface area may
have acted to balance Corg and pyrite weathering
and burial fluxes (and thus O2 fluxes), regardless of
global erosion rates (33).
Alternatively, on the basis of 13
C/12
C and 18
O/16
O
records from sedimentary carbonates, Shackleton
(2) proposed that PO2 declined over the Neogene as
a result of oceaniccooling. He suggestedthefollowing
feedback loop: Cooling increases O2 solubility. This
raises dissolved O2 concentrations, which increases
the volume of ocean sediment exposed to dissolved
O2 and thus also increases global aerobic Corg
remineralization rates (33). On million-year time
scales, Corg burial rates and, therefore, PO2 and O2
concentrations decline until seawater O2 concen-
trations return to their initial (precooling) levels. At
this new steady state, Corg burial rates have returned
to their original values, but PO2 is stabilized at a
lower value.
Shackleton’s hypothesis can be evaluated to first
order in the context of the dO2/N2 data by using
records of past ocean temperature. Specifically,
temperatures in the deep (>1000 m depth) ocean
were roughly constant from 24 to 14 million years
ago (34, 35). Assuming an O2 residence time of ~2
million years and the hypothesis that changes in
ocean temperature modulate PO2, then O2 sources
and sinks would have been in balance by 14 million
years ago. The oceans have cooled on average by
0.3°C per million years over the past 14 million
years and 0.5° to 1.1°C per million years over the
past 5 million years (34, 35). Cooling of 0.3° to 1.1°C
per million years increases O2 solubility by ~7 to
25‰ per million years (36). If dissolved O2 con-
centrations remained constant (as this hypothesis
requires), such changes in O2 solubility necessitate
a decline in PO2 of ~7 to 25‰ per million years.
These rates bracket the rate of decline given by the
ice core record (8.4‰ per million years; Fig. 1A).
We note that deep ocean cooling rates track aver-
age marine cooling rates, but not precisely, because
modern deep waters form in and thus reflect the
temperatures of high latitudes. Regardless, the
critical point is that this simple calculation is
consistent with the ice core–derived dO2/N2
record and supports the hypothesis that global
temperature stabilizes PO2 on geological time
scales through feedbacks associated with Corg
burial rates.
A drop in PO2 over the past 800,000 years due
solely to changes in Corg burial versus oxidation
rates (regardless of the cause) requires positive
CO2 fluxes (~3 × 1011
moles C per year) into the
ocean and atmosphere (19). However, ice core
records of past carbon dioxide partial pressures
(PCO2) show no obvious change in the mean over
SCIENCE sciencemag.org 23 SEPTEMBER 2016 • VOL 353 ISSUE 6306 1429
age (kyr) age (kyr)
-5-5
00
55
1010
00 200200 400400 600600 800800
-5
0
5
10
0 200 400 600 800
O2/N2, all Ar/N2, Vostok
Ar/N2, Dome C
best-fit
O2/N2 line
Expected range of
Ar/N2 trends if
O2/N2 is controlled
by bubble close-off
fractionations or gas
loss
best-fit
Ar/N2 line
-5
0
5
10
100 450 800
-5-5-5
000
555
101010
100100100 450450450 800800800
-10
-10
-5
0
5
10
1400 2300 3200
depth (m)
-10-10-10
-5-5-5-5
0000
5555
10101010
1400140014001400 2300230023002300 3200320032003200
-5
0
5
10
100 450 800
O2/N2(‰)O2/N2(‰)
(‰)
Fig. 2. Evidence that the observed decline in dO2N2 with time does not originate from either secular changes in
bubble close-off fractionations or ice core storage. (A) dAr/N2 and dO2/N2 versus ice age. Bubble close-off processes
and gas loss would cause dAr/N2 and dO2/N2 to covary with slopes of 0.3 to 0.6. The observed dAr/N2 trend does not
overlap with these expected trends (orange wedge), indicating that such processes did not cause the decline in dO2/N2.
(B) Dome C dO2/N2 versus ice age and (C) versus depth. Dotted lines were fit to ice >400,000 years old or >2600 m deep and
extrapolated to younger ages or shallower depths. Extrapolations of the fits pass through the younger data (B) but miss the
deeper data [beyond 4s (C)], indicating depth-dependent glacial properties did not cause the decline in dO2/N2. Gray bands
are 95% confidence intervals. Data are corrected for gravitational, interlaboratory, and bubble close-off fractionations (19).
RESEARCH | REPORTS
onSeptember22,2016http://science.sciencemag.org/Downloadedfrom
the past 800,000 years (37–39) (Fig. 3). To under-
stand how changes in PO2 influence PCO2, we de-
veloped a simple model of the carbon cycle that
allows for changes in weathering and burial rates
of carbonates, Corg, and silicates (19). In the ab-
sence of any PCO2-dependent feedbacks, a constant
decline in dO2/N2 of 8.4‰ over the past million
years from a net imbalance in Corg fluxes causes
PCO2 to rise by ~140 parts per million over the same
time frame. Such a rise is inconsistent with the
PCO2 record (Fig. 3). A PCO2-dependent silicate
weathering feedback (40) can account for the
higher CO2 flux if silicate weathering is enhanced
by ~6% relative to volcanic outgassing. For exam-
ple, response times for silicate weathering of
200,000 to 500,000 years (41) stabilize PCO2 levels
within ~1 million years (Fig. 3).
Changes in Cenozoic climate began millions
of years before the start of our ice core–based
dO2/N2 record 800,000 years ago (e.g., 2, 30, 34, 35).
