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Still the Biggest Control Knob
 Carbon Dioxide in Earth’s Climate History
                               Richard B. Alley,
                               Penn State
                                    CLEAN Workshop
                                    Climate Complexities
                                    May 8, 2012
                                    Please note: I work for
                                    Penn State University,

                                    And help UN IPCC, NRC, etc.,
                                    But I am not representing them,
                                    Just me.


                       G. Comer
                       Foundation
What might control Earth’s temperature?

• Changes in LOTS of things
Brightness of Sun
Distance of Earth from Sun
Blockage of sunlight on its way to us
Reflection of sunlight by Earth (albedo)
Greenhouse effect
What might control Earth’s temperature?

• Changes in LOTS of things
Brightness of Sun—Fast changes small
 (whew!); slow ones offset by thermostat
Distance of Earth from Sun
Blockage of sunlight on its way to us
Reflection of sunlight by Earth (albedo)
Greenhouse effect
What might control Earth’s temperature?

• Changes in LOTS of things
Brightness of Sun
Distance of Earth from Sun—No worry!—
 dino-killer moved Earth less than 1”
Blockage of sunlight on its way to us
Reflection of sunlight by Earth (albedo)
Greenhouse effect
What might control Earth’s temperature?

• Changes in LOTS of things
Brightness of Sun
Distance of Earth from Sun
Blockage of sunlight on its way to us—tiny
 tiny tiny (not enough to matter)
Reflection of sunlight by Earth (albedo)
Greenhouse effect
What might control Earth’s temperature?

• Changes in LOTS of things
Brightness of Sun
Distance of Earth from Sun
Blockage of sunlight on its way to us
Reflection of sunlight by Earth (albedo)—
 can matter; hard to change much by itself
Greenhouse effect
What might control Earth’s temperature?

• Changes in LOTS of things
Brightness of Sun
Distance of Earth from Sun
Blockage of sunlight on its way to us
Reflection of sunlight by Earth (albedo)
Greenhouse effect—can matter a lot
 (Venus…), and easy to change, as we’ll see
What might control Earth’s temperature?

• Changes in LOTS of things
Greenhouse effect—Water vapor hard to
 change except by warming air (hair dryer
 has a heater for a good reason…)
Models: remove air’s water vapor and
 evaporation restores in a few days; remove
 CO2 and Earth freezes over (Pierrehumbert
 et al, 2007; Voigt and Marotzke, 2009)
Basis for CO2-caused warming:
                               Is PHYSICS
            Earth glowing      **Known for over a century
            to cool off        **Refined by Air Force after WWII
                               (operations, communications, and heat-
                               seeking missiles)
                               **Confirmed by history
          CO2 blocking,
          warms                **Observed today (satellites, etc.)
 “Color” in infrared
 (wavenumber cm-1)
Harries et al., 2001, Nature
Climate history confirms warming by CO2

• Temperature and CO2 correlate over time,
  for short-lived and long-lived events
• CO2 warms based on known physics
• Nothing else explains most main features of
  climate history (does not track brightness
  of sun, cosmic rays, or other things closely)
• Warming tends to raise CO2 over short
  times but lower CO2 over long times; history
  thus shows that CO2 controls temperature
  and not vice-versa.
Faint Young Sun “Paradox”
• Sun’s output ~70% of modern 4.6 billion
  years ago—fusing hydrogen to helium
  increases solar core’s density, so faster
  fusion occurs, balancing gravity;
• Yet evidence of liquid water on Earth as far
  back as we have records (~4.4 billion
  years);
• Earth reflects ~30% of sun now, so would
  need perfectly black early Earth (didn’t
  happen) to offset changing sun;
• So, physics plus data point to stronger early
Rock-Weathering Thermostat—When Earth
      cold, CO2 builds up in air, warming; when
      Earth warm, CO2 removed from air, cooling
 CO2 (gas)
                          Rock Weathering
                          removes CO2 from air—
              CaSiO3      CaSiO3+3H2O+2CO2
              (solid)     Ca+2+H4SiO4+2HCO3-
                          Faster when warmer
Volcanoes supply CO2
to air—rate (nearly)                 Shell Growth—
independent of climate               Ca+2+H4SiO4+2HCO3- 
                                     CaCO3+SiO2+3H2O+CO2



                     Shell subduction
                     CaCO3+SiO2

                                  Walker, J.C.G., P.B. Hays and J.F. Kasting, 1981
Rock Weathering Thermostat

• Enough to solve faint young sun paradox (Halevy,
  I., R.T. Pierrehumbert and D.P. Schrag, 2009);
• Supported by physical/chemical understanding;
• Maybe other greenhouse gases, etc. involved;
• If others failed, CO2 there to do the job;
• Is there any evidence for this other than
  physical/chemical unavoidability?
• Probably…Snowball Earth cap carbonates…
Snowball Earth

