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    Do red beds indicate paleoclimatic conditions?:

    A Permian case study

     Nathan D. Sheldon*

     Department of Geology, Royal Holloway University of London, Egham, Surrey TW20 0EX, United Kingdom

    Received 27 September 2004; received in revised form 25 February 2005; accepted 16 June 2005

    Abstract

    Terrestrial red beds have long been interpreted as desert deposits by comparison with modern red deserts. More recently red

     beds have been interpreted as evidence of seasonally dry conditions and a Permo–Triassic Pangean monsoon. Red beds of Cala

    Viola, Sardinia are identified as paleosols and used to reconstruct Late Permian paleoclimatic conditions. Reconstruction of 

     paleoenvironmental conditions based on the paleosols of the Cala Viola indicates warm, humid conditions with no evidence of 

    dry conditions, as in a desert, or of extreme seasonality as in a monsoon. Instead, it is suggested that the red color of the

     paleosols is a result of former good drainage, and that red color in general does not indicate specific paleoclimatic conditions.

    D 2005 Elsevier B.V. All rights reserved.

     Keywords:  Permian; Sardinia; Paleosols; Paleoclimate; Monsoon

    1. Introduction

    A long held dogma is that widespread Triassic

    terrestrial red beds indicate a global transition to warm-

    er and drier conditions than those that characterized the

    Permian (Parrish, 1995). This new climatic system has

     been termed the Pangean mega-monsoon (Kutzbachand Gallimore, 1989). The question to be addressed

    herein is whether red color alone is sufficient evidence

    upon which to base paleoclimatic interpretations.

    Early research on modern red deserts supported the

    interpretation that ancient red beds formed in hot, dry

    climates (Walker, 1976). However, modern red deserts

    of Arizona and Australia are red because of sediments

    recycled from paleosols of Triassic and Miocene age,

    respectively, and most deserts of North and South

    America, Asia, and the Middle East are grey like

    their weathering source rocks. Further, many red

    soils in semi-arid areas such as New Mexico derivedtheir red color from well-drained, warm conditions

    during Pleistocene pluvials, so the red color is relict 

    and related to earlier paleoenvironmental conditions.

    More recently,   Parrish (1998, p. 192)   stated that ter-

    restrial red beds,   b. . .appear to be indicative of cli-

    mates that are warm and dry or seasonal with respect 

    to rainfall. Q  A model put forth by   Dubiel and Smoot 

    (1994)  suggests that continental red bed formation is

    0031-0182/$ - see front matter  D   2005 Elsevier B.V. All rights reserved.

    doi:10.1016/j.palaeo.2005.06.009

    * Tel.: +44 1784 443615.

     E-mail address:  [email protected].

    Palaeogeography, Palaeoclimatology, Palaeoecology 228 (2005) 305–319

    www.elsevier.com/locate/palaeo

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    favored by warm climates with alternating wet-and-

    dry seasons (monsoons) and open, desert to savanna

    vegetation. However, it is not an exact analog because

    a true savanna requires grasslands, which did not evolve until the Cenozoic (Retallack, 2001a; Terry,

    2001). Monsoonal tropical Pakistan and India include

     both grey and red soils and   paleosols (Retallack,

    1991a).   Wynn (2000)   and   Wynn and Retallack 

    (2001)   describe reconstructed savanna ecosystems

    from Cenozoic paleosols in Africa that are not signi-

    ficantly reddened. Furthermore, numerous examples

    have been published of diagenetic reddening of non-

    desert paleosols by dehydration of iron oxyhydroxides

    (Retallack, 1991a, 1997, 2001b; see also the review of 

    older literature in Blodgett et al., 1993).Taken together, these various factors suggest that 

    the origin of red color may not be well-understood or 

    well-explained by existing models. Work presented

    here on Late Permian red beds in Sardinia offers an

    alternative explanation to pronounced aridity or sea-

    sonality. It is suggested that the red color is indicative

    of well-drained conditions and that it provides no

    unequivocal information on the paleoclimatic condi-

    tions at the time of paleosol formation. Instead, paleo-climatic conditions are reconstructed on the basis of 

    other proxies, such as the degree of chemical weath-

    ering, nature and extent of pedogenic carbonate and

    salts, and patterns of root traces and trace fossils.