Thus, we suggest that modest enhancements
in silicate weathering would already have stabi-
lized the portion of the PCO2 ice core record
that is controlled by differences in Corg and
pyrite burial and oxidation. Thus, the combina-
tion of changing PO2 and constant average PCO2
provides distinctive evidence for feedbacks that
regulate PCO2 on geologic time scales (37). Last-
ly, a 2% imbalance in O2 fluxes results in only
a ~0.1‰ shift in the 13
C/12
C ratio of buried
carbon (19).
Our results provide a primary record of declin-
ing PO2 over the past 800,000 years sustained by a
~2% imbalance between O2 sources and sinks.
Critically, this decline is consistent with previously
proposed and relatively simple models that invoke
either the effects of increased Pleistocene erosion
rates or decreased ocean temperature to explain
feedbacks in the global cycles of carbon, sulfur, and
O2—and the effects of both could have contributed
to the observed decline in PO2. Regardless, creat-
ing primary records of past PO2 is the necessary
first step in identifying the fundamental processes
that regulate PO2 on geological time scales. Given
evidence that both global erosion rates and
temperature have changed markedly over the
Cenozoic (42), the ideas presented here may have
implications for the history of PO2 beyond the
Pleistocene.
REFERENCES AND NOTES
1. L. R. Kump, R. M. Garrels, Am. J. Sci. 286, 337–360
(1986).
2. N. Shackleton, Geol. Soc. Lond. Spec. Publ. 26, 423–434
(1987).
3. R. A. Berner, D. E. Canfield, Am. J. Sci. 289, 333–361
(1989).
4. L. A. Derry, C. France-Lanord, Paleoceanography 11, 267–275
(1996).
5. K. W. Hansen, K. Wallmann, Am. J. Sci. 303, 94–148
(2003).
6. N. M. Bergman, T. M. Lenton, A. J. Watson, Am. J. Sci. 304,
397–437 (2004).
7. P. G. Falkowski et al., Science 309, 2202–2204 (2005).
8. R. S. Arvidson, F. T. Mackenzie, M. Guidry, Am. J. Sci. 306,
135–190 (2006).
9. R. A. Berner, Geochim. Cosmochim. Acta 70, 5653–5664
(2006).
10. R. A. Berner, Am. J. Sci. 309, 603–606 (2009).
11. I. J. Glasspool, A. C. Scott, Nat. Geosci. 3, 627–630
(2010).
12. R. Tappert et al., Geochim. Cosmochim. Acta 121, 240–262
(2013).
13. M. L. Bender, Earth Planet. Sci. Lett. 204, 275–289
(2002).
14. K. Kawamura et al., Nature 448, 912–916 (2007).
15. M Suwa, M. L. Bender, Quat. Sci. Rev. 27, 1093–1106
(2008).
16. A. Landais et al., Clim. Past 8, 191–203 (2012).
17. L. Bazin et al., Clim. Past 12, 729–748 (2016).
18. M. E. Smith, thesis, Princeton University, Princeton, NJ
(1998).
19. Materials and methods are available as supplementary
materials on Science Online.
20. M. Battle et al., Nature 383, 231 (1996).
21. M. Bender, T. Sowers, V. Lipenkov, J. Geophys. Res. Atmos.
100, 18651–18660 (1995).
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(2015).
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K. Taylor, E. J. Brook, Science 324, 1431–1434 (2009).
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(1988).
25. R. A. Berner, Geology 34, 413–415 (2006).
26. H. D. Holland, Geochim. Cosmochim. Acta 66, 3811–3826
(2002).
27. The imbalance is calculated as follows: The total imbalance
(moles per million years) for O2 is 0.0084 × nO2, where
nO2 is the total number of moles of O2 in the atmosphere.
The O2 flux is nO2 divided by its residence time. The
residence time of O2 is about 2 million years. The percent
imbalance is the total imbalance divided by the total flux,
or 0.0084nO2/(nO2/2) = 0.017 (1.7%).
28. F. Herman et al., Nature 504, 423–426 (2013).
29. J. K. Willenbring, F. von Blanckenburg, Nature 465, 211–214
(2010).
30. M. A. Torres, A. J. West, G. Li, Nature 507, 346–349
(2014).
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406–407 (1997).
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(1996).
33. J. I. Hedges, R. G. Keil, Mar. Chem. 49, 81–115 (1995).
34. C. H. Lear, H. Elderfield, P. A. Wilson, Science 287, 269–272
(2000).
35. B. Cramer, K. Miller, P. Barrett, J. Wright, J. Geophys. Res.
Oceans 116, C12023 (2011).
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(1992).
37. R. E. Zeebe, K. Caldeira, Nat. Geosci. 1, 312–315
(2008).
38. B. Bereiter et al., Geophys. Res. Lett. 42, 542–549
(2015).
39. J. A. Higgins et al., Proc. Natl. Acad. Sci. U.S.A. 112, 6887–6891
(2015).
40. J. C. Walker, P. Hays, J. Kasting, J. Geophys. Res. 86,
9776–9782 (1981).
41. D. Archer, J. Geophys. Res. Oceans 110, C09S05 (2005).
42. M. Raymo, W. F. Ruddiman, Nature 359, 117–122 (1992).
ACKNOWLEDGMENTS
D.A.S. acknowledges funding from a National Oceanic and
Atmospheric Administration Climate & Global Change
postdoctoral fellowship. J.A.H. and M.L.B. acknowledge
support from National Science Foundation grant ANT-1443263.