• Extensive low-elevation, low-latitude glacial
  deposits from some times on middle-aged Earth;
• Physical understanding: if CO2 warms & rock-
 weathering thermostat works, then
Can get into a snowball with a faint sun if fast
 (thermostat takes ~0.5 million years to work);
Then high snow albedo needs lots of CO2 to thaw;
Then lots of warming and rapid weathering should
  have deposited carbonate rocks rapidly
• And, cap carbonates sit atop snowball deposits.
Where the ice was at different
times (colors of stars relate to
geologic setting) (Hoffman and
Li, 2009, Paleo3)
Boulders dropped by
icebergs into laminated
marine sediment in late
Precambrian time,
Narachaampspos,
Kaokoveld, Namibia. The
chief proponent of the
Snowball Earth hypothesis,
Paul Hoffman, points to
the transition to carbonate
rocks which indicate the
sudden termination of this
frigid event. Photo M. J.
Hambrey.
http://www.swisseduc.ch/
glaciers/glossary/snowball
-earth-en.html




    See Hoffman, P.F. and D.P. Schrag. 2002. The snowball Earth hypothesis: testing the limits
    of global change. Terra Nova 14, 129-155.
CO2 Paleobarometers—How much was there?
• Gold standard is ice-core record;
• So far “only” 800,000 years, duplicated to
  450,000 yrs, and multiply duplicated younger;
• How do we know it works?
Youngest samples agree with instrumental record
Antarctic: same record from different sites with
  different temperature, accumulation, impurities
Sensible “failures”; e.g., in Greenland melt layers,
  expect and find excess CO2 localized, so diffusion
  not smearing much. In warm tropical-glacier ice
  with dead bugs, anomalous high CO2 as expected.
CO2 Paleobarometers
• Many others, based on influence of CO2
  abundance on something else that is
  preserved in sedimentary record, plus data-
  driven biogeochemical modeling;
• Nothing as simple and easy as ice-core data;
• Systematic errors of different techniques
  largely independent, so rely on cross-
  technique agreement;
• Technique development and refinement
  ongoing.
CO2 Paleobarometers
• δ13C of alkenones, soil carbonates, or liverworts:
  plants preferentially use faster diffusing 12C if
  CO2 abundant, but must use 13C if CO2 scarce;
• δ11B or B:Ca of foraminiferal shells: B(OH) 3
  enriched in 11B vs. the B(OH)4- incorporated in
  shells, and B residence time long, so δ11B or B:Ca
  paleo-pH meters linked to CO2
• Fossil-leaf stomata—plants grow leaves with more
  stomata when CO2 lower;
• Offspring-of-BLAG modeling driven by volcanism,
  δ13C, etc.
Resetting the Thermostat
• More CO2 from volcanoes (e.g., more volcanism, or
  shallower subduction zones so more shells
  subducted rather than dissolved);
• Slower weathering—colder or drier climate, or
  less-weatherable materials (e.g., shale at surface,
  vs. basalt), or less plant activity (e.g., pre-land-
  plants less CO2 in soil);
• Less fossil-fuel burial, or more fossil-fuel burning
  (e.g., higher-oxygen oceans because colder or
  less-fertilized);
• Change greatly over time-scales of plate tectonics
  and evolution—100 million years or so.
Figure 4.24 Atmospheric CO2 and continental glaciation 400 Ma to present. Vertical blue
bars, timing and palaeolatitudinal extent of ice sheets (after Crowley, 1998). Plotted CO2
records represent five-point running averages from each of four major proxies (see Royer, 2006
for details of compilation). Also plotted are the plausible ranges of CO2
derived from the geochemical carbon cycle model GEOCARB III (Berner and Kothavala,
2001). All data adjusted to the Gradstein et al. (2004) time scale. Continental ice sheets
grow extensively when CO2 is low. (after Jansen, 2007, that report’s Figure 6.1)
Next
                                        slide




Figure 4.24 Atmospheric CO2 and continental glaciation 400 Ma to present. Vertical blue
bars, timing and palaeolatitudinal extent of ice sheets (after Crowley, 1998). Plotted CO2
records represent five-point running averages from each of four major proxies (see Royer, 2006
for details of compilation). Also plotted are the plausible ranges of CO2
derived from the geochemical carbon cycle model GEOCARB III (Berner and Kothavala,
2001). All data adjusted to the Gradstein et al. (2004) time scale. Continental ice sheets
grow extensively when CO2 is low. (after Jansen, 2007, that report’s Figure 6.1)
Events—The Great Dying
• End-Permian extinction, 251 million years, perhaps
  95% of species became extinct;
• Widespread marine biomarkers of green sulfur
  bacteria that use H2S for photosynthesis (100
  ppm in air is immediate danger to life or health);
• Greatest volcanism in >500 million years (Siberian
  traps) (slow vs. human source, but protracted);
• CO2-induced warmth, fertilization from basalt
  breakdown, sulfur from volcanoes seem to have
  contributed to anoxia and euxinia (H2S) of ocean.
Events—The Saurian Sauna
• Mid-Cretaceous heat;
• No ice near sea-level at poles;
• Continental arrangement, high sea level warm a
  little but not nearly enough to explain warmth
  (Donnadieu et al. 2006);
• Data, model agree on high CO2;
• High CO2 explains warmth (although world maybe
  a tad warmer than models like, especially at
  poles), but warmth does NOT explain high CO2.
  Indeed, warmer conditions tend to lower CO2 by
  faster rock weathering and faster formation of
  fossil fuels.
Tropical
      temperature                                 CO2 level