    2. Geologic context

    Basin-and-Range topography was a result of the

    Carboniferous–Permian Hercynian orogeny from eastern

    Europe to the southern   coast of the United States(Cortesogno et al., 1998). Collision of South Europe

    with North America and Afr ica during the  Late De-

    vonian and Carboniferous (Condie, 1989)   was fol-

    lowed, through Triassic time, by local rifting and

    formation of continental basins in Spain, Southern

    Fig. 1. Map showing the location of field sites and stratigraphic column for the Lago di Baratz section, Verrucano Sardo Formation. LB01-15 are

    sample numbers, and Munsell colour of the sample is to the right of the sample number. The exact transition between the lesser developed

    Mosca Pesca and Lago di Baratz paleosols and the overlying Mácchia paleosols is unknown and may lie in the covered interval (shown with an

    X) rather than at the first logged Mácchia Rossa paleosol.

     N.D. Sheldon / Palaeogeography, Palaeoclimatology, Palaeoecology 228 (2005) 305–319306

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    France, Italy, Corsica, and Sardinia (Cassinis and

    Ronchi, 1997). These basins were filled with clastic

    red beds derived from the orogenic belt.

    In Sardinia, those sediments are part of the Verru-cano Sardo Formation exposed on the Cala Viola

    (bviolet bay Q )   (Fig. 1), and are divided it   into four 

    informal units (Gasperi and Gelmini, 1979). The red

     beds described in this paper are from   bUnit 2, Q  a 150

    m package of sediments composed of sandy conglom-

    erates, grey sandstones, and red sandstones and mud-

    stones. The Cala Viola Nord section is capped by a

    thick, quartz cobble conglomerate that is also exposed

    near the base of the Cala Viola Sud section (Fig. 1).

    The rocks exhibit fluvial paleochannels, tetrapod foot-

     prints, and fossil plants indicating subaerial depositionon alluvial fans and floodplains. Gasperi and Gelmini

    (1979)  examined the limited available fossil assem-

     blages and found Autunian (Early Permian) non-ma-

    rine strata near the base of the sequence and Triassic

    red claystones and sandstones near the top [Units 3

    and 4], overlain by   Middle Triassic (Anisian–Early

    Ladinian) limestone (Cassinis and Ronchi, 1997; Cas-

    sinis et al., 1992). The red beds described here are

    located near the top of the sequence  (top of Unit 2),

    and are thus Late Permian in age (Cassinis et al.,

    1992).

    The Lago di Baratz area (Fig. 1) is well vegetated

    and exposure is generally poor. Three of the four 

     pedotypes are exposed in this section (Fig. 1), includ-

    ing the Lago di Baratz and Mosca Pesca pedotypes,

    which are not preserved in either of the Cala Viola

    sections. In contrast, the Cala Viola sections, with

    localized gentle folding, are well-exposed in sea cliffs

    and rock platforms, and are continuous and conform-

    able with significant lateral variability difficult to

    capture adequately in single stratigraphic sections

    (Figs. 2 and 3). The Lago di Baratz section lies

    stratigraphically below the Cala Viola sections by anunknown thickness of mudstones and sandstones in

    Unit 2 of   Gasperi and Gelmini (1979).   However,

    given that only the middle and upper portions of 

    Unit 2 are red and the lower portion is primarily

    grey, it is possible that the red Mácchia paleosols of 

    the Lago di Baratz section (Fig. 1) represent the first 

    red beds. If this is the case, given the 75–85 m

    exposed in the Cala Viola sections (Figs. 2 and 3)

    and a total thickness of 150 m for Unit 2 (Gasperi and

    Gelmini, 1979), there can be no more than a few tens

    Fig. 2. Stratigraphic column for the Cala Viola Nord section,

    Verrucano Sardo Formation. Symbols and conventions are as in

    Fig. 1. Asterisks next to sample numbers indicate samples that were

    weakly reactive to dilute acid. The thicknesses of the conglomerate

    that caps the Cala Viola Nord and Sud sections are variable, so the

    average thickness is portrayed. Where multiple lithologies are

    shown, there is significant variability along strike and additional

    symbols apply to the right column, which represents the dominant 

    lithology.