All data presented are available in the supplementary
materials. We thank W. Fischer, I. Halevy, N. Planavsky,
J. Severinghaus, and D. Sigman for helpful discussions and
three anonymous reviewers for helpful comments on the
manuscript. D.A.S., J.A.H., and M.L.B. conceived the study
and wrote the manuscript. D.A.S., J.A.H., M.L.B., and Y.Y.
analyzed the data. G.B.D. measured the Dome C dAr/N2 data.
The views expressed in this article are those of the authors
and do not necessarily represent the views of the Department
of Energy or the U.S. Government.
SUPPLEMENTARY MATERIALS
www.sciencemag.org/content/353/6306/1427/suppl/DC1
Materials and Methods
Figs. S1 to S6
Tables S1 to S3
References (43–78)
25 February 2016; accepted 2 August 2016
10.1126/science.aaf5445
1430 23 SEPTEMBER 2016 • VOL 353 ISSUE 6306 sciencemag.org SCIENCE
Fig. 3. Comparison
of calculated and
measured PCO2
values due to declin-
ing PO2 with and
without a PCO2-
dependent silicate
weathering feed-
back. Inclusion of a
silicate weathering
feedback with geolog-
ically reasonable
response times
[200,000 to 500,000
years (41)] stabilizes
PCO2 within ~1 million
years. Thus, increased
silicate weathering
rates could have
compensated for
enhanced CO2 fluxes
from increased net
Corg oxidation more
than 800,000 years
ago. The PCO2 records
are continuous only
from 800,000 years
to the present. The model used to calculate PCO2 values is described in (19); the measured PCO2
values are from (38) and (39). ppm, parts per million.
150150
200200
250250
300300
350350
400400
00 200200 400400 600600 800800 10001000
150
200
250
300
350
400
0 200 400 600 800 1000
age (kyr)
PCO
2
(ppm)
ice core data
No PCO2-dependent silicate weathering feedback
500-kyr response time for PCO2-dependent silicate weathering feedback
400-kyr response time for PCO2-dependent silicate weathering feedback
300-kyr response time for PCO2-dependent silicate weathering feedback
200-kyr response time for PCO2-dependent silicate weathering feedback
No PCO2-dependent silicate weathering feedback
results in changes in PCO2 inconsistent with measured
ice core records.
A PCO2-dependent silicate weathering feedback stabilizes PCO2 within ~1 million
years following the creation of an imbalance in Corg burial versus weathering rates.
RESEARCH | REPORTS
onSeptember22,2016http://science.sciencemag.org/Downloadedfrom
(6306), 1427-1430. [doi: 10.1126/science.aaf5445]353Science
Higgins (September 22, 2016)
D. A. Stolper, M. L. Bender, G. B. Dreyfus, Y. Yan and J. A.
concentrations2A Pleistocene ice core record of atmospheric O
Editor's Summary
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Атмосфера Земли медленно теряет кислород

  • 1. deliver westward acceleration to the mean flow. Furthermore, the stronger tropical upwelling dur- ing Boreal winter slows down the QBO’s descent, allowing more time for the extratropical waves to impact during this particular phase. Of course, it is also possible that our current numerical models can not properly represent the processes disrupting the QBO. To investigate this, the foregoing RMS analysis that was applied to the observational record was applied to his- torical global climate model runs so as to identify possible analogous events (Fig. 4, A to C). Among the available models that produce a QBO inter- nally, only one rarely produced behavior similar totheobserveddisruption, withanexampleshown in Fig. 4D. The extreme profiles resemble those observed during 2016 with a thin layer of west- ward wind appearing within an otherwise east- ward QBO phase. What will happen next? The recent disruption of the QBO is a rare event that occurs in the northern winter. The forecast initialized after the disruption (Fig. 3B) suggests that the QBO will return to more regular phase progression over the coming year. The westward jet that suddenly appeared in the lower stratosphere is predicted to amplify in the summer of 2016 and progress downward with time. Eastward flow then descends from the 20-hPa level and dominates the lower stratospheric flow toward the end of 2016, returning the QBO to its typical behavior. We then expect regular and predictable QBO cycling to continue from 2017, as occurs in the available climate models (Fig. 4D). Nonetheless, as the climate warms in the future, climate models that simulate these events suggest that similar dis- ruptions will occur up to three times every 100 years for the more extreme of the standard climate change scenarios. This is consistent with a pro- jected strengthening of the Brewer-Dobson cir- culation due to increasing stratospheric wave activity (14) and the recently observed weakening of the QBO amplitude in the lower stratosphere (21) under climate change. However, robustly modeling how the QBO and its underlying pro- cesses and external influences will change in the future remains elusive. There is a further outcome of the 2016 dis- ruption of the QBO. After an eastward QBO at the onset of the 2015–2016 winter, the QBO at the onset of the coming winter of 2016–2017 was expected to be westward. The disruption of early 2016 means that an eastward QBO phase is now again expected in the lower stratosphere. Because of the expected QBO influence on the Atlantic jet stream, this increases the risk of a strong jet, winter storms, and heavy rainfall over northern Europe in the coming winter (22, 23). Note added in proof: A similar finding was pub- lished by Newman et al. (24) during the final re- vision period of the present study. REFERENCES AND NOTES 1. R. A. Ebdon, Q. J. R. Meteorol. Soc. 86, 540–542 (1960). 