      Temperature
      then +≈18oF

                                                  CO2 then

                                                     Now
                                                     Pre-human

         Now           Pre-human?




100 million years ago, Demarara Rise (Atlantic,
~9oN), Bice et al., 2006, Paleoceanography.
CO2 necessary to explain ice-free poles, hot tropics. Changes perhaps a bit bigger
than expected.
Scary thought
   NOT a forecast, but within the realm of
   possibility based on refereed science: we
   might make it too hot for unprotected
   humans to live in large parts of the Earth.

“…the wetbulb temperature...today…never exceeds 31 °C. Any exceedence of
35 °C for extended periods should induce hyperthermia in humans and other
mammals, as dissipation of metabolic heat becomes impossible…this …would
begin to occur with global-mean warming of about 7 °C, calling the habitability of
some regions into question. With 11–12 °C warming, such regions would spread
to encompass the majority of the human population as currently distributed.
Eventual warmings of 12 °C are possible from fossil fuel burning.” Sherwood &
Huber, PNAS, 2010
Time in
                                                                     next slide




Figure 4.24 Atmospheric CO2 and continental glaciation 400 Ma to present. Vertical blue
bars, timing and palaeolatitudinal extent of ice sheets (after Crowley, 1998). Plotted CO2
records represent five-point running averages from each of four major proxies (see Royer, 2006
for details of compilation). Also plotted are the plausible ranges of CO2
derived from the geochemical carbon cycle model GEOCARB III (Berner and Kothavala,
2001). All data adjusted to the Gradstein et al. (2004) time scale. Continental ice sheets
grow extensively when CO2 is low. (after Jansen, 2007, that report’s Figure 6.1)
~9oF ocean,
                        14oF land Arctic
                        warming, to
                        mid-70s
                        summer ocean




Figure 3.8. Global compilation of more than 40 deep sea benthic δ18O isotopic records
taken from Zachos et al. (2001), updated with high-resolution Eocene through Miocene
records from Billups et al. (2002), Bohaty and Zachos (2003), and Lear et al. (2004).
Dashed blue bars, times when glaciers came and went or were smaller than now; solid
blue bars, ice sheets of modern size or larger. (Figure and text modified from IPCC
Chapter 6, Paleoclimate, Jansen et al., 2007.)
Events—Paleocene-Eocene Thermal Maximum
• Strong isotopic anomaly—formerly-living
  (isotopically light) CO2 source (maybe at least
  partly CH4, but event long enough to shift to CO2);
• Widespread few-degree warming; models have
  trouble simulating as much warming as occurred;
• Acidic ocean (sea-floor dissolution & extinction);
• Many more effects—enhanced insect damage,
  plant and animal migration, animal dwarfing;
• Too short-lived to be caused by drifting
  continents, etc., probably some coincidences
  involved (nothing else this big for LONG times!);
• Recovery time matches carbon-cycle models well;
Zachos et al., 2005, Science
Still much slower
                             than human release;
                             maybe a similar




                  54
                             amount.
                               Zachos et al., 2001,
                               Science, PETM
                             The LPTM as recorded in benthic d13C
                             and d18O records (A and B,
                             respectively) from Sites 527 and 690 in