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    of meters between the top of the Lago di Baratz

    section and the bottom of the Cala Viola Nord section.

    3. Methods

    Paleosols were recognized in the field on the basis

    of ped morphology, horizonation, root traces, and

    grain size changes (Retallack, 1997). Munsell color 

    was recorded as well as the qualitative degree of 

    calcareousness on t he basis of reaction with dilute

    hydrochloric acid (Retallack, 1997). Samples werecollected for petrography and geochemical analysis

    from three sites north of Alghero, near Lago di Barat z

    and at two localities on the Cala Viola (Fig. 1).

    Geochemical data were obtained from a commercial

    laboratory (Intertek of Vancouver, B.C.) using XRF,

    ICP-MS,   and titration (FeO) and are compiled in

    Table 1. Paleosols were classified   into pedotypes

    (Retallack, 1997; Retallack, 2001b)   on   the basis of 

     physical and chemical characteristics (Sheldon and

    Retallack, 2001; Sheldon et al., 2002),  and analyzed

    using the factor function approach (Jenny, 1941).Bulk density (q) was measured by the clod method

    using paraffin; analysis of 10 replicates of a single

    sample gave an uncertainty of 0.09 g cm3.

    4. Evidence of pedogenesis

    Paleosols in the Cala Viola sections fine up-profile

    and are notably finer  grained than the succession as a

    whole (Figs. 2 and 3). This difference shows up in the

    weathering profile of the sections as well (Fig. 4A)

    and in contrast to the fluvially-derived sandstones

    (Fig. 4B). Many of the paleosols also preserve drab-

    haloed root traces (Fig. 4C,F) and rarely, vertical

     burrows (Fig. 4C,D). Burrows range up to one cm

    in diameter and show some internal structure consis-

    tent with backfilling by an arthropod. Non-calcareous

    rhizoliths are well-preserved in some of the paleosols,

     both in hand specimen and thin section (Fig. 4H).

    Both root traces and burrows penetrate deeply into

     paleosol profiles (Fig. 4C), indicating that the paleo-

    water table was substantially below the surface. Point 

    counts of thin sections (e.g., Fig. 4E,H) are consistent with the field observation that paleosols are more fine-

    grained than interfluve sandstones, siltstones, and

    mudstones. Some of the Cala Viola paleosols have

    an observed clay bulge (Fig. 5)  and illuviation argil-

    lans observable in thin section consistent with subsur-

    face accumulation of clay in a Bt horizon. A and B

    horizons of paleosols have 80–97% clay and phyllo-

    silicate minerals and 3–20% quartz and lithics (includ-

    ing feldspars) with an average of less than 10%,

    whereas C horizons and other fluvial sediments all

    Fig. 3. Stratigraphic column for the Cala Viola Sud section,  Verru-

    cano Sardo Formation. Symbols and conventions are as in  Fig. 1.See Fig. 2   caption for additional information.

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    Table 1

    Geochemical data

    Sample Level

    (m)

    React a  Horizon SiO2   TiO2   Al2O3   Fe b FeO Fe2O3   MnO MgO CaO Na2O K 2O P2O5   LOI Total

    LB02 3.6 N 77.98 0.37 12.64 1.80 0.45 1.30 0.02 0.27 0.07 n/a 1.85 0.07 4.03 99.1

    LB03 4.4 N A/Bwc 78.63 0.30 9.62 4.81 0.39 4 .37 0.03 0.21 0.08 n/a 0.97 0.12 4.16 99.3