2. R. J. Reed, W. J. Campbell, L. A. Rasmussen, D. G. Rogers, J. Geophys. Res. 66, 813–818 (1961). 3. M. P. Baldwin et al., Rev. Geophys. 39, 179–229 (2001). 4. J. M. Wallace, Rev. Geophys. 11, 191 (1973). 5. P. H. Haynes, Q. J. R. Meteorol. Soc. 124, 2645–2670 (1998). 6. U. Niemeier et al., Atmos. Chem. Phys. 9, 9043–9057 (2009). 7. J. R. Holton, H.-C. Tan, J. Atmos. Sci. 37, 2200–2208 (1980). 8. J. A. Anstey, T. G. Shepherd, Q. J. R. Meteorol. Soc. 140, 1–21 (2014). 9. J. Kidston et al., Nat. Geosci. 8, 433–440 (2015). 10. A. A. Scaife et al., Geophys. Res. Lett. 41, 1752–1758 (2014). 11. B. Naujokat, J. Atmos. Sci. 43, 1873–1877 (1986). 12. R. S. Lindzen, J. R. Holton, J. Atmos. Sci. 25, 1095–1107 (1968). 13. J. R. Holton, R. S. Lindzen, J. Atmos. Sci. 29, 1076–1080(1972). 14. N. Butchart, Rev. Geophys. 52, 157–184 (2014). 15. A. R. Plumb, R. C. Bell, Q. J. R. Meteorol. Soc. 108, 335–352 (1982). 16. R. E. Dickinson, J. Atmos. Sci. 25, 984–1002 (1968). 17. T. J. Dunkerton, Atmos.-Ocean 21, 55–68 (1983). 18. K. Hamilton, A. Hertzog, F. Vial, G. Stenchikov, J. Atmos. Sci. 61, 383–402 (2004). 19. J. S. Kinnersley, S. Pawson, J. Atmos. Sci. 53, 1937–1949 (1996). 20. C. MacLachlan et al., Q. J. R. Meteorol. Soc. 141, 1072–1084 (2015). 21. Y. Kawatani, K. Hamilton, Nature 497, 478–481 (2013). 22. R. A. Ebdon, Aust. Meteorol. Mag. 104, 282–285 (1975). 23. C. Huntingford et al., Nat. Clim. Change 4, 769–777 (2014). 24. P. A. Newman, L. Coy, S. Pawson, L. R. Lait, Geophys. Res. Lett. 10.1002/2016GL070373 (2016). 25. D. P. Dee et al., Q. J. R. Meteorol. Soc. 137, 553–597 (2011). 26. D. G. Andrews, M. E. McIntyre, J. Atmos. Sci. 33, 2031–2048 (1976). 27. NCAS British Atmospheric Data Centre, European Centre for Medium-Range Weather Forecasts: ECMWF operational analysis: Assimilated Data (2006); http://catalogue.ceda.ac. uk/uuid/c46248046f6ce34fc7660a36d9b10a71. 28. E. P. Gerber et al., Bull. Am. Meteorol. Soc. 93, 845–859 (2012). ACKNOWLEDGMENTS We thank the European Centre for Medium-Range Weather Forecasts for providing ERA-Interim and Operational Analysis data (www.ecmwf.int/en/forecasts) and the Freie Universität Berlin for providing radiosonde data (www.geo.fu-berlin.de/en/met/ag/ strat/produkte/qbo). The CMIP5 data was obtained from the British Atmospheric Data Centre (browse.ceda.ac.uk/browse/ badc/cmip5). A summary of data used in the study is listed in table S1. S.M.O. was supported by UK Natural Environment Research Council grants NE/M005828/1 and NE/P006779/1. A.A.S., J.R.K., and N.B. were supported by the Joint UK Business, Energy and Industrial Strategy/Defra Met Office Hadley Centre Climate Programme (GA01101). A.A.S. and J.R.K. were additionally supported by the EU Seventh Framework Programme SPECS (Seasonal-to- decadal climate Prediction for the improvement of European Climate Services) project. We acknowledge the scientific guidance of the World Climate Research Programme for helping motivate this work, coordinated under the framework of the Stratosphere-troposphere Processes and their Role in Climate (SPARC) QBOi activity led by S.M.O., J.A.A., N.B., and K.H. The analysis of observations and reanalyses was performed by K.H., C.Z., S.M.O., J.A.A., and N.B. J.R.K. and A.A.S. provided the analysis of the seasonal forecasts, and V.S. identified analogous events in global climate model output. A.A.S. first alerted us to the disruption of the QBO in observational data. All authors were equally involved in the interpretation of the results and preparation of the manuscript. SUPPLEMENTARY MATERIALS www.sciencemag.org/content/353/6306/1424/suppl/DC1 Table S1 2 July 2016; accepted 29 August 2016 10.1126/science.aah4156 ATMOSPHERIC OXYGEN A Pleistocene ice core record of atmospheric O2 concentrations D. A. Stolper,1 * M. L. Bender,1,2 G. B. Dreyfus,1,3 † Y. Yan,1 J. A. Higgins1 The history of atmospheric O2 partial pressures (PO2) is inextricably linked to the coevolution of life and Earth’s biogeochemical cycles. Reconstructions of past PO2 rely on models and proxies but often markedly disagree. We present a record of PO2 reconstructed using O2/N2 ratios from ancient air trapped in ice. This record indicates that PO2 declined by 7 per mil (0.7%) over the past 800,000 years, requiring that O2 sinks were ~2% larger than sources. This decline is consistent with changes in burial and weathering fluxes of organic carbon and pyrite driven by either Neogene cooling or increasing Pleistocene erosion rates. The 800,000-year record of steady average carbon dioxide partial pressures (PCO2) but declining PO2 provides distinctive evidence that a silicate weathering feedback stabilizes PCO2 on million-year time scales. T he importance of O2 to biological and geo- chemical processes has led to a long-standing interest in reconstructing past atmospheric O2 partial pressures (PO2, reported at stan- dard temperature and pressure) (1–12). How- ever, there is no consensus on the history of Phanerozoic PO2, with reconstructions disagree- ing by as much as 0.2 atm, the present-day pres- sure of O2 in the atmosphere (e.g., 7, 10). Even over the past million years, it is not known whether atmospheric O2 concentrations varied or whether the O2 cycle was in steady state (Fig. 1A). Knowl- edge of PO2 over the past million years could provide new insights into the O2 cycle on geologic time scales and serve as a test for models and proxies of past PO2. Here we present a primary record of PO2 over the past 800,000 years, recon- structed using measured O2/N2 ratios of ancient air trapped in polar ice. O2/N2 ratios of this kind have been extensively used to date ice cores on the basis of the corre- lation between O2/N2 and local summertime SCIENCE sciencemag.org 23 SEPTEMBER 2016 • VOL 353 ISSUE 6306 1427 1 Department of Geosciences, Princeton University, Princeton, NJ 08544, USA. 2 Institute of Oceanology, Shanghai Jiao Tong University, Shanghai 200240, China. 