                  Age (Ma)
                             the south Atlantic (73), and Site 865 in
                             the western Pacific (26). The time scale
More CO2 Warmer              is based on the cycle stratigraphy of
                             Site 690 (30) with the base of the
                             excursion placed at 54.95 Ma. The
                             other records have been correlated to
                             Site 690 using the carbon isotope
                             stratigraphy. Apparent leads and lags
                             are artifacts of differences in sample
                             spacing. The oxygen isotope values
                             have been adjusted for species-specific
                  56         vital effects (118), and the temperature
                             scale on the right is for an ice-free
                             ocean. The negative carbon isotope
                             excursion is thought to represent the
                             influx of up to 2600 Gt of methane from
                             dissociation of seafloor clathrate (111).
Fig. 1. Representative insect damage diversity on PETM leaves. (a) Dicot sp. WW007 (Fabaceae) leaf about one-third consumed by insect
herbivores (USNM 530967). (b) Characteristic large, circular hole-feeding (DT4) found only on dicot sp.WW006(530968). (c) Serpentine mine
with a solid frass trail becoming massive (DT43) on an unidentifiable dicot (530969). (d) Polylobate to clustered galls (DT125) on dicot sp.
WW007 (Fabaceae, 530970). (e) Blotch mine with a sinusoidal frass trail (DT37) on dicot sp. WW003 (530971). ( f) Blotch mine with distinct
coprolites and terminal chamber (DT35) on dicot sp. WW006 (530972). (g) Serpentine
mine with a solid frass trail (DT43) on dicot sp. WW004 (530973). (h) Semilinear serpentine mine with terminal chamber (DT40) on dicot sp.
WW005 (530974). (Scale bars: white, 1 mm; black, 5 mm.) Currano et al., 2008, PNAS (>5000 fossil leaves, Wyoming)
Climate Not Just CO2 (Younger Dryas real)
• But, when I joined this field, there were lots of
  apparent mismatches between CO2 and
  temperature histories;
• Most have disappeared partially or completely as
  more and better data were collected:
 Ordovician glaciation now appears to have
  followed CO2 fall (Young et al., 2009);
 Apparently cool tropics/hot poles with high CO2
 now known to be hot in both (Bice et al., 2006);
 Improved Miocene CO2 and temperature
 reconstructions now show better agreement (e.g.,
 Kurschner et al., 2009);
Vostok, Petit et al.
Milankovitch predicted bumps
under arrows; found 50 years
later.
Vostok, Petit et al.
CO2 as part of ice-age cycling
• Ice ages paced by orbits; whole world
  cooled/warmed even though almost no change in
  total sun;
• After big ice grew in Canada, rising polar summer
  sunshine (obliquity both poles, precession north)
  began polar warming and ice melting;
• This changed Atlantic circulation, slowing warming
  in N and speeding in S;
• This shifted winds S from S. America, moving
  water and allowing CO2 escape from deep ocean
• Which warmed world including falling-sun tropics
(e.g., Jansen+ 2007; Hansen+ 2008; Alley 2003; Cuffey & Brook 2000;
    Anderson+ 2009; Broecker+ 2010; Denton+ 2010, Shakun+ 2012)
Figure 6.14. Simulated temperatures during the last 1 kyr with and without anthropogenic forcing, and also with weak or strong solar irradiance variations. Global mean
radiative forcing (W m–2) used to drive climate model simulations due to (a) volcanic activity, (b) strong (blue) and weak (brown) solar irradiance variations, and (c) all other
forcings, including greenhouse gases and tropospheric sulphate aerosols (the thin flat line after 1765 indicates the fixed anthropogenic forcing used in the ‘Nat’ simulations).
(d) Annual mean NH temperature (°C) simulated by three climate models under the forcings shown in (a) to (c), compared with the concentration of overlapping NH
temperature reconstructions (shown by grey shading, modified from Figure 6.10c to account for the 1500 to 1899 reference period used here). ‘All’ (thick lines) used
anthropogenic and natural forcings; ‘Nat’ (thin lines) used only natural forcings. All forcings and temperatures are expressed as anomalies from their 1500 to 1899 means; the
temperatures were then smoothed with a Gaussian-weighted filter to remove fluctuations on time scales less than 30 years. Note the different vertical scale used for the
volcanic forcing compared with the other forcings. The individual series are identified in Table 6.3.
Today
                Climate didn’t change




                                                                      Warmer
                                        Climate didn’t
                                        change

                                        When more cosmic rays
                                        reached Earth




Cosmic rays, magnetic field don’t matter much to climate.

From Muschler et al., 2005, QSR. δ18O (proxy for temperature) from GRIP core
F
(top), the concentration of 10Be (middle), and the flux of 10Be (bottom). The
Laschamp event of near-zero magnetic field (red arrow) allowed increased
cosmic-ray flux producing more 10Be, but with no apparent effect on climate.
So, where does that leave us?
• If higher CO2 warms, climate history is sensible,
  and CO2 caused or amplified most main changes;
• There is now no plausible alternative to this;
• If higher CO2 doesn’t warm, we must explain how
  physicists are so wrong, and how so many
  suddenly-unexplained events happened;
• CO2 may be forcing or feedback—air is warmed by
  a CO2 molecule regardless of how it got there;
• Paleoclimatic data show climate sensitivity similar
  to values in modern models (~3oC for doubled
  CO2), perhaps with somewhat higher values over
  centuries or millennia especially in polar regions.
So, where does that leave us?
• Lots of knobs control the Earth’s climate system;
• “Sun” knob isn’t twiddled much over short times,
  and ineffective over long times because of CO2;
• Magnetic-field, cosmic-ray, space-dust, other
  “space” knobs not shown to matter, and no more
  than fine-tuning (except very rare dinosaur-killer)
• Much on Earth matters regionally—a continent
  cools going from equator to pole, and North
  Atlantic ocean circulation is important—but global
  effect weak except through CO2;
• Much to learn! But, the complex history of Earth’s
  climate points to the power of human CO2 release.
Carbon Dioxide Biggest Control of Earth's Climate