    LB04A 5.9 N C 66.80 0.70 14.89 7.30 0.51 6.73 0.05 0.60 0.16 0.10 2.75 0.15 5.79 99.8

    LB04B 6.0 N C 70.08 0.81 17.22 1.68 0.45 1.19 0.01 0.74 0.09 0.19 3.40 0.05 5.31 100.0

    LB04C 6.2 N A/Bw 69.27 0.84 17.08 1.73 0.51 1.16 0.02 0.66 0.06 0.20 3.56 0 .05 5.08 99.1

    LB04D 6.4 N A 67.22 0.70 15.35 6.52 0.58 5.88 0.05 0.59 0.09 0.08 2.88 0.11 5.66 99.8

    LB11 13.0 N C 75.11 0.52 14.21 2.83 0.45 2.33 0.03 0.62 0.11 0.03 2.48 0.07 4.29 100.8

    LB12 13.2 N C 66.15 0.72 16.84 5.58 0.71 4.79 0.02 1.14 0.12 0.14 3.95 0.08 4.99 100.4

    LB13 13.5 N C 61.17 0.80 18.76 6.54 0.71 5.75 0.02 1.40 0.08 0.17 4.82 0.06 5.27 99.8

    LB14 13.7 N Bw 62.34 0.79 18.84 5.15 0.90 4.15 0.02 1.30 0.10 0.21 4.69 0.06 5.93 100.3

    LB15 13.9 N A 61.20 0.78 18.63 7.02 0.64 6.31 0.02 1.32 0.08 0.15 4.70 0.08 5.30 99.9

    CV03 1.7 N Bw 58.00 0.92 19.18 6.61 0.84 5.68 0.05 1.81 0.90 0.16 5.22 0.06 6.67 100.4

    CV06 4.2 N 56.05 0.84 16.17 6.06 1.61 4.27 0.13 2.60 3.50 0.23 4.05 0.07 9.78 101.1

    CV07 5.5 N C 48.79 0.72 16.40 6.19 0.71 5.40 0.46 4.30 5.26 0.22 4.41 0.09 12.5 100.0

    CV08 5.8 N Bt 54.82 0.87 19.81 6.40 1.03 5.26 0.07 2.21 1.50 0.17 5.47 0.12 7.92 100.4

    CV09 6.1 N Bt 56.93 0.91 20.65 6.49 0.90 5.49 0.02 1.67 0.28 0.15 5.72 0.12 6.27 100.1

    CV10 6.5 N A 57.71 0.91 20.21 6.98 0.77 6.12 0.02 1.57 0.20 0.18 5.27 0.08 6.12 100.0

    CV13 10.1 N 56.05 0.91 19.22 6.32 0.90 5.32 0.07 2.00 1.31 0.16 5.30 0.08 7.39 99.7

    CV16 12.4 N C 55.56 0.78 14.59 6.55 1.74 4.62 0.18 3.03 4.20 0.32 3.79 0.04 10.7 101.4

    CV19 14.1 Y C 56.24 0.86 16.04 3.47 1.87 1.40 0.17 3.12 4.47 0.18 3.87 0.09 11.1 101.5

    CV22 17.2 Y Bt 30.48 0.47 9.25 3.30 1.03 1.51 0.91 10.6 15.5 0.29 2.26 0.06 26.7 100.8

    CV24 19.15 N C 56.12 0.59 13.94 4.64 1.42 3.07 0.18 3.27 5.08 0.26 3.58 0.05 11.4 100.5

    CV25 19.85 N Bt 51.90 0.63 11.69 4.83 0.51 4.26 0.34 4.77 7.67 0.19 2.89 0.07 14.2 99.7

    CV26 20.65 Y A 14.89 0.25 4.99 2.98 0.26 2.69 0.91 15.1 22.6 0.22 1.10 0.07 35.4 98.8

    CV27 22.05 Y Bt 56.94 0.89 19.69 7.98 0.77 7.12 0.02 1.44 0.29 0.09 5.79 0.14 5.82 99.9

    CV28 23.2 N C 53.35 0.83 15.45 5.58 0.77 4.72 0.06 1.50 1.90 0.22 4.24 0.09 6.61 90.6

    CV29 24.2 N Bt 59.56 0.89 19.87 6.59 0.64 5.88 0.03 1.24 0.19 0.17 4.95 0.12 5.43 99.7CV30 24.9 N Bt 57.89 0.93 20.01 8.35 0.58 7.71 0.03 1.20 0.14 0.12 4.77 0.11 5.75 99.9