3 Laboratoire des Sciences du Climat et de l'Environnement, Gif-sur-Yvettte, France. *Corresponding author. Email: dstolper@princeton.edu †Present address: U.S. Department of Energy, Washington, DC 20585, USA. RESEARCH | REPORTS onSeptember22,2016http://science.sciencemag.org/Downloadedfrom
  • 2. insolation (13–17). Despite being directly tied to atmosphericcompositions,O2/N2 ratioshavenever before been used to reconstruct past PO2. Landais et al. (16) and Bazin et al. (17), while using O2/N2 ratios for ice core dating, noted a decline in O2/N2 values with time (i.e., toward the present). They suggested that this decline could be due to sec- ular changes in air entrapment processes, gas loss during core storage, or changes in atmospheric O2/N2, but they did not evaluate these hypotheses. Given the potential for O2/N2 ratios to directly constrain Pleistocene PO2, we present compiled O2/N2 measurements from multiple ice core re- cords and evaluate their geochemical implications. We compiled published O2/N2 ice core records from Greenland [Greenland Ice Sheet Project 2 (GISP2) (18)] and Antarctica [Vostok (13), Dome F (14), and Dome C (17); table S1], along with previously unpublished Antarctic Ar/N2 records [Vostok and Dome C; table S2]. The data were treated as follows [see (19) for more details]. (i) Measured ratios were corrected for gravitational fractionations and are reported using d notation dO2=N2 ¼ 1000Â ½O2Š=½N2Šsample ½O2Š=½N2Špreanthropogenic atmosphere −1 ! ð1Þ dAr=N2 ¼ 1000Â ½ArŠ=½N2Šsample ½ArŠ=½N2Šmodern atmosphere −1 ! ð2Þ where brackets denote concentrations. A decrease indO2/N2 of1permil(‰)equatestoa0.1%decrease in PO2 relative to the preanthropogenic atmosphere (i.e., the modern atmosphere corrected for fossil fuel combustion). We define the preanthropogenic atmosphere as having dO2/N2 = 0‰ and dAr/N2 = 0‰. (ii) Only analyses of bubble-free ice with clathrates were considered. (iii) The portions of the dO2/N2 and dAr/N2 signals linked to insola- tion (13–17) were removed (figs. S1 and S2). (iv) We corrected for differences in bubble close-off fractionations between ice cores and interlabo- ratory offsets by assuming that, in the absence of such effects, trapped gases of a given age share identical atmospheric O2/N2 and Ar/N2 values (figs. S3 and S4). The fully corrected data are plotted versus ice age in Figs. 1B (dO2/N2) and 2A (dAr/N2). dΟ2/N2 values decrease by 8.4‰ per million years (±0.2, 1s), consistent with the observations of Landais et al. (16) and Bazin et al. (17). dAr/N2 values in- crease by 1.6‰ per million years (±0.2, 1s), which is discussed below. The decline in dO2/N2 with time could result from temporal changes in bubble entrapment processes, effects of ice core storage, a decline in PO2, or an increase in the partial pressure of atmo- spheric N2 (PN2). We now evaluate these possi- bilities in the context of the dO2/N2 record. dO2/N2 values of gas extracted from ice are ~5 to10‰lowerthanthoseofambientair(13–18,20,21). Additionally, dAr/N2 covaries with dO2/N2 along slopes of 0.3 to 0.6 (fig. S5) (19, 21, 22). These depletions and covariations have been attributed to fractionations created during bubble close-off on the basis of measurements and models of firn air (20, 22) and the covariation of dO2/N2 and dAr/N2 with local insolation (figs. S1 and S2) (13–17, 19). If secular changes in bubble close-off fractionations caused the decline in dO2/N2, then dAr/N2 values should covary with dO2/N2 along slopes of 0.3 to 0.6 and thus decline by 2.5 to 5.0‰ per million years. Instead, dAr/N2 increases with time by 1.6‰ per million years (±0.2, 1s; Fig. 2A). The increasing trend is largely due to a subset of Vostok data from 330,000- to 370,000-year-old ice that is lower in dAr/N2 by ~1‰ compared with younger data. Exclusion of this subset yields an increase in dAr/N2 with time of only 0.35‰ (±0.20, 1s), within the 2s error range of no change. Re- gardless, whichever way the dAr/N2 are ana- lyzed, they are inconsistent with the decline in dO2/N2 being caused by bubble close-off pro- cesses (Fig. 2A). Ice core storage, under some conditions, causes the dO2/N2 values of trapped gases to decline (14–17). Thus, the second possibility that we con- sider is that ice core storage lowered the dO2/N2 values so that the slope observed in Fig. 1 is an artifact. For example, a change in dO2/N2 cor- related with ice age but unrelated to atmospheric compositions could result if the retention of O2 versus N2 during storage is a function of pre- coring properties controlled by original ice depths (e.g., in situ temperature, pressure, or