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Carbon Dioxide Biggest Control of Earth's Climate

  • 1. Still the Biggest Control Knob Carbon Dioxide in Earth’s Climate History Richard B. Alley, Penn State CLEAN Workshop Climate Complexities May 8, 2012 Please note: I work for Penn State University, And help UN IPCC, NRC, etc., But I am not representing them, Just me. G. Comer Foundation
  • 2. What might control Earth’s temperature? • Changes in LOTS of things Brightness of Sun Distance of Earth from Sun Blockage of sunlight on its way to us Reflection of sunlight by Earth (albedo) Greenhouse effect
  • 3. What might control Earth’s temperature? • Changes in LOTS of things Brightness of Sun—Fast changes small (whew!); slow ones offset by thermostat Distance of Earth from Sun Blockage of sunlight on its way to us Reflection of sunlight by Earth (albedo) Greenhouse effect
  • 4. What might control Earth’s temperature? • Changes in LOTS of things Brightness of Sun Distance of Earth from Sun—No worry!— dino-killer moved Earth less than 1” Blockage of sunlight on its way to us Reflection of sunlight by Earth (albedo) Greenhouse effect
  • 5. What might control Earth’s temperature? • Changes in LOTS of things Brightness of Sun Distance of Earth from Sun Blockage of sunlight on its way to us—tiny tiny tiny (not enough to matter) Reflection of sunlight by Earth (albedo) Greenhouse effect
  • 6. What might control Earth’s temperature? • Changes in LOTS of things Brightness of Sun Distance of Earth from Sun Blockage of sunlight on its way to us Reflection of sunlight by Earth (albedo)— can matter; hard to change much by itself Greenhouse effect
  • 7. What might control Earth’s temperature? • Changes in LOTS of things Brightness of Sun Distance of Earth from Sun Blockage of sunlight on its way to us Reflection of sunlight by Earth (albedo) Greenhouse effect—can matter a lot (Venus…), and easy to change, as we’ll see
  • 8. What might control Earth’s temperature? • Changes in LOTS of things Greenhouse effect—Water vapor hard to change except by warming air (hair dryer has a heater for a good reason…) Models: remove air’s water vapor and evaporation restores in a few days; remove CO2 and Earth freezes over (Pierrehumbert et al, 2007; Voigt and Marotzke, 2009)
  • 9. Basis for CO2-caused warming: Is PHYSICS Earth glowing **Known for over a century to cool off **Refined by Air Force after WWII (operations, communications, and heat- seeking missiles) **Confirmed by history CO2 blocking, warms **Observed today (satellites, etc.) “Color” in infrared (wavenumber cm-1) Harries et al., 2001, Nature
  • 10. Climate history confirms warming by CO2 • Temperature and CO2 correlate over time, for short-lived and long-lived events • CO2 warms based on known physics • Nothing else explains most main features of climate history (does not track brightness of sun, cosmic rays, or other things closely) • Warming tends to raise CO2 over short times but lower CO2 over long times; history thus shows that CO2 controls temperature and not vice-versa.
  • 11. Faint Young Sun “Paradox” • Sun’s output ~70% of modern 4.6 billion years ago—fusing hydrogen to helium increases solar core’s density, so faster fusion occurs, balancing gravity; • Yet evidence of liquid water on Earth as far back as we have records (~4.4 billion years); • Earth reflects ~30% of sun now, so would need perfectly black early Earth (didn’t happen) to offset changing sun; • So, physics plus data point to stronger early
  • 12. Rock-Weathering Thermostat—When Earth cold, CO2 builds up in air, warming; when Earth warm, CO2 removed from air, cooling CO2 (gas) Rock Weathering removes CO2 from air— CaSiO3 CaSiO3+3H2O+2CO2 (solid) Ca+2+H4SiO4+2HCO3- Faster when warmer Volcanoes supply CO2 to air—rate (nearly) Shell Growth— independent of climate Ca+2+H4SiO4+2HCO3-  CaCO3+SiO2+3H2O+CO2 Shell subduction CaCO3+SiO2 Walker, J.C.G., P.B. Hays and J.F. Kasting, 1981
  • 13. Rock Weathering Thermostat • Enough to solve faint young sun paradox (Halevy, I., R.T. Pierrehumbert and D.P. Schrag, 2009); • Supported by physical/chemical understanding; • Maybe other greenhouse gases, etc. involved; • If others failed, CO2 there to do the job; • Is there any evidence for this other than physical/chemical unavoidability? • Probably…Snowball Earth cap carbonates…
  • 14. Snowball Earth • Extensive low-elevation, low-latitude glacial deposits from some times on middle-aged Earth; • Physical understanding: if CO2 warms & rock- weathering thermostat works, then Can get into a snowball with a faint sun if fast (thermostat takes ~0.5 million years to work); Then high snow albedo needs lots of CO2 to thaw; Then lots of warming and rapid weathering should have deposited carbonate rocks rapidly • And, cap carbonates sit atop snowball deposits.