    CV31 26.15 N 55.13 0.61 11.67 4.29 0.51 3.72 0.15 1.18 6.57 0.56 2.41 0.05 11.5 94.6

    CV45 46.5 N C 58.99 0.40 6.22 1.26 0.32 0.90 0.12 6.17 9.31 0.25 1.57 0.03 14.5 99.1

    CV46 48.0 N BC 58.65 0.71 12.04 3.43 0.45 2.93 0.09 4.28 5.56 0.59 2.85 0.04 9.89 98.6

    CV47 49.25 N Bw 83.50 0.26 8.57 1.23 0.45 0.73 0.01 0.28 0.22 0.05 1.57 0.03 2.75 99.0

    Sample Rho

    (g cm3)

    CIA K Clayeynessd (P

     bases/Al)d Salin.d Gleyd MAP MAT Bae Sr Y Nb Zr Rb

    LB02 2.52 0.095 0.22 0.16 0.77 132 66 25 28 164 112

    LB03 2.39 98.51 0.07 0.18 0.11 0.198 1540 15.3 76 36 18 18 141 72

    LB04A 2.58 0.13 0.33 0.21 0.17 351 92 31 21 257 137

    LB04B 2.49 0.15 0.35 0.23 0.84 362 127 42 28 312 194

    LB04C 2.50 97.49 0.15 0.35 0.24 0.98 1509 12.8 377 116 37 22 281 180LB04D 2.55 98.11 0.13 0.32 0.21 0.22 1528 13.4 293 95 29 22 260 151

    LB11 2.59 0.11 0.32 0.19 0.43 208 61 23 22 229 159

    LB12 2.59 0.15 0.45 0.27 0.33 358 107 36 28 280 240

    LB13 2.64 0.18 0.49 0.29 0.27 423 121 34 21 215 292

    LB14 2.53 97.28 0.18 0.47 0.29 0.48 1503 12.0 405 123 33 28 229 293

    LB15 2.54 97.94 0.18 0.47 0.29 0.23 1522 12.0 398 128 38 23 225 276

    CV03 2.71 90.99 0.195 0.63 0.31 0.33 1328 11.6 622 117 37 23 171 266

    CV06 2.70 0.17 1.095 0.29 0.84 1636 134 34 21 284 195

    CV07 2.71 0.20 1.56 0.31 0.29 544 122 34 16 144 210

    CV08 2.81 86.82 0.21 0.73 0.31 0.44 1223 11.5 998 105 30 22 114 262

    (continued on next page)

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    have 15–35% quartz and lithics, with an average of 

    about 20%. Many of the fluvial sediments, and two of 

    the paleosols, have non-calcareous sandy concretionsranging in size from mm-scale (Fig. 4E) to decimeter 

    scale. Typically these are grey-green, fine- to medium-

    grained sand in otherwise red sediments. Grey-green

    color in iron-bearing paleosols is typically associated

    with unoxidized iron. These apparent micro-reducing

    conditions may be attributable to the former presence

    of decaying organic matter, and may have been

    formed in a fashion similar to the drab-haloed root 

    traces.

    Bulk rock geochemical properties of fluvial rocks

    may also be used to identify paleosols and to separate paleosol orders (Sheldon et al., 2002). Net gains and

    losses of different elements may be calculated by

    examining the mobility of the element of interest 

    relative to some assumed immobile element (Chad-

    wick et al., 1990; e.g.,  Driese et al., 2000). Elements

    that are typically considered as immobile during

    weathering include Ti, Zr, Nb, Hf, and under some pH conditions, Al. Ti, Zr, and Nb were considered and

    Ti was selected both because it was immobile relative

    to Zr and Nb and because it is the most abundant of 

    the three elements. The open system mass-transport 

    function for element j in the weathered sample (w)

    is defined as follows (e.g.,   Chadwick et al., 1990):

    s j;w  ¼   qwC  j;w

    =   q pC  j; p

      ei;w þ 1

    1   ð1Þ

    where   qw   is the density of the weathered material,

    C  j,w is the chemical concentration (weight percentage)of element j in the weathered material,   q p   is the

    density of the parent material, and  C  j,p is the chemical

    concentration (weight percentage) of element j in the

     parent material. If  s j,w=0 (i.e., element w was immo-

    Sample Rho

    (g cm3)

