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5.18 Soils and Global Change in the Carbon Cycle over Geological Time G. J. Retallack University of Oregon, Eugene, OR, USA

5.18.1 INTRODUCTION 1 5.18.2 APPROACHES TO THE STUDY OF PALEOSOLS 3 5.18.2.1 Molecular Ratios 4 5.18.2.2 Strain and Mass-Transfer Analysis 5 5.18.2.3 Analyses of Stable Isotopes of Carbon and Oxygen 7 5.18.3 RECORD OF PAST SOIL AND GLOBAL CHANGE 7 5.18.3.1 Origins of Soil 8 5.18.3.2 Greenhouse Paleosols 9 5.18.3.3 Icehouse Paleosols 10 5.18.3.4 Cambro-Ordovician Greenhouse Paleosols 11 5.18.3.5 Terminal Ordovician Icehouse Paleosols 13 5.18.3.6 Siluro-Devonian Greenhouse Paleosols 13 5.18.3.7 Late Devonian to Icehouse Paleosols 13 5.18.3.8 Triassic–Jurassic Greenhouse Paleosols 15 5.18.3.9 Early Cretaceous Icehouse Paleosols 17 5.18.3.10 Cretaceous–Paleogene Greenhouse Paleosols 17 5.18.3.11 Neogene Icehouse Paleosols 17 5.18.3.12 Pleistocene Glacial and Paleosols 19 5.18.4 SOILS AND GLOBAL CARBON CYCLE CHANGES 21 ACKNOWLEDGMENTS 23 REFERENCES 23

5.18.1 INTRODUCTION amplified by biological acidification (Schwartz- mann and Volk, 1991; see Chapter 5.06). These Soils play an important role in the carbon mineral nutrients fuel photosynthetic fixation cycle as the nutrition of photosynthesized bio- and chemical reduction of atmospheric CO2 mass. Nitrogen fixed by microbes from air is a into plants and plantlike microbes, which are at limiting nutrient for ecosystems within the first the base of the food chain. Plants and photo- flush of ecological succession of new ground, synthetic microbes are consumed and oxidized and sulfur can limit some components of wet- by animals, fungi, and other respiring land ecosystems. But in the long term, the lim- microbes, which release CO2, methane, and iting soil nutrient is phosphorus extracted water vapor into the air. These greenhouse by weathering from minerals such as apatite gases absorb solar radiation more effectively (Vitousek et al., 1997a; Chadwick et al., 1999). than atmospheric oxygen and nitrogen, and are has an especially voracious appetite for important regulators of planetary temperature common alkali (Na þ and K þ ) and alkaline- and albedo (Kasting, 1992). Variations in (Ca2 þ and Mg2 þ ) cations, supplied solar insolation (Kasting, 1992), mountainous by hydrolytic weathering, which is in turn topography (Raymo and Ruddiman, 1992),

1 2 Soils and Global Change in the Carbon Cycle over Geological Time and ocean currents (Ramstein et al., 1997) also tapped underground reservoirs of fossil fuels, play a role in climate, but this review focuses on and our other perturbations of the carbon cycle the carbon cycle. The carbon cycle is discussed have also been significant (Vitousek et al., in detail in Volume 8 of this treatise. 1997b; see Chapter 8.10). The greenhouse model for global paleocli- Atmospheric increase of carbon in CO2 to mate has proven remarkably robust (Retallack, 750 Gt C by deforestation and fossil fuel burn- 2002), despite new challenges (Veizer et al., ing has driven ongoing global warming, but is 2000). The balance of producers and consumers not quite balanced by changes in the other car- is one of a number of controls on atmospheric bon reservoirs, leading to a search for a ‘‘mis- balance, because CO2 is added sing sink’’ of some 1.871.3 Gt C, probably in to the air from fumaroles, volcanic eruptions, terrestrial organisms, soils, and sediments of and other forms of mantle degassing (Holland, the northern hemisphere (Keeling et al., 1982; 1984). Carbon dioxide is also consumed Siegenthaler and Sarmiento, 1993; Stallard, by burial as carbonate and organic matter 1998). Soil organic matter is a big, rapidly within limestones and other sedimentary cycling reservoir, likely to include much of this rocks; organic matter burial is an important missing sink. long-term control on CO2 levels in the atmos- During the geological past, the sizes of, and phere (Berner and Kothavala, 2001). The fluxes between, these reservoirs have varied magnitudes of carbon pools and fluxes involved enormously as the world has alternated provide a perspective on the importance of between greenhouse times of high carbon soils compared with other carbon reservoirs content of the atmosphere, and icehouse (Figure 1). times of low carbon content of the atmosphere. Before industrialization, there was only Oscillations in the atmospheric content of 15 600 Gt (1 Gt ¼ 10 g) of carbon in CO2 and greenhouse gases can be measured, estimated, methane in the atmosphere, which is about the or modeled on all timescales from annual to same amount as in all terrestrial biomass, but eonal (Figure 2). The actively cycling surficial less than half of the reservoir of soil organic carbon reservoirs are biomass, surface oceans, carbon. The ocean contained only B3Gt of air, and soils, so it is no surprise that the biomass carbon. The deep ocean and sediments fossil record of life on Earth shows strong comprised the largest reservoir of bicarbonate linkage to global climate change (Berner, 1997; and organic matter, but that carbon has been Algeo and Scheckler, 1998; Retallack, 2000a). kept out of circulation from the atmosphere There is an additional line of evidence for for geologically significant periods of time past climatic and atmospheric history in the (Schidlowski and Aharon, 1992). Humans have form of fossil soils, or paleosols, now known

Atmosphere 600

100 50 50 0.6 74 74 Land biota 610 0.6 50 Rivers Surface ocean 1,000 Soil & detritus 0.8 Biota 3 10 1,560 6 1 DOC 700 4 90 100

Sediments 6 Intermediate and deep waters 4.8 × 107 1.2 × 107 38,000 Carbonate Organic 0.2

Figure 1 Pools and fluxes of reduced carbon (bold) and oxidized carbon (regular) in Gt in the preindustrial carbon cycle. Sources: Schidlowski and Aharon (1992), Siegenthaler and Sarmiento (1993), and Stallard (1998). Approaches to the Study of Paleosols 3

335

330

325

dioxide (ppm) dioxide Atmospheric carbon Atmospheric

320 Dec-68 Dec-69 Dec-70 Dec-71 Dec-72 Dec-73 (a) Calendar year 300

250

200

dioxide (ppm) dioxide Atmospheric carbon Atmospheric

150 300 200 100 0 (b) Thousands of years ago 6,000

4,000

2,000

dioxide (ppm) dioxide Atmospheric carbon Atmospheric 0 300 200 100 0 (c) Millions of years ago 8,000

6,000

4,000

dioxide (ppm) dioxide 2,000 Atmospheric carbon Atmospheric

0 400 200 0 (d) Millions of years ago

Figure 2 Variation in atmospheric CO2 composition on a variety of timescales ranging from annual to eonal (a) Reproduced from Keeling et al. (1982). (b) Reproduced by permission of Publishing Group from Petit et al. (1999). (c) Reproduced from Retallack (2001d). (d) Reproduced by permission of American Journal of Science from Berner and Kothavala (2001). to be abundant throughout the geological 5.18.2 APPROACHES TO THE STUDY record (Retallack, 1997a, 2001a). This chapter OF PALEOSOLS addresses evidence from fossil soils for global climate change in the past, and attempts to as- Many approaches to the study of paleosols sess the role of soils in carbon cycle fluctuations are unlike those of soil science, and more like through the long history of our planet. soil geochemistry prior to the earlier part of the 4 Soils and Global Change in the Carbon Cycle over Geological Time twentieth century (Thaer, 1857; Marbut, 1935). tropical regions for geologically significant pe- Such measures of soil fertility as cation- riods of time (Oxisols of Soil Survey Staff, exchange capacity and base saturation that 1999), the molar ratio of alumina over bases are used for characterizing surface soils (Buol can reach 100 or more, indicating that the slow et al., 1997) are inappropriate for the study of progress of hydrolysis has almost gone to paleosols because of profound modification of completion. the cation-exchange complex during burial Application of this approach to a Preca- and lithification of paleosols (Retallack, mbrian (1,000 Ma) paleosol from Scotland 1991). Many paleosols are now lithified and (Figure 3) showed the expected decrease of amenable to study using petrographic thin sec- hydrolytic weathering down from the surface, tions, X-ray diffraction, electron microprobe, and an overall degree of hydrolytic alteration and bulk chemical analysis (Holland, 1984; that is modest compared with deeply weathered Ohmoto, 1996; Retallack, 1997a). modern soils (Figure 4). Effects of hydrolysis of this paleosol can also be seen in petrographic thin sections and electron 5.18.2.1 Molecular Weathering Ratios microprobe analyses, which document convers- ion of feldspar into clay (Retallack and Soil formation (see Chapter 5.01) is not only Mindszenty, 1994). a biological and physical alteration of rocks, Other molar weathering ratios can be devised but a slow chemical transformation following to reflect leaching (Ba/Sr), oxidation (FeO/ a few kinds of reactions that seldom reach Fe2O3), calcification (CaO þ MgO/Al2O3), and chemical equilibrium. In many soils, the most salinization (Na2O/K2O). Two of these ratios important of these reactions is hydrolysis: the reflect differential solubility of chemically com- incongruent dissolution of minerals such as parable elements, but the calcification ratio feldspars to yield clays and alkali and alkaline- quantifies the accumulation of pedogenic cal- earth cations in solution. A useful proxy for cite and dolomite, and the ratio of iron of dif- the progress of this reaction in soils and ferent valence gives reactant and product of paleosols is the molar ratio of alumina (repre- iron oxidation reactions. In the Precambrian senting clay) over the sum of lime, magnesia, paleosol illustrated (Figure 4), these molar ra- soda, and potash (representing major cationic tios indicate that the profile was oxidized and nutrients lost into soil solution). A large well drained, but little leached, calcified, or database of North American soils (Sheldon salinized. Advantages of using molar weather- et al.,2002) has shown that this ratio is ing ratios are their simplicity and precision, free usually less than 2 for fertile soils (Alfisols and of assumptions concerning parent material Mollisols of Soil Survey Staff, 1999), but more composition and changes in volume during than 2 in less-fertile soils (Ultisols). In soils weathering and burial compaction. Smooth that have been deeply weathered in humid depth functions of molar weathering ratios