  • 15. Where the ice was at different times (colors of stars relate to geologic setting) (Hoffman and Li, 2009, Paleo3)
  • 16. Boulders dropped by icebergs into laminated marine sediment in late Precambrian time, Narachaampspos, Kaokoveld, Namibia. The chief proponent of the Snowball Earth hypothesis, Paul Hoffman, points to the transition to carbonate rocks which indicate the sudden termination of this frigid event. Photo M. J. Hambrey. http://www.swisseduc.ch/ glaciers/glossary/snowball -earth-en.html See Hoffman, P.F. and D.P. Schrag. 2002. The snowball Earth hypothesis: testing the limits of global change. Terra Nova 14, 129-155.
  • 17. CO2 Paleobarometers—How much was there? • Gold standard is ice-core record; • So far “only” 800,000 years, duplicated to 450,000 yrs, and multiply duplicated younger; • How do we know it works? Youngest samples agree with instrumental record Antarctic: same record from different sites with different temperature, accumulation, impurities Sensible “failures”; e.g., in Greenland melt layers, expect and find excess CO2 localized, so diffusion not smearing much. In warm tropical-glacier ice with dead bugs, anomalous high CO2 as expected.
  • 18. CO2 Paleobarometers • Many others, based on influence of CO2 abundance on something else that is preserved in sedimentary record, plus data- driven biogeochemical modeling; • Nothing as simple and easy as ice-core data; • Systematic errors of different techniques largely independent, so rely on cross- technique agreement; • Technique development and refinement ongoing.
  • 19. CO2 Paleobarometers • δ13C of alkenones, soil carbonates, or liverworts: plants preferentially use faster diffusing 12C if CO2 abundant, but must use 13C if CO2 scarce; • δ11B or B:Ca of foraminiferal shells: B(OH) 3 enriched in 11B vs. the B(OH)4- incorporated in shells, and B residence time long, so δ11B or B:Ca paleo-pH meters linked to CO2 • Fossil-leaf stomata—plants grow leaves with more stomata when CO2 lower; • Offspring-of-BLAG modeling driven by volcanism, δ13C, etc.
  • 20. Resetting the Thermostat • More CO2 from volcanoes (e.g., more volcanism, or shallower subduction zones so more shells subducted rather than dissolved); • Slower weathering—colder or drier climate, or less-weatherable materials (e.g., shale at surface, vs. basalt), or less plant activity (e.g., pre-land- plants less CO2 in soil); • Less fossil-fuel burial, or more fossil-fuel burning (e.g., higher-oxygen oceans because colder or less-fertilized); • Change greatly over time-scales of plate tectonics and evolution—100 million years or so.
  • 21. Figure 4.24 Atmospheric CO2 and continental glaciation 400 Ma to present. Vertical blue bars, timing and palaeolatitudinal extent of ice sheets (after Crowley, 1998). Plotted CO2 records represent five-point running averages from each of four major proxies (see Royer, 2006 for details of compilation). Also plotted are the plausible ranges of CO2 derived from the geochemical carbon cycle model GEOCARB III (Berner and Kothavala, 2001). All data adjusted to the Gradstein et al. (2004) time scale. Continental ice sheets grow extensively when CO2 is low. (after Jansen, 2007, that report’s Figure 6.1)
  • 22. Next slide Figure 4.24 Atmospheric CO2 and continental glaciation 400 Ma to present. Vertical blue bars, timing and palaeolatitudinal extent of ice sheets (after Crowley, 1998). Plotted CO2 records represent five-point running averages from each of four major proxies (see Royer, 2006 for details of compilation). Also plotted are the plausible ranges of CO2 derived from the geochemical carbon cycle model GEOCARB III (Berner and Kothavala, 2001). All data adjusted to the Gradstein et al. (2004) time scale. Continental ice sheets grow extensively when CO2 is low. (after Jansen, 2007, that report’s Figure 6.1)
  • 23. Events—The Great Dying • End-Permian extinction, 251 million years, perhaps 95% of species became extinct; • Widespread marine biomarkers of green sulfur bacteria that use H2S for photosynthesis (100 ppm in air is immediate danger to life or health); • Greatest volcanism in >500 million years (Siberian traps) (slow vs. human source, but protracted); • CO2-induced warmth, fertilization from basalt breakdown, sulfur from volcanoes seem to have contributed to anoxia and euxinia (H2S) of ocean.
  • 24. Events—The Saurian Sauna • Mid-Cretaceous heat; • No ice near sea-level at poles; • Continental arrangement, high sea level warm a little but not nearly enough to explain warmth (Donnadieu et al. 2006); • Data, model agree on high CO2; • High CO2 explains warmth (although world maybe a tad warmer than models like, especially at poles), but warmth does NOT explain high CO2. Indeed, warmer conditions tend to lower CO2 by faster rock weathering and faster formation of fossil fuels.