    CIA K Clayeynessd (P

     bases/Al)d Salin.d Gleyd MAP MAT Bae Sr Y Nb Zr Rb

    CV09 2.77 96.47 0.21 0.54 0.31 0.36 1479 11.5 449 98 33 24 120 280CV10 2.74 96.84 0.21 0.51 0.30 0.28 1490 11.8 418 94 30 21 153 270

    CV13 2.74 0.20 0.70 0.31 0.38 1081 125 27 25 147 260

    CV16 2.64 0.15 1.37 0.32 0.84 951 92 36 19 237 184

    CV19 2.65 0.17 1.28 0.28 2.97 959 113 42 19 301 196

    CV22 2.76 0.18 6.26 0.32 1.52 537 87 43 10 93 94

    CV24 2.67 0.15 1.56 0.31 1.03 2439 136 33 16 195 163

    CV25 2.58 0.13 2.52 0.29 0.27 2434 142 41 12 306 124

    CV26 2.82 0.20 16.2 0.31 0.22 9654 272 29 nd 31 40

    CV27 2.74 96.68 0.21 0.54 0.33 0.24 1485 11.3 507 158 33 24 125 270

    CV28 2.54 0.18 0.79 0.32 0.36 51,452 1017 22 nd 151 178

    CV29 2.70 96.95 0.20 0.46 0.28 0.24 1493 12.0 3292 262 32 22 159 244

    CV30 2.72 97.79 0.20 0.43 0.27 0.17 1518 12.3 367 179 47 21 173 241

    CV31 2.60 0.13 1.58 0.30 0.31 34,767 688 30 9 269 95CV45 2.69 0.06 5.57 0.34 0.79 275 73 34 20 202 79

    CV46 2.75 0.12 2.08 0.34 0.34 303 107 32 22 390 138

    CV47 2.60 94.67 0.07 0.37 0.21 1.37 1428 13.4 144 78 17 23 133 102

    a  Reactive with dilute HCl. b Total iron as Fe2O3.c Refers to samples at the boundary between two horizons.d Molar ratios: clayeyness= (Al2O3 /SiO2);

    P bases / Al = (CaO + MgO + Na2O + K 2O)/Al2O3; salinization (Na2O + K 2O)/Al2O3; gleiza-

    tion=(FeO/Fe2O3).e All trace element compositions.

    Table 1 (continued )

    Fig. 4. Field and petrographic photos. A) Outcrop photo of the Cala Viola Nord section; paleosols sit on top of the coarser, horizontal benches in

    the section (arrow). B) Outcrop photo showing the complex fluvial character of Verrucano Sardo Formation. C) Profile of a Cala Viola paleosol;

    the light colored vertical streaks are rhizoliths and drab-haloed root traces (arrows). D) Close-up of vertically oriented burrows in a paleosol A

    horizon (arrow). E) mm-scale quartz concretion (sample CV-20). F) Root traces (arrow) deep in the C horizon of a paleosol, penetrating nearly

    to into the A horizon of the underlying paleosol. G) Laterally discontinuous ground water gleying (arrow) features where the water table was

    ephemerally closer to the surface. H) Thin section of a root trace (sample CV-12).

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     bile), then   ei,w   can be solved for separately allowing

    us to bypass volume (as in the classical definition of 

    strain) as follows (e.g.,  Chadwick et al., 1990):

    ei;w  ¼   q pC  j; p

    =   qwC  j;w

    1   ð2Þ

    where   ei,w   is the strain on immobile element i in the

    weathered sample. The parent materials for the profiles

    were overbank mudstones and sandstones as appropri-

    ate, with separate geochemical analyses for each of the

     paleosol profiles (Table 1; lowermost C horizon anal-

    yses).  Fig. 6  shows the losses or gains of Ca and Sr 

    (which occupy the same sites in most minerals) in the

    type Mácchia and Cala Viola paleosols assuming Ti

    was immobile during weathering (calculated following

    Chadwick et al. (1990)). Although both pedotypes have

    lost much of their Ca relative to their parent material,

    the Cala Viola paleosol has clearly been more weath-

    Fig. 5. Chemical degree of weathering. A) Ca and Sr loss in the type Mácchia and Cala Viola paleosols assuming Ti is immobile. A tau value of 