TorridonianTorridonian ssedimentsediments

1 m

LewisianLewisian ggneissneiss

AmphiboliteAmphibolite ddikeike

Figure 3 Sheigra paleosol (bleached and reduced zone B1 m thick to right) under Torridonian (1,000 Ma) alluvial fan deposits, and Staca paleosol at same unfoncormity but on amphibolite (left-hand side) near the hamlet of Sheigra, northwest Scotland. Photo courtesy of G. E. Williams; geological age revised by Williams and Schmidt (1997). Approaches to the Study of Paleosols 5

Point count data Molecular weathering ratios Type Sheigra clay Al2O3 Soil horizons Percent Percent Na2O CaO + MgO Al2O3 FeO CaO+MgO+ Ba Field observations grain size composition SiO Fe O K2O Al2O3 2 + 2 3 Na2O K2O Sr 50 50 0 3 6 0 1 2 0 0.1 0.2 0.5 1 0 5 10 1 3 m. Clay Silt SandGravelDusky red (10R3/4) Sand 317 0 Dusky red 318 At Clay Clay (5R3/2) 320 Dusky red (5R3/3) & greenish gray 321 (5GY5/1) Dusky red (5R3/2) 1 Weathering rind 323

Greenish gray 324 (5GY6/1) Co

Dark gray (N4) 327 2

Dark reddish Quartz Corestone gray (5R4/1)

Weathering rind res 328

Greenish gray silt 3 (5GY6/1)

Crack between coCrack

Opaque 4 Dark gray (N4)

dspar 329 Fel

Sand

5

nblende

e

ed hor R Biotit

6 Chloritiz

Dark gray (N4) 330

Biotite gneiss Pink color Salinization CalcificationClayeyness Base loss Leaching Gleization none none moderate moderate moderate none Pegmatite Brown color Ripple mark Bedding Ferruginized

Figure 4 Columnar section (measured in field), petrographic composition (from point counting), and mo- lecular weathering ratios (from major element chemical analyses) of the Sheigra paleosol. Reproduced by permission of Society for Sedimentary Geology from Retallack and Mindszenty (1994).

(Figure 4) are characteristic of soils and paleo- samples, which can illustrate reaction paths sols, whereas parent material heterogeneity (Bestland and Retallack, 1993). is revealed by erratic swings in weathering ratios. Whole-rock chemical analyses are com- monly used to calculate molar weathering 5.18.2.2 Strain and Mass-Transfer Analysis ratios, and thus conflate weathered parts of the soil with unweathered interiors of soil A full accounting of volume and chemical grains. This problem can be circumvented changes during weathering and burial can be by calculating molar weathering ratios from made by assuming that one component of a electron microprobe spot analyses of weathered paleosol has remained stable from the parent and unweathered grains within paleosol material. This method requires measurement 6 Soils and Global Change in the Carbon Cycle over Geological Time of bulk density and identification of a parent which includes a partial normalization to alu- material. Alumina, titania, and zirconium are mina. commonly used as stable constituents, with Limitations on calculating strain and mass zirconium favored because its mobility can be transfer come mainly from the identification checked by microscopic examination of pitting and characterization of the parent material of of grains of zircon, which is the main soil min- soils and paleosols. The actual materials from eral containing zirconium (Brimhall et al., which they weathered no longer exist (Jenny, 1991). The assumption of geochemical stabil- 1941). The nature of parent materials can be ity allows one to calculate volume losses or reconstructed by studying the rock or sediment gains (i.e., strain) of samples from a parent lower within soil or paleosol profiles. Parent composition and material losses or gains (i.e., material reconstruction can be checked chem- mass transfer) of individual chemical elements ically and petrographically for degree of weath- from a soil or paleosol (see Chapter 5.01). This ering in igneous or metamorphic rocks below a formulation of strain is especially useful for soil (Figures 3 and4 ), but is not so easily as- paleosols, because some component of strain sessed in sediments or colluvium below a soil. It is due to burial compaction, which can be ex- is difficult to rule out soil formation from a thin pressed visually (Figure 5). sedimentary or colluvial cap to an igneous The Precambrian paleosol illustrated as an rock, although large influxes of new material example of this approach shows moderate from wind, floods, or landslide will be revealed weathering and volume loss with weathering by positive strain values. and burial compaction. Most elements were Kinetic modeling approaches (Merino lost from the profile, except potassium, and in et al., 1993) can be applied to isovolumetric one (but not another adjacent) paleosol, iron weathering if conservation of volume is sup- (Figure 5). This represents a thorough geo- ported by textural evidence (Delvigne, 1998). chemical accounting of changes relative to zir- Computer-aided thermodynamic modeling conium during soil development and burial of ancient weathering has also proven useful, of this paleosol, but is not at variance with especially for Precambrian paleosols (Schmitt, the simpler molar weathering ratio approach, 1999).

Swell & lose Swell Swell & lose Swell Swell & lose Swell & gain & gain & gain Al Fe2+ Fe3+ 0 0 0

−0.2 −0.2 −0.2

−0.4 −0.4 −0.4

as fraction cm)

Shrink Shrink Shrink & lose & gain & gain Shrink & gain

g (

−0.4 −0.2 0 −1 −0.5 0 0.3 −0.5 0 0.5 Transported mass of selected elements ( as fraction grams)

Swell & lose Swell Swell & lose Swell Swell Swell & gain & gain & gain & lose Mg + Ca Na K 0 0 0