  • 25. Tropical temperature CO2 level Temperature then +≈18oF CO2 then Now Pre-human Now Pre-human? 100 million years ago, Demarara Rise (Atlantic, ~9oN), Bice et al., 2006, Paleoceanography. CO2 necessary to explain ice-free poles, hot tropics. Changes perhaps a bit bigger than expected.
  • 26. Scary thought NOT a forecast, but within the realm of possibility based on refereed science: we might make it too hot for unprotected humans to live in large parts of the Earth. “…the wetbulb temperature...today…never exceeds 31 °C. Any exceedence of 35 °C for extended periods should induce hyperthermia in humans and other mammals, as dissipation of metabolic heat becomes impossible…this …would begin to occur with global-mean warming of about 7 °C, calling the habitability of some regions into question. With 11–12 °C warming, such regions would spread to encompass the majority of the human population as currently distributed. Eventual warmings of 12 °C are possible from fossil fuel burning.” Sherwood & Huber, PNAS, 2010
  • 27. Time in next slide Figure 4.24 Atmospheric CO2 and continental glaciation 400 Ma to present. Vertical blue bars, timing and palaeolatitudinal extent of ice sheets (after Crowley, 1998). Plotted CO2 records represent five-point running averages from each of four major proxies (see Royer, 2006 for details of compilation). Also plotted are the plausible ranges of CO2 derived from the geochemical carbon cycle model GEOCARB III (Berner and Kothavala, 2001). All data adjusted to the Gradstein et al. (2004) time scale. Continental ice sheets grow extensively when CO2 is low. (after Jansen, 2007, that report’s Figure 6.1)
  • 28. ~9oF ocean, 14oF land Arctic warming, to mid-70s summer ocean Figure 3.8. Global compilation of more than 40 deep sea benthic δ18O isotopic records taken from Zachos et al. (2001), updated with high-resolution Eocene through Miocene records from Billups et al. (2002), Bohaty and Zachos (2003), and Lear et al. (2004). Dashed blue bars, times when glaciers came and went or were smaller than now; solid blue bars, ice sheets of modern size or larger. (Figure and text modified from IPCC Chapter 6, Paleoclimate, Jansen et al., 2007.)
  • 29. Events—Paleocene-Eocene Thermal Maximum • Strong isotopic anomaly—formerly-living (isotopically light) CO2 source (maybe at least partly CH4, but event long enough to shift to CO2); • Widespread few-degree warming; models have trouble simulating as much warming as occurred; • Acidic ocean (sea-floor dissolution & extinction); • Many more effects—enhanced insect damage, plant and animal migration, animal dwarfing; • Too short-lived to be caused by drifting continents, etc., probably some coincidences involved (nothing else this big for LONG times!); • Recovery time matches carbon-cycle models well;
  • 30. Zachos et al., 2005, Science
  • 31. Still much slower than human release; maybe a similar 54 amount. Zachos et al., 2001, Science, PETM The LPTM as recorded in benthic d13C and d18O records (A and B, respectively) from Sites 527 and 690 in Age (Ma) the south Atlantic (73), and Site 865 in the western Pacific (26). The time scale More CO2 Warmer is based on the cycle stratigraphy of Site 690 (30) with the base of the excursion placed at 54.95 Ma. The other records have been correlated to Site 690 using the carbon isotope stratigraphy. Apparent leads and lags are artifacts of differences in sample spacing. The oxygen isotope values have been adjusted for species-specific 56 vital effects (118), and the temperature scale on the right is for an ice-free ocean. The negative carbon isotope excursion is thought to represent the influx of up to 2600 Gt of methane from dissociation of seafloor clathrate (111).
  • 32. Fig. 1. Representative insect damage diversity on PETM leaves. (a) Dicot sp. WW007 (Fabaceae) leaf about one-third consumed by insect herbivores (USNM 530967). (b) Characteristic large, circular hole-feeding (DT4) found only on dicot sp.WW006(530968). (c) Serpentine mine with a solid frass trail becoming massive (DT43) on an unidentifiable dicot (530969). (d) Polylobate to clustered galls (DT125) on dicot sp. WW007 (Fabaceae, 530970). (e) Blotch mine with a sinusoidal frass trail (DT37) on dicot sp. WW003 (530971). ( f) Blotch mine with distinct coprolites and terminal chamber (DT35) on dicot sp. WW006 (530972). (g) Serpentine mine with a solid frass trail (DT43) on dicot sp. WW004 (530973). (h) Semilinear serpentine mine with terminal chamber (DT40) on dicot sp. WW005 (530974). (Scale bars: white, 1 mm; black, 5 mm.) Currano et al., 2008, PNAS (>5000 fossil leaves, Wyoming)