clathrate size). We evaluate this possibility by using three approaches. (i) Gas loss during core storage causes dAr/N2 todeclineathalftherateofdO2/N2 (21,23,24). However, as discussed above, the dAr/N2 values are not consistent with such a change (Fig. 2A). (ii) Because some ice properties (e.g., temperature and pressure) can vary linearly with ice depth, we tested whether the Dome C dO2/N2 data are better fit by a linear relationship when plotted against ice age or depth. We note that only the Dome C ice core’s age-depth relationship is suffi- ciently curvilinear for this test to be useful. We linearly regressed both age and depth against 1428 23 SEPTEMBER 2016 • VOL 353 ISSUE 6306 sciencemag.org SCIENCE O2/N2(‰) age (kyr)age (kyr) -4 -2 0 2 4 6 8 10 -4 -2 0 2 4 6 8 10 0 600400200 800 Dome F Vostok Dome C Best-fit line: Slope = 8.4 ‰/myr (±0.2, 1 ) 20.95 21.03 21.12 20.87 PO2(100xatm) GISP2 -15 -10 -5 0 5 10 15 20 25 30 0 200 400 600 800000 200200200 400400400 600600600 800800800 Glasspool and Scott (2010) [11] Falkowski et al. (2005) [7] ice core data best-fit line Kump and Garrels (1986) [1] Shackleton (1987) [2] Berner and Canfield (1989) [3] Derry and France-Lanord (1996) [4] Tappert et al. (2013) [12] Hansen and Wallmann (2003) [5] Bergman et al. (2004) [6] Arvidson et al. (2006) [8] Berner (2006) [9] Berner (2009) [10] 20.95 21.16 21.37 20.74 PO2(100xatm) 21.58 O2/N2(‰) [2] [9] [7] [6] best-fit line [1] [11] [5] [4] [12] [3] [8] [10] Fig. 1. dO2/N2 and PO2 values versus age from ice cores and from model and proxy predictions. (A) Comparison of the ice core data with model and proxy predictions (1–12). (B) dO2/N2 versus ice age from ice cores. dO2/N2 decreases by 8.4‰ per million years (±0.2, 1s). Gray bands are 95% confidence intervals. Data are corrected for gravitational, interlaboratory, and bubble close-off fractionations (19). kyr, thousand years; myr, million years. RESEARCH | REPORTS onSeptember22,2016http://science.sciencemag.org/Downloadedfrom
  • 3. dO2/N2 for ice older than ~400,000 years (i.e., deeper than 2600 m) and extrapolated the fits to younger ages and shallower depths. The extrap- olation forage(Fig. 2B)passesthrough the younger data, whereas the extrapolation for depth (Fig. 2C) misses the shallower data (by >4s). (iii) Repeat dO2/N2 measurements of Vostok ice from the same age interval (150,000 to 450,000 years ago) made 10 years apart (13, 15) differ onaverage by 6‰, with longer storage leading to lower dO2/N2. Despite this, regressing dO2/N2 against time yields statisti- cally identical (within 1s) slopes of dO2/N2 versus age for both data sets (fig. S6). Collectively, the data and tests presented above provide no support for the observed decrease in dO2/N2 over time being an artifact of either bubble close-off processes as they are currently under- stood or ice core storage. Consequently, we hy- pothesize and proceed with the interpretation that the observed decline in dO2/N2 reflects changes in PO2 or PN2. Because N2 has a billion-year at- mosphericlifetime(25),welinkthedeclineindO2/N2 with time exclusively to a decline in PO2. Our hypothesis is further supported by the observa- tion that data from all four ice cores individually exhibit the same general trends and magnitudes of decreasing dO2/N2 with time (table S3), even though each was drilled, stored, and analyzed differently. The question raised by this record is why PO2 has decreased by ~7‰ over the past 800,000 years. Changes in PO2 require imbalances between O2 sources [dominantly modern sedimentary organic carbon (Corg) and pyrite burial] and sinks (dominantly ancient sedimentary Corg and pyrite oxidation) (26). Thus, a higher rate of oxidative weathering relative to Corg and/or pyrite burial over the past million years could have caused the observed PO2 de- cline. The ~2-million-year (+1.5/ –0.5 million years) (26) geological residence time of O2, combined with the decline in dO2/N2 of 8.4‰ per million years, indicates that O2 sinks were 1.7% larger than sources over the past 800,000 years (27). We now explore possible causes for this drawdown, examining first the impact of changing erosion rates and second the impact of global cooling on PO2. Global erosion rates influence the amount of rock weathered (con- suming O2) and sediment buried (releasing O2). These rates have been suggested to have increased up to 100% in the Pleistocene rel- ative to the Pliocene (28) [though this is debated (29)]. Thus, the pos- sibility exists that increased Pleisto- cene sedimentary erosion and burial rates affected PO2 levels. Indeed, Torres et al. (30) modeled that in- creasing erosion rates over the past 15 million years enhanced oxida- tion of sedimentary pyrite rela- tive to burial so that PO2 declined on average by 9 to 25‰ per million years. This is similar to the decline given by the ice core record (8.4‰ per million years). We note that whether increasing erosion rates cause PO2 to decline (instead of increase) is unknown (31). Large increases (e.g., 100%) in Pleistocene ero- sion rates, if they did occur, likely would have required processes that keep O2 sources and sinks balanced within ~2% (the observed imbalance). Such processes could include the proposed PO2- dependent control of Corg burial fluxes on sedimen- tary phosphorus burial rates (32). Alternatively, sedimentary mineral surface area is