−0.2 −0.2 −0.2

Strain due to burial & weatherin

−0.4 −0.4 −0.4

Shrink Shrink Shrink & lose & gain & gain Shrink & gain

−1 −0.5 0 −0.5 0 0.3 012

Sheigra clay Sheigra clay Staca clay Staca clay Likely compaction profile surface horizon profile surface horizon due to burial Figure 5 Mass transfer and strain of the Sheigra paleosol. The stippled bars are a range of values for likely strain due to burial compaction, as opposed to pedogenic strain. Reproduced by permission of Society for Sedimentary Geology from Retallack and Mindszenty (1994). Record of Past Soil and Global Change 7 5.18.2.3 Analyses of Stable Isotopes of Carbon intrudes into soil pores, and can be fixed there and Oxygen by the precipitation of pedogenic carbonate. In contrast, under low atmospheric CO2 levels, Three isotopes of carbon are commonly CO2 of soil air is isotopically light, because it is assayed by mass spectrometer: the common respired with relatively minor isotopic fraction- isotope 12C, the rare isotope 13C, and the ra- ation from isotopically light soil plant material, diogenic isotope 14C. Radiocarbon is formed in and may, therefore, generate isotopically light the atmosphere, incorporated within plants and pedogenic carbonate. It is also prudent to animals, and then fossilized as a constituent of measure the isotopic composition of organic carbonates and organic carbon. The progre- carbon in the same paleosol, as a guide to the ssive radioactive decay of radiocarbon is used isotopic composition of CO2 in the ancient for isotopic dating, but unfortunately its abun- atmosphere, because this can vary substan- dance decreases to undetectable amounts after tially (Mora et al., 1996; Jahren et al., 2001). A 5 B10 years. In contrast, the stable isotopes atmospheric CO2 curve con- 12C and 13C are found in rocks and paleosols of structed from a compilation of such data all geological ages. Their relative abundance is (Ekart et al., 1999) is consistent with independ- commonly reported on a scale of per mil that ent evidence of CO2 levels from the stomatal reflects their ratios normalized to a standard, a index of fossil leaves during all but a few fossil belemnite from the Peedee formation of episodes of catastrophic methane–clathrate North Carolina (PDB), or the mean value of outbursts (Retallack, 2001b, 2002). modern ocean water (SMOW). These carbon The attenuation of atmospheric isotopic val- isotopic values (d13C) are affected by a variety ues within paleosol profiles can also be used to of physical, chemical, and biological processes. estimate former soil respiration (Yapp and The key photosynthetic enzyme of plants, Rub- Poths, 1994), sometimes with surprising results, isco, selects the light isotope (12C) preferentially such as the near-modern soil respiration rates to the heavy isotope (13C), so that plant organic inferred from the dramatic attenuation of matter is isotopically much lighter (d13C more isotopic values (d13C) in a Late Ordovician negative) than the atmospheric or oceanic CO2 paleosol (Figure 6). In this case, carbonate oc- from which it was derived. cluded within pedogenic goethite was analyzed, Some plants employ a photosynthetic rather than pedogenic carbonate itself, because pathway creating at first a three-carbon phos- this might have been contaminated by over- phoglyceric acid (C3 or Calvin–Benson photo- lying marine rocks. synthesis). These plants fractionate isotopes Oxygen isotopes, 16O and 18O, are usually more intensely, and so have more negative reported in per mil (d18O) relative to the same d13C values (33% to 22% PDB) than plants standards used for carbon isotopes (PDB and that use a photosynthetic pathway creating at SMOW). Oxygen isotopes are also fractionated first a four-carbon malic and aspartic acid (C4 differently by C3 and C4 plants because they or Hatch–Slack :16% to 9% contribute to the mass of CO2 taken in for PDB). Crassulacean acid metabolism (CAM) is photosynthesis (Farquhar et al., 1993). Oxygen yet another photosynthetic pathway, which isotopic values are also determined by the com- creates organic matter of intermediate isotopic position of water in soil, coming in as rain, composition (35% to 11% PDB). Me- and later flowing out as groundwater through thanogenic microbes are more extreme in their buried paleosols (Amundson et al., 1998). fractionation of the light isotope (d13C down to Temperature, degree of evaporation, and salin- 110% and typically 60% PDB; Jahren ity strongly affect the isotopic composition et al., 2001). Today most C4 plants are trop- of oxygen in surface water, and can potentially ical grasses, and most CAM plants are sub- be inferred from the isotopic composition of merged aquatic plants and desert succulents. oxygen in paleosol carbonates (Mora et al., Most other kinds of plants use the C3 photo- 1998), paleosol clays (Bird and Chivas, 1993), synthetic pathway. There is the potential to and fossils in paleosols (Jahren and Sternberg, recognize these various metabolic pathways 2002). from the isotopic composition of organic car- bon in paleosols and fossil plants, and in the fossils of animals that ate the plants (Cerling 5.18.3 RECORD OF PAST SOIL AND et al., 1997; MacFadden et al., 1999; Krull GLOBAL CHANGE and Retallack, 2000). The isotopic composition of carbon in car- Paleosols have long been recognized in the bonate in paleosols can also be used as a CO2 geological record (Hutton, 1795; Webster, 1826; paleobarometer (Cerling, 1991). Under high Buckland, 1837), but their great abundance atmospheric CO2 levels, isotopically heavy CO2 in terrestrial sedimentary sequences was not 8 Soils and Global Change in the Carbon Cycle over Geological Time