  • 33. Climate Not Just CO2 (Younger Dryas real) • But, when I joined this field, there were lots of apparent mismatches between CO2 and temperature histories; • Most have disappeared partially or completely as more and better data were collected:  Ordovician glaciation now appears to have followed CO2 fall (Young et al., 2009);  Apparently cool tropics/hot poles with high CO2 now known to be hot in both (Bice et al., 2006);  Improved Miocene CO2 and temperature reconstructions now show better agreement (e.g., Kurschner et al., 2009);
  • 35. Milankovitch predicted bumps under arrows; found 50 years later.
  • 37. CO2 as part of ice-age cycling • Ice ages paced by orbits; whole world cooled/warmed even though almost no change in total sun; • After big ice grew in Canada, rising polar summer sunshine (obliquity both poles, precession north) began polar warming and ice melting; • This changed Atlantic circulation, slowing warming in N and speeding in S; • This shifted winds S from S. America, moving water and allowing CO2 escape from deep ocean • Which warmed world including falling-sun tropics (e.g., Jansen+ 2007; Hansen+ 2008; Alley 2003; Cuffey & Brook 2000; Anderson+ 2009; Broecker+ 2010; Denton+ 2010, Shakun+ 2012)
  • 38. Figure 6.14. Simulated temperatures during the last 1 kyr with and without anthropogenic forcing, and also with weak or strong solar irradiance variations. Global mean radiative forcing (W m–2) used to drive climate model simulations due to (a) volcanic activity, (b) strong (blue) and weak (brown) solar irradiance variations, and (c) all other forcings, including greenhouse gases and tropospheric sulphate aerosols (the thin flat line after 1765 indicates the fixed anthropogenic forcing used in the ‘Nat’ simulations). (d) Annual mean NH temperature (°C) simulated by three climate models under the forcings shown in (a) to (c), compared with the concentration of overlapping NH temperature reconstructions (shown by grey shading, modified from Figure 6.10c to account for the 1500 to 1899 reference period used here). ‘All’ (thick lines) used anthropogenic and natural forcings; ‘Nat’ (thin lines) used only natural forcings. All forcings and temperatures are expressed as anomalies from their 1500 to 1899 means; the temperatures were then smoothed with a Gaussian-weighted filter to remove fluctuations on time scales less than 30 years. Note the different vertical scale used for the volcanic forcing compared with the other forcings. The individual series are identified in Table 6.3.
  • 39. Today Climate didn’t change Warmer Climate didn’t change When more cosmic rays reached Earth Cosmic rays, magnetic field don’t matter much to climate. From Muschler et al., 2005, QSR. δ18O (proxy for temperature) from GRIP core F (top), the concentration of 10Be (middle), and the flux of 10Be (bottom). The Laschamp event of near-zero magnetic field (red arrow) allowed increased cosmic-ray flux producing more 10Be, but with no apparent effect on climate.
  • 40. So, where does that leave us? • If higher CO2 warms, climate history is sensible, and CO2 caused or amplified most main changes; • There is now no plausible alternative to this; • If higher CO2 doesn’t warm, we must explain how physicists are so wrong, and how so many suddenly-unexplained events happened; • CO2 may be forcing or feedback—air is warmed by a CO2 molecule regardless of how it got there; • Paleoclimatic data show climate sensitivity similar to values in modern models (~3oC for doubled CO2), perhaps with somewhat higher values over centuries or millennia especially in polar regions.
  • 41. So, where does that leave us? • Lots of knobs control the Earth’s climate system; • “Sun” knob isn’t twiddled much over short times, and ineffective over long times because of CO2; • Magnetic-field, cosmic-ray, space-dust, other “space” knobs not shown to matter, and no more than fine-tuning (except very rare dinosaur-killer) • Much on Earth matters regionally—a continent cools going from equator to pole, and North Atlantic ocean circulation is important—but global effect weak except through CO2; • Much to learn! But, the complex history of Earth’s climate points to the power of human CO2 release.

Editor's Notes

  1. Pierrehumbert, R. T., G. Brogniez and R. Roca, 2007, “On the Relative Humidity of the Atmosphere,” in Schneider, T. and A. Sobel (eds.), The Global Circulation of the Atmosphere (Princeton University Press, Princeton, NJ), p. 150; also Voigt, A. and J. Marotzke, 2009, “ The transition from the present-day climate to a modern Snowball Earth,” Climate Dynamics, doi 10.1007/s00382-009-0633-5
  2. Pierrehumbert, R. T., G. Brogniez and R. Roca, 2007, “On the Relative Humidity of the Atmosphere,” in Schneider, T. and A. Sobel (eds.), The Global Circulation of the Atmosphere (Princeton University Press, Princeton, NJ), p. 150; also Voigt, A. and J. Marotzke, 2009, “ The transition from the present-day climate to a modern Snowball Earth,” Climate Dynamics, doi 10.1007/s00382-009-0633-5