known to positively correlate with total sedimentary Corg and pyrite content (33). Hedges and Kiel (33) pro- posed that the total eroded and total buried min- eral surface areas today are about equal. If this was true in the past, the conservation of eroded versus newly generated mineral surface area may have acted to balance Corg and pyrite weathering and burial fluxes (and thus O2 fluxes), regardless of global erosion rates (33). Alternatively, on the basis of 13 C/12 C and 18 O/16 O records from sedimentary carbonates, Shackleton (2) proposed that PO2 declined over the Neogene as a result of oceaniccooling. He suggestedthefollowing feedback loop: Cooling increases O2 solubility. This raises dissolved O2 concentrations, which increases the volume of ocean sediment exposed to dissolved O2 and thus also increases global aerobic Corg remineralization rates (33). On million-year time scales, Corg burial rates and, therefore, PO2 and O2 concentrations decline until seawater O2 concen- trations return to their initial (precooling) levels. At this new steady state, Corg burial rates have returned to their original values, but PO2 is stabilized at a lower value. Shackleton’s hypothesis can be evaluated to first order in the context of the dO2/N2 data by using records of past ocean temperature. Specifically, temperatures in the deep (>1000 m depth) ocean were roughly constant from 24 to 14 million years ago (34, 35). Assuming an O2 residence time of ~2 million years and the hypothesis that changes in ocean temperature modulate PO2, then O2 sources and sinks would have been in balance by 14 million years ago. The oceans have cooled on average by 0.3°C per million years over the past 14 million years and 0.5° to 1.1°C per million years over the past 5 million years (34, 35). Cooling of 0.3° to 1.1°C per million years increases O2 solubility by ~7 to 25‰ per million years (36). If dissolved O2 con- centrations remained constant (as this hypothesis requires), such changes in O2 solubility necessitate a decline in PO2 of ~7 to 25‰ per million years. These rates bracket the rate of decline given by the ice core record (8.4‰ per million years; Fig. 1A). We note that deep ocean cooling rates track aver- age marine cooling rates, but not precisely, because modern deep waters form in and thus reflect the temperatures of high latitudes. Regardless, the critical point is that this simple calculation is consistent with the ice core–derived dO2/N2 record and supports the hypothesis that global temperature stabilizes PO2 on geological time scales through feedbacks associated with Corg burial rates. A drop in PO2 over the past 800,000 years due solely to changes in Corg burial versus oxidation rates (regardless of the cause) requires positive CO2 fluxes (~3 × 1011 moles C per year) into the ocean and atmosphere (19). However, ice core records of past carbon dioxide partial pressures (PCO2) show no obvious change in the mean over SCIENCE sciencemag.org 23 SEPTEMBER 2016 • VOL 353 ISSUE 6306 1429 age (kyr) age (kyr) -5-5 00 55 1010 00 200200 400400 600600 800800 -5 0 5 10 0 200 400 600 800 O2/N2, all Ar/N2, Vostok Ar/N2, Dome C best-fit O2/N2 line Expected range of Ar/N2 trends if O2/N2 is controlled by bubble close-off fractionations or gas loss best-fit Ar/N2 line -5 0 5 10 100 450 800 -5-5-5 000 555 101010 100100100 450450450 800800800 -10 -10 -5 0 5 10 1400 2300 3200 depth (m) -10-10-10 -5-5-5-5 0000 5555 10101010 1400140014001400 2300230023002300 3200320032003200 -5 0 5 10 100 450 800 O2/N2(‰)O2/N2(‰) (‰) Fig. 2. Evidence that the observed decline in dO2N2 with time does not originate from either secular changes in bubble close-off fractionations or ice core storage. (A) dAr/N2 and dO2/N2 versus ice age. Bubble close-off processes and gas loss would cause dAr/N2 and dO2/N2 to covary with slopes of 0.3 to 0.6. The observed dAr/N2 trend does not overlap with these expected trends (orange wedge), indicating that such processes did not cause the decline in dO2/N2. (B) Dome C dO2/N2 versus ice age and (C) versus depth. Dotted lines were fit to ice >400,000 years old or >2600 m deep and extrapolated to younger ages or shallower depths. Extrapolations of the fits pass through the younger data (B) but miss the deeper data [beyond 4s (C)], indicating depth-dependent glacial properties did not cause the decline in dO2/N2. Gray bands are 95% confidence intervals. Data are corrected for gravitational, interlaboratory, and bubble close-off fractionations (19). RESEARCH | REPORTS onSeptember22,2016http://science.sciencemag.org/Downloadedfrom