13 CPDB Mole fraction

of goethite (%) CO in goethite Gravel

Clay Silt Sand 3 cm −18 −16 −14 0.004 0.006 0 Marine fossils

Dolostone

Oolitic ironstone

50 Red color

Brown color

Ferruginized surface

Bedding 100

Figure 6 Isotopic composition of carbon in carbonate and mole fraction CO3 in goethite of a Late Ordovician paleosol from Iron Knob, Wisconsin, showing surprisingly high soil respiration from shallow distance of adjustment of soil to atmospheric values. Reproduced by permission of Paleontological Society from Retallack (2000a). appreciated until the 1970s (Allen, 1974; Retal- Aeronautical and Space Administration lack, 1976). Many variegated red beds, such as (NASA) in using the widely understood word the Big Badlands of South Dakota, soil for nonsedimentary modified surfaces of are volumetrically dominated by paleosols the Moon and the Mars. (Retallack, 1983). Almost all coal seams are Whether there was or is life on Mars remains paleosols (Histosols), and these are not the only uncertain (McSween, 1997). There is no dis- paleosols in thick coal measure sequences cernible life in lunar or martian soils at the time (Retallack, 1994a). Thousands of paleosols of of this writing, but that may change with future all geological ages have been described since human discoveries and colonization of space. If the early 1980s, and there is now the prospect the Moon and the Mars are considered to have of using them to interpret long-term patterns soils, then soil formation goes back to the of environmental and biotic change. first alterations of planetismal and planetary surfaces which occurred in place, as opposed to those transported to form sediments, which are distinct and antithetic to soil formation. 5.18.3.1 Origins of Soil Thus defined, both soils and sediments are very ancient. Soil, like love and home, is difficult to define Hydrolytic alteration of mafic minerals (pyr- precisely. If one follows some soil scientists in oxene and olivine) to clays (iron-rich smectite), defining soil as a medium of plant growth (Buol oxides (magnetite), carbonates (gypsum, cal- et al., 1997), then the formation of soils began cite), and salts (kieserite) has been documented either at the advent of vascular land in carbonaceous chondritic meteorites (Bunch plants (Gray, 1993), or at the advent and Chang, 1980; Volume 1 of this treatise). of nonvascular land plants (Strother, 2000), or Carbonaceous chondrites also show opaque at the Late Precambrian advent of eukaryotic weathering rinds around mafic grains, cross- soil algae or algal phycobionts of lichens cutting veins filled with carbonate, clay skins, (Retallack, 1994b; Steiner and Reitner, 2001). and distinctive clayey birefringence fabrics A geological view of soils, however, would in- (sepic plasmic fabric; Retallack, 2001a). Car- clude rocks and soils altered by hydrolytic bonate veins have been dated radiometrically at weathering, which has been well documented at no more than 50 Ma younger than enclosing least as far back as the Archean (2,800 Ma; Rye clayey meteorites dated at 4,566 Ma (Birck and and Holland, 1998). Hydrolytic weathering has Alle` gre, 1988; Endress et al., 1996). Carbon- also been proposed for rocks as old as aceous chondrites are similar to the surface of 3,500 Ma (Buick et al., 1995), and meteorites some asteroids (Veverka et al., 1997). One in- as old as 4,566 Ma (Retallack, 2001a). The terpretation of carbonaceous chondrites is as author prefers to follow the US National fragments of paleosols from asteroid-sized Record of Past Soil and Global Change 9 planetesimals formed early during the forma- subjected to exceptionally detailed geochemical tion of the solar system. As primeval soils of and petrographic analyses. Along with many the solar system, they were similar in their other Precambrian paleosols reviewed by Rye smectites, salts, and carbonates to the soils of and Holland (1998), these paleosols reveal Mars, which are probably paleosols relict from the antiquity and thoroughness of hydrolytic a time of free water at the martian surface until weathering during the Precambrian. Even at least 2,500 Ma (Retallack, 2001a). then, rock and sediment were under relentless A second interpretation of carbonaceous acid attack, which leached base cations (espe- chondrites is as primary condensates of the cially Ca2 þ ,Mg2 þ , and Na þ ), and left thick, solar nebula. By this view, their hydrolytic clayey soil. alteration is due to melting in cometary nuclei It is likely that at least back to 3,500 Ma, the during close passes with the Sun, or due to principal environmental acid driving this hy- transient heating events by shock waves or drolytic reaction was carbonic acid dissolved in collisions (McSween, 1999). Other carbon- rain and groundwater (Holland, 1984), as is the aceous chondrites show metamorphic altera- case in soils today (Nahon, 1991). Much soil tion with minerals similar to those in Earth CO2 may also have come from respiring organ- formed during deep burial under elevated isms, which also could have contributed temperatures and pressures (Brearley, 1999). organic acids. Nitric and sulfuric acid may Like soils and paleosols on Earth and Mars, have been locally important in soils developed carbonaceous chondrites demonstrate the great on particular parent materials, but nitrogen antiquity of hydrolytic weathering in dilute and sulfur salts are so far unreported in Pre- acidic solutions, presumably of carbonic acid cambrian paleosols, unlike modern soils of derived from water vapor and CO2. These re- mine dumps (Borden, 2001), and hypothesized main the principal gases released from volca- modern soils on Mars (Bell, 1996; Farquhar noes, and soils remain important buffers for et al., 2002) and Venus (Barsukov et al., 1982; this environmental acid. Basilevsky et al., 1985). This view of the likely acids involved in for- ming Precambrian soils on Earth is supported by the isotopic composition of carbon, nit- 5.18.3.2 Archean–Paleoproterozoic rogen, and sulfur in sedimentary organic mat- Greenhouse Paleosols ter, carbonates, sulfates, and sulfides, which are surprisingly similar to their modern counter- Despite predictions that Precambrian paleo- parts back to 3,500 Ma, and unlike meteoritic sols would be thin, rocky, and dominated by or mantle values (Schidlowski et al., 1983; Des physical weathering (Schumm, 1956), hundreds Marais, 1997; Canfield and Teske, 1996). of Precambrian paleosols now described have Evidence for life in Precambrian soils comes been found to be thick, clayey, deeply weath- from isotopic studies of organic carbon within ered, and in some cases with possible traces of paleosols. Microlaminated chips in the 2,765 life, so that chemical and biological weathering Ma Mt. Roe paleosol of Western Australia can be traced back almost to the beginning of have extremely depleted carbon isotopic com- 13 the suitably preserved sedimentary rock record positions (d Corg 40%). Isotopic fraction- on Earth (Rye and Holland, 2000). The oldest ation of carbon to this degree is only known in known profile interpreted to be a paleosol methanogens and methanotrophs (Rye and shows alteration to depths of 50 m on granites Holland, 2000). These chips could be fragments unconformably underlying the 3,500 Ma sedi- of pond scum rather than a true soil microb- mentary succession of the Warrawoona Group iota. Organic matter in the 2,560 Ma Schagen in northwestern Western Australia (Buick paleosols of South Africa is not nearly as de- 13 et al., 1995). Corundum ores in the 3,500 Ma pleted (16% to 14%d Corg) as organic Aldan Schists of Siberia have been interpreted matter in overlying marine sediments (35% to 13 as metamorphosed, deeply weathered bauxites 30%d Corg). Interpretation of the carbon in (Serdyuchenko, 1968). this paleosol as the signature of a hypersaline The Jerico Dam paleosol of South Africa microbial soil community is compatible with (3,000 Ma; Grandstaff et al., 1986), the Pronto shallow dolocretes and other features of the paleosol of Canada (2,450 Ma; Mossman and paleosols (Watanabe et al., 2000). Farrow, 1992), the Hokkalampi paleosol of Normal isotopic values for soil organic mat- 13 Finland (2,200 Ma; Marmo, 1992), a variety ter (25% to 27%d Corg) have been re- of paleosols associated with the Hekpoort ported from Precambrian paleosols as well Basalt of South Africa (2,100 Ma; Yang and (Mossman and Farrow, 1992; Retallack and Holland, 2003), and the Sheigra paleosol of Mindszenty, 1994). Virtually all Precambrian Scotland (1,000 Ma; Figures 3 and4 ) have been paleosols have a very low content of organic 10 Soils and Global Change in the Carbon Cycle over Geological Time carbon comparable with that of well-drained atmospheric greenhouse effect was probably paleosols of the Phanerozoic. If life had been also much higher than at present, because present in the Early Precambrian paleosols, it was necessary to maintain planetary temper- they would have become carbonaceous in the atures above that of the freezing of water at absence of a decomposing microbiota of ac- the time of a faint young Sun (Kasting, 1992; tinobacteria and of fungi and metazoans during Pavlov et al., 2000). the later Precambrian. Isotopic evidence thus suggests that methanogenic, hypersaline, nor- mal, and decompositional microbes were pre- sent in Precambrian paleosols. Other evidence 5.18.3.3 Proterozoic Icehouse Paleosols for life in Precambrian paleosols includes mi- crofossils (1,300 Ma; Horodyski and Knauth, The oldest known periglacial paleosols 1994), microbial trace fossils (2,200 Ma; Retal- are from the 2,300 to 2,400 Ma Ramsay Lake lack and Krinsley, 1993), chemofossils Formation of Ontario, Canada (Young and (2,900 Ma; Prashnowsky and Schidlowski, Long, 1976; Schmidt and Williams, 1999). They 1967), plausible megafossils (2,900 Ma; Hall- have prominent ice wedges, which are strongly bauer et al., 1977; Retallack, 1994b), and the tapering cracks filled originally with ice, but impressive thickness and soil structure of Pre- now with massive or horizontally layered sand cambrian paleosols (3,500 Ma; Retallack, 1986, and claystone breccia. Modern ice wedges form 2001a; Buick et al., 1995; Gutzmer and Beukes, in climates with a mean annual temperature 1998; Beukes et al., 2002). Life and its by- of4to8 1C, coldest month temperatures of products such as polysaccharides may have 25 to 40 1C, warmest month temperatures been soil binders, like molasses applied to a of 10–20 1C, and a mean annual precipitation cornfield (Foster, 1981), protecting soils from of 50–500 mm (Williams, 1986; Bockheim, physical weathering so that biochemical weath- 1995). Periglacial paleosols of the Late Pre- ering could proceed. cambrian (600–1,000 Ma) in Scotland, Norway, The likely existence of microbial mats at the and South Australia include sand wedges soil surface considerably complicates the use of (Figure 7), which indicate an even drier and paleosols as indicators of ancient atmospheres more frigid climate: a mean annual tempera- (Ohmoto, 1996). Tropical rainforest soils now ture of 12 to 20 1C, a mean cold-month have soil CO2 levels up to 110 times that of the temperature of35 1C, a mean warm-month atmosphere, because of high levels of soil res- temperature of 4 1C, and mean annual precip- piration by termites and microbes of an abun- itation of 100 mm (Williams, 1986). Some of dant supply of soil organic matter that forms in the Late Precambrian glaciations were remark- a living membrane separating the subsoil from able in extending to very low latitudes, as in- the atmosphere (Brook et al., 1983; Colin et al., dicated by the paleomagnetic inclination of 1992). Nevertheless, modeling by Pinto and glaciogene sediments, and have been dubbed Holland (1988) makes it unlikely that microbial events (Kirschvink, 1992; scums of the Precambrian were as productive Hoffman et al., 1998; Schmidt and Williams, and effective membranes as rainforests. 1999). Between and before these Precambrian The observation that Precambrian paleosols episodes of periglacial paleosols and associated were chemically weathered to an extent com- glaciogene sediments there is no evidence of parable with rainforest soils today probably frigid conditions, so that the alternation of indicates much higher levels of CO2 in the at- global icehouse and greenhouse paleoclimates mosphere at that time (Holland, 1984). The is ancient indeed. extent of this greenhouse is poorly constrained, These climatic fluctuations could be attrib- but the apparent lack of siderite in paleosols uted to changes in solar luminosity, volcanic such as the Hekpoort and Mt. Roe paleosols degassing, or ocean current reorganization with has been used by Rye et al. (1995) to argue that continental drift (Barley et al., 1997; Dalziel, CO2 concentrations could not have been more 1997), but paleosols reveal that these ice ages than ca. 100 times present levels before the rise were also times of change in the atmosphere of oxygen at ca. 2,100 Ma. and life on land. Highly ferruginized pisolitic Siderite is common in Phanerozoic wetland lateritic paleosols first appear in the geological paleosols (Ludvigsen et al., 1998) in which re- record at 2,200–1,920 Ma in South Africa spired soil CO2 exceeded this level. Thus, the (Gutzmer and Beukes, 1998; Beukes et al., estimate of Rye et al. (1995) of no more than 2002). The lateritic paleosols are part of a 100 times present levels of soil CO2 also is a complex erosional landscape with a variety of cap on soil respiration and biological pro- paleosols of significantly different geological ductivity during the Precambrian (Sheldon ages, including mildly oxidized (Retallack, et al., 2001). The contribution of CH4 to the 1986; Maynard, 1992) and chemically reduced Record of Past Soil and Global Change 11

10 cm

Figure 7 Near-vertical sandstone wedge remaining from fill of ice wedge penetrating the Cattle Grid Breccia (680 Ma), in the Mt. Gunson Mine, South Australia. Photo courtesy of G. E. Williams. paleosols (Rye and Holland, 1998). Opinions algae and before the origin of metazoans differ on the nature and timing of this apparent (Heckman et al., 2001). This question is also oxygenation event. Holland (1984), Holland discussed in Chapter 5.06. There has long been and Beukes (1990), and Yang and Holland a debate about plausible permineralized as- (2003) proposed an abrupt rise from less than comycetes in the 770 Ma Skillogallee Dolomite 0.1% (v/v) to more than 3% O2 at B2,100 Ma. of South Australia (Retallack, 1994b). Late In contrast, Ohmoto (1996, 1997) and Be- Precambrian (600 Ma) enigmatic fossils, widely ukes et al. (2002) argue that the Great Oxida- called ‘‘Twitya disks’’ after their original tion Event interpretation does not take into northwest Canadian discovery site, are proba- account the reducing power of biological bly microbial colonies (Grazdhankin, 2001), activity within Precambrian paleosols, and that and some have been found in ferruginized O2 levels were close to present levels from 3,000 paleosols (Retallack and Storaasli, 1999). Lat- to 1,800 Ma. An intermediate view of rising, est Precambrian (550–540 Ma) interglacial and but fluctuating atmospheric oxidation also is postglacial circular fossils, widely interpreted compatible with available paleosol data (Retal- as cnidarian medusae, have also been reinter- lack, 2001a), and with limited evidence from preted as lichenized microbial colonies and mass-independent fractionation of sulfur iso- are found in paleosols (Retallack, 1994b; topes (Farquhar et al., 2002). Grazdhankin, 2001; Steiner and Reitner, Oxidation of the atmosphere and soils could 2001). The appearance of lichens with their have come from lichens, possibly actinolichens, deeply reaching rhizines in a world of cyano- considering the small diameter of their fila- bacterial mats could have greatly increased the ments, reported from the 2,900 Ma Carbon rate of biochemical weathering, carbon seques- Leader of South Africa (Hallbauer et al., 1977). tration, oxygenation of the atmosphere, and Their organic geochemical and isotopic compo- global cooling (Schwartzmann and Volk, 1991). sition gives clear evidence of a photosynthetic component (Prashnowsky and Schidlowski, 1967). The potent greenhouse gas CH4 was produced by methanogens, detected isotopically 5.18.3.4 Cambro-Ordovician Greenhouse in a paleosol dated at 2,765 Ma (Rye and Hol- Paleosols land, 2000). Later, plausibly lichenlike and car- bon-sequestering organisms are represented by The most obvious way in which Ordovician enigmatic, small (1 0.5 mm), encrusted, and paleosols differ from those of the Precambrian ellipsoidal objects in the 2,200 Ma Waterval is in the local abundance of animal burrows. Onder and correlative paleosols (Retallack and Because burrows are known in Late Pre- Krinsley, 1993; Gutzmer and Beukes, 1998). A cambrian marine rocks, the main problem in later swing to greenhouse conditions could be establishing the presence of animals on land inferred from molecular sequence data for a during the Ordovician was to prove that the Mid- to Late Precambrian (1,458–966 Ma) burrows were formed at the same time as the origin of ascomycete fungi, after the origin of paleosols, and not during inundation before or 12 Soils and Global Change in the Carbon Cycle over Geological Time after soil formation. This evidence came in part community of microbial soil respirers. Burrows from petrographic studies of soil carbonate in are not obvious in the Late Ordovician Iron the paleosols, which is cut by some burrows Knob paleosol of Wisconsin, but the short dis- and cuts across other burrows (Figure 8). This tance of attenuation to atmospheric values of 13 carbonate is a largely micritic mixture of calcite CO2 mole fraction and d C values of carbon in and dolomite, as is common in pedogenic car- goethite of that paleosol (Figure 6) indicate soil bonates (Retallack, 1985). Compelling evidence respiration rates comparable to those of mod- also came from the isotopic composition of ern savanna grassland soils (Yapp and Poths, carbon in this carbonate, which was isotopi- 1994). This is remarkable, because there are no cally too light to have formed in aquatic or clear root traces in Ordovician paleosols, and marine environments (Retallack, 2001c). Com- palynological evidence indicates no more than parable burrows and tracks of millipedelike a cover of liverwort-like plants to feed such soil creatures have now been reported in several respiration (Strother et al., 1996; Strother, Ordovician paleosol sequences (Johnson et al., 2000). Primary carbon fixation by these 1994; Trewin and McNamara, 1995; Retallack, thin thalli with short root hairs could not have 2000a), but these were probably only a small created a quantity of biomass or humus com- part of the overall soil respiration of Ordovi- parable to that of modern grasslands. Further- cian paleosols. Glomalean fungi discovered more, organic-lean, red Ordovician paleosols in Ordovician marine rocks of Wisconsin (Re- contain only sparse reduction spots and soil decker et al., 2000) were also part of an active carbonate nodules (Retallack, 1985; Driese and

10 µm 100 µm Tetrahedraletes Hypothetical grayae liverwort

10 mm

Hypothetical millipede

Bk 5 mm Scoyenia C horizon beerboweri

cm

No vertical exaggeration

Figure 8 Reconstructed ecosystem of the Late Ordovician Potters Mills paleosol from central Pennsylvania. Reproduced by permission of Palaeontological Association from Retallack (2000a). Record of Past Soil and Global Change 13 Foreman, 1992), indicating modest carbon root traces are small and shallow within the storage in soil organic matter and carbonate profiles (Figure 9b). The earliest known vascular compared, e.g., with modern savanna grassland land plants of the Middle and Late Silurian soils (de Wit, 1978). The Ordovician paleosols lacked true roots. Instead, they had stems that studied so far show unusually high soil respi- ran along the surface and just beneath the sur- ration, considering their probable low levels of face of the soil as runners and rhizomes fur- primary productivity. They also formed at a nished with thin unicellular root hairs (Kenrick time estimated from sedimentary mass balance and Crane, 1997). Plant bioturbation in soils models as the steamiest greenhouse period of only extended down to a few centimeters, but all Phanerozoic time, with B16 times the burrows of millipedes reached more deeply, and present atmospheric levels of CO2 (Berner and in some soils were more abundant than plant Kothavala, 2001). The carbon budget of traces (Retallack, 1985). In addition to detriti- known Ordovician paleosols would have con- vorous and perhaps also herbivorous millipedes tributed to this greenhouse. (Retallack, 2001c), Late Silurian soil faunas included predatory centipedes and spiderlike trigonotarbids (Jeram et al., 1990). Fungal 5.18.3.5 Terminal Ordovician Icehouse hyphae and spores in Silurian and Devonian Paleosols rocks indicate proliferation of chytrids and other fungi (Sherwood-Pike and Gray, 1985; Taylor Periglacial paleosols, unknown in Cambrian and Taylor, 2000). and Early to Middle Ordovician rocks, are Early Devonian paleosols have abundant found again in latest Ordovician (Hirnantian) traces of true roots, including woody tap roots rocks. Periglacial paleosols are best documented of a variety of land plants (Elick et al., 1998). in South Africa, where patterned ground and Root traces reached tens of centimeters down sand wedges are common in red beds of the into paleosols, extending greatly the depth of Pakhuis Formation (Daily and Cooper, 1976). the active rhizosphere and its associated The ice sheets extended over much of Africa mucigel of microbes. Among the numerous (Ghienne, 2003).The causes of this are roots of Early and Middle Devonian paleosols, especially enigmatic, because volcanic activity the burrows of soil fauna are less prominent increased through the Ordovician and the con- (Figure 9b). Devonian soils also have higher tinents were dispersed (Bluth and Kump, 1991), clay content and are more deeply weathered of thus working against cold Late Ordovician bases than Silurian or Ordovician soils (Figure poles. Mass balance models make the Ordovi- 9a). They have isotopically lighter pedogenic cian ice age seem particularly enigmatic, be- carbon, closer to the isotopic composition of cause they predict atmospheric CO2 levels 16 coexisting organic carbon, than Silurian and times PAL (Berner and Kothavala, 2001). This Ordovician paleosols (Mora et al., 1996; Mora may be an artifact of the 10 Ma spacing of data and Driese, 1999). Within the parameters of the points in the model, blurring the o10 Ma du- pedogenic carbonate palaeobarometer of Cer- ration of the ice age that is indicated by carbon ling (1991), these data indicate declining at- isotopic data (Brenchley et al., 1994). Studies of mospheric levels of CO2 from the Silurian into carbonate isotopic compositions from paleosols the Devonian (Figure 9c). Consumption of at- within the glacial interval are needed to re- mospheric CO2 by increased hydrolytic weath- examine this question. Also needed is an exam- ering, and burial of carbon in limestone and ination of paleosols within this interval for organic matter during the Silurian and Devon- evidence of fossil mosses, which would have ian has been widely interpreted as an instance been more deeply rooted than liverworts and of atmospheric global change induced by the so have accelerated weathering and carbon of life (Retallack, 1997b; Berner, sequestration. Rare Late Ordovician mosslike 1997; Algeo and Scheckler, 1998). megafossils (Snigirevskaya et al., 1992) and spores (Nøhr-Hansen and Koppelhus, 1988) support indications from cladistic analysis 5.18.3.7 Late Devonian to Permian Icehouse (Kenrick and Crane, 1997) for a latest Ordovi- Paleosols cian origin of mosses. Periglacial paleosols and glaciogene sedimen- tary facies unknown in Silurian and Early 5.18.3.6 Siluro-Devonian Greenhouse to Middle Devonian appear in the latest Paleosols Devonian, and remain locally common in and Permian rocks, especially Root traces of vascular land plants appear in within the Gondwana supercontinent, then po- Silurian paleosols, but until the Early Devonian, sitioned near the south pole (Figure 10; Krull, 14 Soils and Global Change in the Carbon Cycle over Geological Time

0.3

io Alumina/bases 0.2 30 20 0.1

Clay content 10 Volume % Volume Molecular rat 0 0 (a)

30 Rooting depth 1

20 Root trace density 0.5

10 Depth (m) Depth Volume % Volume Burrow density (b) 30

20 Paleosol carbon isotopes 20 Mass balance

10 model 10 Times present Times atmospheric level atmospheric (c)

30 Maximum thickness 10 (m) Average First peat 20 thickness (permineralized) 5 10

Average (m) Maximum (d)

2 Stems and 2 trunks

1 1

Maximum

diameter (m) Roots and rhizomes (e)

First 200 First 200 seeds First First trees Woody clades land vascular

100 plants plants 100 Number

Herbaceous clades (f)

60 Insects 60 Myriapod Myriapod 40 tracks fossils Tetrapods 40 Myriapod Arachnids Number 20 burrows 20

450 400 350 300 Ma Ordovician Sil. Devon. Carbonifer. Perm. (g) Figure 9 Early Paleozoic changes in (a) soil differentiation as indicated by clay content (vol.%) and alumina/ bases (molar ratio) of the most weathered horizon of calcareous red paleosols; (b) soil bioturbation as indicated by proportion of transect in paleosols occupied by roots or burrows (percent) and by measured rooting depth (m); (c) atmospheric CO2 levels (PAL) calculated from a sedimentary mass balance model; (d) maximum coal seam thickness and average thickness of at least 10 consecutive seams (m); (e) diameter of fossil plant stems and roots (m); (f) diversity of fossil land plants (number of species); (g) diversity of soil animals (number of families). Reproduced by permission of American Association for the Advancement of Science from Retallack (1997c).