  • 4. the past 800,000 years (37–39) (Fig. 3). To under- stand how changes in PO2 influence PCO2, we de- veloped a simple model of the carbon cycle that allows for changes in weathering and burial rates of carbonates, Corg, and silicates (19). In the ab- sence of any PCO2-dependent feedbacks, a constant decline in dO2/N2 of 8.4‰ over the past million years from a net imbalance in Corg fluxes causes PCO2 to rise by ~140 parts per million over the same time frame. Such a rise is inconsistent with the PCO2 record (Fig. 3). A PCO2-dependent silicate weathering feedback (40) can account for the higher CO2 flux if silicate weathering is enhanced by ~6% relative to volcanic outgassing. For exam- ple, response times for silicate weathering of 200,000 to 500,000 years (41) stabilize PCO2 levels within ~1 million years (Fig. 3). Changes in Cenozoic climate began millions of years before the start of our ice core–based dO2/N2 record 800,000 years ago (e.g., 2, 30, 34, 35). Thus, we suggest that modest enhancements in silicate weathering would already have stabi- lized the portion of the PCO2 ice core record that is controlled by differences in Corg and pyrite burial and oxidation. Thus, the combina- tion of changing PO2 and constant average PCO2 provides distinctive evidence for feedbacks that regulate PCO2 on geologic time scales (37). Last- ly, a 2% imbalance in O2 fluxes results in only a ~0.1‰ shift in the 13 C/12 C ratio of buried carbon (19). Our results provide a primary record of declin- ing PO2 over the past 800,000 years sustained by a ~2% imbalance between O2 sources and sinks. Critically, this decline is consistent with previously proposed and relatively simple models that invoke either the effects of increased Pleistocene erosion rates or decreased ocean temperature to explain feedbacks in the global cycles of carbon, sulfur, and O2—and the effects of both could have contributed to the observed decline in PO2. Regardless, creat- ing primary records of past PO2 is the necessary first step in identifying the fundamental processes that regulate PO2 on geological time scales. Given evidence that both global erosion rates and temperature have changed markedly over the Cenozoic (42), the ideas presented here may have implications for the history of PO2 beyond the Pleistocene. REFERENCES AND NOTES 1. L. R. Kump, R. M. Garrels, Am. J. Sci. 286, 337–360 (1986). 2. N. Shackleton, Geol. Soc. Lond. Spec. Publ. 26, 423–434 (1987). 3. R. A. Berner, D. E. Canfield, Am. J. Sci. 289, 333–361 (1989). 4. L. A. Derry, C. France-Lanord, Paleoceanography 11, 267–275 (1996). 5. K. W. Hansen, K. Wallmann, Am. J. Sci. 303, 94–148 (2003). 6. N. M. Bergman, T. M. Lenton, A. J. Watson, Am. J. Sci. 304, 397–437 (2004). 7. P. G. Falkowski et al., Science 309, 2202–2204 (2005). 8. R. S. Arvidson, F. T. Mackenzie, M. Guidry, Am. J. Sci. 306, 135–190 (2006). 9. R. A. Berner, Geochim. Cosmochim. 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Sigman for helpful discussions and three anonymous reviewers for helpful comments on the manuscript. D.A.S., J.A.H., and M.L.B. conceived the study and wrote the manuscript. D.A.S., J.A.H., M.L.B., and Y.Y. analyzed the data. G.B.D. measured the Dome C dAr/N2 data. The views expressed in this article are those of the authors and do not necessarily represent the views of the Department of Energy or the U.S. Government. SUPPLEMENTARY MATERIALS www.sciencemag.org/content/353/6306/1427/suppl/DC1 Materials and Methods Figs. S1 to S6 Tables S1 to S3 References (43–78) 25 February 2016; accepted 2 August 2016 10.1126/science.aaf5445 1430 23 SEPTEMBER 2016 • VOL 353 ISSUE 6306 sciencemag.org SCIENCE Fig. 3. Comparison of calculated and measured PCO2 values due to declin- ing PO2 with and without a PCO2- dependent silicate weathering feed- back. Inclusion of a silicate weathering feedback with geolog- ically reasonable response times [200,000 to 500,000 years (41)] stabilizes PCO2 within ~1 million years. Thus, increased silicate weathering rates could have compensated for enhanced CO2 fluxes from increased net Corg oxidation more than 800,000 years ago. The PCO2 records are continuous only from 800,000 years to the present. The model used to calculate PCO2 values is described in (19); the measured PCO2 values are from (38) and (39). ppm, parts per million. 150150 200200 250250 300300 350350 400400 00 200200 400400 600600 800800 10001000 150 200 250 300 350 400 0 200 400 600 800 1000 age (kyr) PCO 2 (ppm) ice core data No PCO2-dependent silicate weathering feedback 500-kyr response time for PCO2-dependent silicate weathering feedback 400-kyr response time for PCO2-dependent silicate weathering feedback 300-kyr response time for PCO2-dependent silicate weathering feedback 200-kyr response time for PCO2-dependent silicate weathering feedback No PCO2-dependent silicate weathering feedback results in changes in PCO2 inconsistent with measured ice core records. A PCO2-dependent silicate weathering feedback stabilizes PCO2 within ~1 million years following the creation of an imbalance in Corg burial versus weathering rates. RESEARCH | REPORTS onSeptember22,2016http://science.sciencemag.org/Downloadedfrom
  • 5. (6306), 1427-1430. [doi: 10.1126/science.aaf5445]353Science Higgins (September 22, 2016) D. A. Stolper, M. L. Bender, G. B. Dreyfus, Y. Yan and J. A. concentrations2A Pleistocene ice core record of atmospheric O Editor's Summary This copy is for your personal, non-commercial use only. Article Tools http://science.sciencemag.org/content/353/6306/1427 article tools: Visit the online version of this article to access the personalization and Permissions http://www.sciencemag.org/about/permissions.dtl Obtain information about reproducing this article: is a registered trademark of AAAS.ScienceAdvancement of Science; all rights reserved. The title Avenue NW, Washington, DC 20005. Copyright 2016 by the American Association for the in December, by the American Association for the Advancement of Science, 1200 New York (print ISSN 0036-8075; online ISSN 1095-9203) is published weekly, except the last weekScience onSeptember22,2016http://science.sciencemag.org/Downloadedfrom