1999). However, unlike periglacial paleosols plants. The earliest documented examples of of the Ordovician and Precambrian, these tundra (polar shrubland) vegetation have been Late Paleozoic profiles include root traces of found in paleosols with freeze–thaw banding what must have been frost-hardy woody and thufur mounds in Carboniferous glacigene Record of Past Soil and Global Change 15

Figure 10 Deep clastic dike in a coal of the Weller Coal Measures of the Allan Hills, , interpreted as infill of periglacial polygonal patterned ground (E. S. Krull for scale). sedimentary rocks near Lochinvar in south- Latest Devonian paleosols also include coals eastern Australia (Retallack, 1999a). Taiga from the oldest woody peats. Thin peats of (polar forest) paleosols with discontinuous per- herbaceous plant remains such as the Rhynie mafrost deformation are found in Early Perm- Chert of Scotland (Rice et al., 1995) and the ian red beds near Kiama, also in southeastern Barzass coal of Siberia (Krassilov, 1981) are Australia (Retallack, 1999b). found in Early Devonian rocks, but by the lat- Milankovitch-scale temporal variation in cli- est Devonian (Algeo and Scheckler, 1998) and mate and sea level has long been recognized in into the Carboniferous, woody coals became cyclothemic sedimentation in North American widespread and thick (Figure 9d). Carbon con- paleotropical Carboniferous marginal marine sumption by accelerated weathering in forest sequences, and this in turn has been related soils and carbon burial in coals are widely ac- to ice-volume fluctuations on the south polar knowledged as the likely cause for mass bal- Gondwana supercontinent (Rasbury et al., ance estimates of Late Paleozoic high 1998; Miller and West, 1998). Full glacial coal atmospheric oxygen levels (perhaps 35 vol.%) seams (Histosols) alternating with interglacial and near-modern CO2 levels (Berner et al., marine rocks are a clear indication of these 2000). Low Permian atmospheric CO2 levels changes. Environmental alternations of full- are also confirmed by stomatal index studies glacial, dry, calcareous, swelling-clay soils (Retallack, 2001b). These atmospheric trends (Vertisols), and interglacial, wet, decalcified, and coeval changes in oceanic Mg/Ca ratio forest soils (Alfisols) indicate a terrestrial could be attributed to changes in volcanic and contribution to multimillenial-scale change in hydrothermal activity, particularly at mid- atmospheric greenhouse gases and paleoclimate ocean ridges (Stanley and Hardie, 1999). (Retallack, 1995). However, the abundance of Early Paleozoic By Middle Devonian time, the evolution of pedogenic dolomite, but Late Paleozoic and increasingly larger plants culminated in trees Neogene pedogenic calcite (Retallack, 1985, with trunks up to 1.5 m in diameter, which 1993), suggests a role for soils in these changes leave obvious large root traces in paleosols in oceanic ionic chemistry, as well as in (Driese et al., 1997), as well as abundant per- changing atmospheric CO2 levels. mineralized stumps and logs (Meyer-Berthaud et al., 1999). Middle Devonian paleosols are also the oldest known with clay-enriched sub- surface horizons (argillic horizons of Soil 5.18.3.8 Triassic–Jurassic Greenhouse Survey Staff, 1999). The clay in modern forest Paleosols soils is partly formed by weathering in place, and is partly washed down root holes, which Greenhouse paleoclimates right from the taper strongly downward in forest trees. Evid- very beginning of the Mesozoic have been ence of both neoformation and illuviation of revealed by discovery of deeply weathered clay can be seen in thin sections of Devonian paleosols in earliest Triassic rocks of Antarc- forested paleosols (Retallack, 1997b). tica (Figure 11), which even at that time was at 16 Soils and Global Change in the Carbon Cycle over Geological Time

Organic Al2O3 13 carbon + + Field observations CPDB CaO MgO Percent + organic (‰) (%) Na2O K2O Ba/Sr grain size −35 −25 −15 0.5 1 350 5 10 0 50 100 Clay Silt Sand Gravel 0.1 cm Sand 0 A

Clay Bt

50

leosol Silt

C 100

John pa clay

150

Trough cross bedding Wavy bedding Planar bedding Woody root traces Burrow Figure 11 Geochemical (isotopic, major, and trace element) and petrographic (point count) data for a deeply weathered paleosol which formed at a latitude of 701 S in the Allan Hills of Antarctica during the Early Triassic. This is the John paleosol, an Ultisol (Sombrihumult), as indicated especially by its high ratios of alumina to bases and barium to strontium, and its strong subsurface enrichment in clay. Extremely light carbon isotopic values deep in the profile imply a role for methanogenic methane in this postapocalyptic greenhouse. Reproduced by permission of Geological Society of America from Krull and Retallack (2000). paleolatitudes of 65–771 S(Retallack and Release mechanisms for methane could have Krull, 1999). Comparable modern soils are included meteorite impacts, Siberian Traps vol- Ultisols (Soil Survey Staff, 1999) and Acrisols canism, or continental shelf collapse, which also (FAO, 1988), which are not found either have been invoked as causes for extinctions at north of 481 N latitude or south of 401 S, and this time (Hallam and Wignall, 1997). Really are rare outside subtropical regions. Green- large life crises were also times of transient house conditions at this time are also indicated global greenhouses indicated by stomatal index by stomatal index studies of fossil seed ferns data (Retallack, 2001b) at the earliest Jurassic (Retallack, 2001b) and the isotopic composi- (Pliensbachian), Early Jurassic (Toarcian), tion of carbon and oxygen in marine and Mid-Jurassic (Bathonian), Early Cretaceous nonmarine carbonate and organic matter (Aptian), Mid-Cretaceous (Cenomanian–Turo- (Holser and Scho¨ nlaub, 1991). nian), earliest Paleocene (Danian), and earliest The timing and magnitude of this greenhouse Eocene (Ypresian). During the Early Mesozoic, and isotopic excursion immediately at and after atmospheric CO2 minima also were high (at the greatest mass extinction of all time has least twice that of the present), and this general suggested a catastrophic release of methane and long-term greenhouse calls for a different from permafrost or marine clathrate deposits and noncatastrophic explanation. Paleosols and (Krull and Retallack, 2000; Krull et al., 2000). permineralized wood of forest ecosystems at There is no other source of carbon that is suf- high latitudes provide evidence for this long- ficiently large and isotopically depleted to create term greenhouse during which no periglacial the observed negative carbon isotopic anomaly. paleosols are recorded (Ollier and Pain, 1996; Record of Past Soil and Global Change 17 Retallack, 2001a). The Triassic appearance of mid-Cretaceous greenhouse was unusually long large sauropod dinosaurs such as Mass- and profound, judging from the stomatal index ospondylus and Plateosaurus, together with of fossil ginkgo leaves (Retallack, 2001b). Vol- footprints and other dinoturbation (Lockley, canic activity that created the enormous On- 1991), and of a variety of termite and ant nests tong–Java Plateau has been cited as a cause for in paleosols (Hasiotis and Dubiel, 1995), would this long-term greenhouse (Larson, 1991), but have effectively increased the destruction of there is another plausible explanation in the woody tissues in and on soils (Olsen, 1993). The co-evolution with angiosperms of ornithopod effect of such evolutionary innovation may dinosaurs such as Iguanodon, with their im- have been to decrease carbon sequestration by pressive dental batteries for processing large lignin in swamps, forests, and their soils. amounts of foliage. The feeding and trampling efficiency of these large, newly evolved dino- saurs may have further promoted the spread of early angiosperms with their ability to tolerate 5.18.3.9 Early Cretaceous Icehouse Paleosols higher levels of disturbance than other plants (Bakker, 1985). Newly evolved ornithopod di- Fossil patterned and hummocky ground nosaurs and their trackways are associated reveal permafrost conditions during the Early with carbonaceous and early successional Cretaceous (Aptian) sediments of southeastern paleosols (Entisols, Inceptisols, and Histosols), Australia, which at that time was at 66–761 S whereas archaic sauropod dinosaurs and their and attached to the Antarctic portion of the trackways remained associated with less fertile Gondwana supercontinent (Rich and Vickers- and less carbonaceous paleosols (Aridisols) Rich, 2000). This ice age does not appear to throughout the Cretaceous (Retallack, 1997c). have been as extensive or severe as the Permo- Other times of unusually extensive tropical Carboniferous or modern ice ages. This episode paleosols were the latest Paleocene (55 Ma; of planetary cooling coincides with a dramatic Taylor et al., 1992), latest Eocene (35 Ma; Best- evolutionary radiation of flowering plants land et al., 1996; Retallack et al., 2000), and (Retallack and Dilcher, 1986; Truswell, 1987; Middle (16 Ma; Schwarz, 1997). These Crane et al., 1995). The key evolutionary events are notable as short-lived ( 0.5 Myr) innovation of flowering plants was an ab- o spikelike warmings in both stable isotopic breviated life cycle, in which pollination, ferti- records from the ocean (Veizer et al., 2000; lization, and germination followed one another Zachos et al., 2001) and stomatal index in quick succession (Wing and Boucher, 1998). studies (Retallack, 2001b). The latest Paleocene Early angiosperms were largely confined to warm spike is associated with such profound weakly developed soils (Entisols) of disturbed carbon isotopic lightening that it can only coastal and streamside habitats, which they reasonably be attributed to the methane from colonized and weathered more rapidly than as- isotopically light methane clathrates from sociated conifers and cycadlike plants (Retal- ocean floor sediments, permafrost, or volcanic lack and Dilcher, 1981). Angiosperm leaves intrusion (Koch, 1998). Short-term physical were less coriaceous and less well defended with forcings are thus also recorded in the paleosol resins and other toxins, and so rotted more record of paleoclimate. rapidly to create a richer soil humus than leaves of conifers and cycadlike plants (Knoll and James, 1987). Erosion control and soil humifi- cation from newly evolved angiosperms may 5.18.3.11 Neogene Icehouse Paleosols have played a role in Early Cretaceous chilling. Periglacial paleosols appear during Late Mi- ocene time (8 Ma) in Antarctica (Sugden et al., 1995; Retallack et al., 2001), where soil 5.18.3.10 Cretaceous–Paleogene Greenhouse development is so slow that some surface soils Paleosols may be of comparable antiquity (Campbell and Claridge, 1987). Antarctic soil formation is not Another long period of generally warmer only promoted by ground ice deformation, but planetary climates without evidence of polar ice includes the effects of salt accumulation and caps or periglacial paleosols lasted from the eolian mass addition in an extremely dry con- Mid-Cretaceous to the latest Eocene. Mid-Cre- tinental frigid climate (Figure 12). taceous (Cenomanian) tropical paleosols (Ulti- The Late Miocene is best known for the sols and Oxisols) are known from South Messinian salinity crisis, when the Mediterra- Australia, then at 601 S(Firman, 1994), and nean Sea became a desert (Krijgsman et al., the United States, then at 451 N(Thorp and 1999). It was also a significant time for geogra- Reed, 1949; Joeckel, 1987; Mack, 1992). The phic and climatic expansion of grassland Molecular weathering ratios Al O Na O 2 3 2 Al O FeO Field observations Point count data CaO + MgO 2 3 CaO + MgO + Ba/Sr Percent Percent K2O SiO Fe O Munsell color Al O 2 Na O + K O 2 3 Sil dilation Weathering grain size composition 2 3 2 2 ε ε ( Zr & Ti) rinds (mm)

Silt Sand Gravel Clay 50 50 0 5 10 0 5 10 0.1 0.3 5 155510 15 0 0.2 0.4 1 2

cm Very pale brown Samples R- 2,364 (10YR7/3) 0 Light brown 2,365 (7.5YR6/4) A Gray (5Y6/1) 2,366 Sand-filled clastic Ti dikes grayish brown (2.5Y5/2) Bw Brown (7.5YR5/4) 2,367 Zr 50

Sand

agments 2,368

Gravel

Light yellowish By fr Rock

brown (10YR6/4) 2,369 Silt 100 2,370 16

Dark gray

(5Y4/1) C Quartz 2,371

Clay Feldspar Sand Pyroxene and hornblende Gypsum

Figure 12 Geochemical data for the Siesta paleosol of age (3 Ma) from the Meyer Desert Formation at Oliver Bluffs, central Transantarctic Mountains. Reproduced by permission of Geological Society of London from Retallack et al. (2001). Record of Past Soil and Global Change 19

Overlying loessic sediment

Dark brown crumb- textured mollic

epipedon (A horizon) 79 cm 79

Calcareous nodules (Bk horizon)

Figure 13 Tall grassland (Mollisol) paleosol with thick, dark brown crumb-textured surface over a deep (79 cm) white nodular calcic horizon, over a thinner short grassland paleosols with carbonate nodules at a depth of 39 cm, in the Late Miocene (7 Ma) Ash Hollow Formation, 13 km north of Ellis, Kansas. biomes and their characteristic soils: Mollisols form at shallow depths within soil profiles in of Soil Survey Staff (1999) or Chernozems of dry climates and deeper within the profile in FAO (1988). Evidence for this transformation more humid climates (Jenny, 1941; Retallack, in tropical regions comes from the dramatic 1994c). Observations of depth to carbonate change to a less depleted (less negative) carbon horizon together with root traces and crumb isotopic composition (d13C) of pedogenic car- peds of grassland paleosols can be used to con- bonate and organic matter, and of the apatite strain the paleoclimatic range of grasslands of fossil mammalian tooth enamel attributed to (Retallack, 1997d, 2001d). the tropical expansion of C4 grasses (Cerling Observations on hundreds of paleosols in the et al., 1997; MacFadden, 2000). There is also North American Great Plains, Oregon, Paki- evidence from adaptations to grazing in fossil stan, and East Africa have revealed a broad mammals (Janis et al., 2002), from traces of schedule of origin and paleoclimatic expansion grassland invertebrates such as dung beetles of bunch and then sod grasslands (Figure 14). (Genise et al., 2000), and from increased abun- The increased organic carbon content, high in- dance of silica bodies (phytoliths) and pollen ternal surface area, elevated albedo, and greater characteristic of grasses (Stro¨ mberg, 2002). water retention capacity of grasslands com- Paleosols also demonstrate Late Miocene pared with woodlands of comparable climatic expansion of grasslands capable of forming sod regions would have been a potent force for of the sort that is unrolled to create lawns and global cooling as grasslands emerged to occupy golf courses. The dense growth of fine (o2mm almost a quarter of the current land area (Best- diameter) adventitious roots, together with the land, 2000; Retallack, 2001d). Mountain uplift slime of abundant earthworms, create a char- and ocean currents played a role in Neogene acteristic soil structure consisting of fine crumb climate change as well (Raymo and Ruddiman, peds, which can be preserved in paleosols 1992; Ramstein et al., 1997), but there remain (Figure 13). Grassland soils are also unusually problems with the timing and magnitude of rich in organic matter, intimately admixed with carbon sequestration by these physical mecha- clay, often with as much as 10 wt.% C down to nisms (Retallack, 2001d). a meter or more, although this organic matter is not always preserved in paleosols. The soft, low-density upper horizons of grassland soils 2 þ 2 þ are also rich in mineral nutrients (Ca ,Mg , 5.18.3.12 Pleistocene Glacial and Interglacial þ þ Na , and K ), and their subsurface horizons Paleosols commonly include nodules of soil carbonate (usually micritic low magnesium calcite). It has Over the past million years, large ice caps long been known that such pedogenic nodules have grown to engulf the present-day location 20 Soils and Global Change in the Carbon Cycle over Geological Time

10 m Pliocene Woodland Desert Desert Short sod grassland Tall sod grasssland scrub grasssland

Height

Depth 1 m

Woodland 10 m Miocene Dry woodland Desert Desert Short sod grassland scrub grasssland

Height

Depth 1 m

Woodland 10 m Dry woodland Oligocene Desert Desert scrub grasssland

Height

Depth 1 m

Woodland 10 m Eocene Desert Mallee woodland scrub

Height

Depth 1 m 200 400 600 800 Mean annual precipitation (mm)

Non-mollic Near-mollic Mollic Sediment soil soil brown soil

Carbonate nodules Figure 14 A scenario for climatic and geographic expansion of grasslands and their soils in the Great Plains of . Reproduced by permission of Society for Sedimentary Geology from Retallack (1997d). of Chicago within more than a kilometer of ice extreme paleoclimatic oscillations on the other during glacial maxima, then retreated to the Milankovitch frequencies of 42 and 23 ka (Hays current ice caps of Greenland and Alaska et al., 1976; Petit et al., 1999). In Illinois, in- during interglacial times at Milankovitch scale terglacials are defined by paleosols such as the frequencies of 100 ka. There have also been less Sangamon paleosol, which is comparable with Soils and Global Carbon Cycle Changes 21 modern forest soils under oak–hickory forest. 5.18.4 SOILS AND GLOBAL CARBON The 42 and 23 ka interstadials are defined by CYCLE CHANGES paleosols such as the Farmdale paleosol, which is comparable with modern boreal forest paleo- Over geological time there have been dra- sols under spruce forest (Follmer et al., 1979). matic changes in soil, life, and air that are well Ice, till, loess, and periglacial soils (Gelisols) al- represented in the fossil record of soils. Paleo- ternated with forest soils (Alfisols or Incepti- sols are an underexploited record of past sols) through these paleoclimatic fluctuations. environments in land. This review has empha- Oscillations between different ecosystems sized mainly the evidence from paleosols for can be inferred from many paleosol sequences, changes in carbon cycling and greenhouse gases even beyond the ice margin (Figure 15). In the (CO2,CH4, and H2O) in the atmosphere over Palouse loess of Washington, for example, geological timescales. It is unremarkable that grassland soils (Mollisols) with crumb peds paleosols would change, particularly at high and earthworm castings during latitudes, as global climates warmed or cooled and interstadials alternate with sagebrush soils with changing atmospheric loads of greenhouse (Aridisols) with cicada burrows and shallow gases. It is notable that sequences of paleosols carbonate horizons during glacials and inters- can, under certain circumstances, be high-res- tadial minima (Busacca, 1989; O’Geen and olution records of such paleoclimatic change Busacca, 2001). Vegetation of the paleosols can (Figure 15). Parallels between biological activ- be inferred from carbon isotopic values typical ity within soils and greenhouse gas composition for CAM saltbush in the sagebrush paleosols, have been emphasized in this review as fertile and for C3 grasses in the grassland paleosols, as ground for future research (Figure 16). Olsen well as from the characteristic phytoliths of (1993) has suggested that soil producers such as these plants (Blinnikov et al., 2002). Compara- plants cool the planet, but soil consumers such ble alternations of ecosystems with paleocli- as animals warm it. This idea, which the author matic fluctuation are seen in many has dubbed the Proserpina principle after the sequences of paleosols (Paepe and van Over- ancient Roman goddess of spring (Retallack, loop, 1990; Feng et al., 1994; Wang et al., 2000b), is undeniable for the annual spring fall 1998). Differences in primary production and and autumn rise of atmospheric CO2 with carbon sequestration of these alternating northern hemisphere leaf sprouting and shed- ecosystem types on a global basis may have ding (Figure 2a). This explanation is especially played a role in the relative abundance of demonstrated by the muted and out-of-phase greenhouse gases during glacial–interglacial annual fluctuation of CO2 in the southern hem- paleoclimatic cycles. isphere (Mooney et al., 1987), where there is Ice core records show as little as 180 ppmv less fertile land, more evergreen plants, and CO2 during glacial periods and 280 ppmv different seasons. The question addressed here during interglacials, in a strongly asymmetric is whether the Proserpina principle operates on pattern of gradual drawdowns followed by geologically significant timescales, and so far, steep rises known as terminations (Figure 2b). such a simple idea does not conflict with the Even higher CO2 levels during interglacials are and paleoclimate outlined here. prevented by high plant productivity of forests On evolutionary timescales, it is the biochem- in humid, previously glaciated terrains and of ical evolution of lignin, pyrethrin, caffeine, and grasslands in arid rangelands. This slow weath- other substances that deter herbivory, digestion, ering and biomass building, together with nu- and decay, which affect rates of carbon burial in trient leakage to the ocean and carbon burial sediments as the principal long-term control on there, could draw down greenhouse gases and atmospheric CO2 levels. The role of trees and bring on cooling. As ice expands and grass- their soils in Late Paleozoic carbon sequestra- lands are converted into deserts, the carbon tion, cooling, and glaciation is widely accepted sequestration capacity of soils and ecosystems (Berner, 1997; Algeo and Scheckler, 1998; see is diminished. Large herds of mammals or Chapter 5.06). The role of humans in global populations of humans could disturb these warming is also becoming well known (Vit- impoverished soils into dustbowl conditions ousek et al., 1997b). According to the Proser- and the massive carbon oxidation events of a pina principle, humans may not have been the glacial termination. Such long-term biological only organisms to have had significant effects trends, metered by steadily declining and then on climate. There remain many other instances abruptly renewed soil nutrients, could amplify of global change less clearly related to changes other drivers of climate, which include large in life and soils, in part because the numerous ice caps, ocean currents, mountain building, paleosols of appropriate age have not yet been and orbital configuration (Muller and Mac- studied in detail. Asteroid impacts, volcanic Donald, 2000). eruptions, and methane outburst events also Carbon Oxygen Earthworm Cicada Kahlotus, Washington Calcareousness isotopes isotopes fecal pellets burrows 13 18 CPDB OPDB Soil development Hue Grain size carbonate (‰) opal (‰) Marine oxygen

m −8 −6 −4 −5 −3 −1 isotope

Weak

Weak 50% Strong Strong Gravel

Rare Rare Clay

Silt 10YR 10R Common Common Sand stage 0 NIX

1 NIX 14.0 ± 2.4 ka 12 ka MSH-S ash 17.2 ± 1.9 ka Silt 2

TLAL

(40.1 ka) Clay (46.0 ka) NIX

5 NIX

MSH-C ash 40.8 ± 4.7 ka NIX 3 49.2 ± 7.7 ka Sand 59 ka

TLAL 4 Silt

10 NIX early MSH ash 5 (83.2 ka) NIX

NIX

Little weathered Caliche with Blocky-structured Crumb-structured volcanic ash cicada burrows reddish paleosol brown paleosol

Figure 15 Alternating paleoenvironments of desert CAM shrublands and C3 grasslands represented by a sequence of Quaternary paleosols (0–100 ka) in the Palouse loess near Kahlotus, Washington, USA; showing (left to right), field section with thermoluminescence dates and paleosol identification (NIX and TLAL are pedotypes for buried Mollisols of grasslands and Aridisols of sagebrush respectively), paleosol position and development (represented by black boxes), paleosol calcareousness (scale based on acid reaction), Munsell hue (measured dry in field), sand–silt–clay proportion, d13C of pedogenic carbonate, d18O of opal phytoliths, abundance of earthworm pellets, and abundance of cicada burrows. Source: Retallack (2001c). References 23

Archaean Archaean actinobacteria Archaean actinolichens? Archaean methanogens 106 Paleoproterozoic paleosol problematica ascomycetes? Neoproterozoic lichens? Ordovician millipedes Ordovician mosses 105 Devonian chytrid fungi Devonian trees and swamps Triassic sauropods and termites Cretaceous angiosperms (ppmV) 4 2 10 Cretaceous ornithopods Oligocene grasslands Eutrophic forest, swamp, grassland Oligotrophic forest, bog, desert 103 Holocene eutrophic ecosystems Glacial terminations Autumn leaf fall

Spring budding Atmospheric CO Atmospheric

Altithermal Little ice age Global warming 102 109 108 107 106 105 104 103 102 10 1 Millions Centuries Decades Years before present

Figure 16 The Proserpina principle relates variation in atmospheric CO2 concentration with coeval evolutio- nary and ecological events on a variety of timescales. Carbon sequestering evolutionary innovations and ecological transitions (closed symbols) alternate with carbon oxidizing evolutionary innovations and ecological transitions (open symbols). The CO2 curve is a composite of those shown in Figure 2 and by Kasting (1992). affect life and the carbon cycle, producing tran- Barley M. E., Pickard A. L., and Sylvester P. J. (1997) sient greenhouse events (Retallack, 2001b). Emplacement of a large igneous province as a possible cause of banded iron formation 2.45 billion years ago. Ocean currents and mountain building also Nature 385, 55–58. are likely to play a role in carbon sequestration Barsukov V. L., Volkhov V. P., and Khodakovsky I. L. (Raymo and Ruddiman, 1992; Ramstein et al., (1982) The crust of Venus: theoretical models of chemical 1997). Soils and their ecosystems play an im- and mineral composition. J. Geophys. Res. Suppl. 87A, portant role in the carbon cycle today, and the 3–9. Basilevsky A. T., Kuzmin R. O., Nikolaeva O. V., Pronin history of that role now decipherable from A. A., Ronca A. B., Avdvesky V. S., Uspensky G. R., paleosols appears ripe for modeling and other Cheremukhina Z. P., Semenchenko V. V., and Ladygin quantitative comparisons with other likely con- V. M. (1985) The surface of Venus as revealed by trols on global paleoclimate change. the Venera landings. Part II. Geol. Soc. Am. Bull. 96, 137–144. Bell J. F. (1996) Iron sulfate, carbonate and hydrated min- ACKNOWLEDGMENTS erals on Mars. In Mineral Spectroscopy: A Tribute to Roger G. Burns (eds. M. D. Dyar, C. MacCammon, and Nathan Sheldon, Hope Jahren, and Tim M. W. Schaeffer). Geochem. Soc. Spec. Publ., vol. 5, pp. 359–380. White have been sounding boards for the ideas Berner R. A. (1997) The rise of plants and their effect on presented here. I also thank J. I. Drever and weathering and atmospheric CO2. Science 276, 543–546. H. D. Holland for helpful reviews. Berner R. A. and Kothavala Z. (2001) GEOCARBIII: a revised model of atmospheric CO2 over Phanerozoic time. Am. J. Sci. 301, 182–204. REFERENCES Berner R. A., Petsch S. T., Lake J. A., Beerling D. J., Popp B. N., Lane R. S., Laws E. A., Westley M. B., Cassor N., Algeo T. J. and Scheckler S. E. (1998) Terrestrial–marine tele- Woodward F. I., and Quick W. P. (2000) Isotopic frac- connections in the Devonian: links between the evolution of tionation and atmospheric oxygen: implications for land plants, weathering processes and anoxic events. Phil. Phanerozoic evolution. Science 287, 1630–1633. Trans. Roy. Soc. London B 353, 113–130. Bestland E. A. (2000) Weathering flux and CO2 consump- Allen J. R. L. (1974) Geomorphology of Siluro-Devonian tion determined from paleosol sequences across the alluvial plains. Nature 249, 644–645. Eocene–Oligocene transition. Palaeogeogr. Palaeo- Amundson R., Stern L., Baisden T., and Wang Y. (1998) climatol. Palaeoecol. 156, 301–326. The isotopic composition of soil and respired CO2. Bestland E. A. and Retallack G. J. (1993) Volcanically Geoderma 82, 83–114. influenced calcareous paleosols from the Miocene Bakker R. T. (1985) The Dinosaur Heresies. William Kiahera Formation, Rusinga Island, Kenya. Geol. Soc. Morrow, New York. London J. 150, 293–310. 24 Soils and Global Change in the Carbon Cycle over Geological Time

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