    1 represents 100% loss of Ca relative to the parent material, and a tau value of 0 represents the parent material. Both paleosols lost Ca, withthe Cala Viola type profile showing greater Ca loss, consistent with a greater degree of chemical weathering. Other elements such as Sr show

    more complicated changes, but are still consistent with a greater degree of chemical weat hering in the ty pe Cala Viola profile. B) Additional

    geochemistry (CIA K (Maynard, 1992) and clayeyness (molar ratio of alumina to silica; Retallack, 1997)). of the type Cala Viola profile Thesignificant offset between values low in the profile and high in profile is evidence of intense chemical weathering. The clayeyness index shows a

    b bulge Q  consistent with the field identification of a Bt horizon.

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    ered, a finding consist ent with the field classification of 

    the paleosols (Table 2). Paleosols generally exhibit the

    highest degree of chemical weathering within their Aand B horizons, with a decrease in weathering down

     profile. Fig. 5B shows the chemical index of alteration

    without potash (Maynard, 1992) for the type Cala Viola

     paleosol. This pattern is consistent with pedogenesis

    rather than fluvial sedimentation where one would

     predict a more erratic variation from bed to bed, but 

    where most values would cluster around a   btypical Q 

    value for the whole sedimentary succession.

    4.1. Pedotypes

    Four pedotypes (sensu   Retallack, 1994)   were

    identified and given names in Italian from their 

    field localities or reconstructed similarity to a given

    environment.

    4.1.1. Cala Viola ( bviolet bay Q  )

    The type Cala Viola paleosol crops out in the

    northern Cala Viola section. Cala Viola paleosols are

    comparable to modern Alfisols (Soil Survey   Staff,

    1998) in the USDA soil classification scheme (Table

    2). They are moderately developed (see   Retallack (1988) for definitions of the degree of development),

    with no relict bedding, blocky peds, and subsurface Bt 

    or Bw horizons. Cala Viola profiles are typically A– 

    Bt–C, and represent   a fairly   stable landscape (i.e.,

    infrequently flooded; Table 3).

    4.1.2. Lago di Baratz ( b Baratz’s lake Q  )

    The type Lago di Baratz paleosol crops out in the

    Lago di Baratz section. Lago di Baratz paleosols are

    comparable to modern Entisols (Soil Survey Staff,

    1998) in the USDA soil classification scheme (Table

    2). They are very weakly developed, with some relict 

     bedding and no diagnostic subsurface horizons. Lago

    di Baratz profiles are A–C and represent a frequently

    disturbed landscape (i.e., flooded; Table 3).

    4.1.3. Mácchia ( bunderbrush Q  )

    The type Mácchia paleosol crops out in the Lago di

    Baratz section, and Mácchia paleosols are found in

     both field areas. Mácchia paleosols are comparable to

    modern Inceptisols (Soil Survey Staff, 1998)   in the

    USDA soil classification scheme (Table 2). They are

    weakly developed with little relict bedding or pedstructure. Mácchia profiles are A–(Bw)–C and repre-

    sent a fairly stable landscape (Table 3).

    4.1.4. Mosca Pesca ( b fly fishing  Q  )

    The type Mosca Pesca paleosol outcrops in the

    Lago di Baratz section. Mosca Pesca paleosols are

    comparable to modern Entisols (Soil Survey Staff,

    1998) in the USDA soil classification scheme (Table

    2). They are very weakly developed, preserve relict 

     bedding, lack ped structure, and lack diagnostic sub-

    Fig. 6. Gleization for the type profiles of the Cala Viola and Mácchia pedotypes. Gleization is the molar ratio of ferrous (Fe2+) to ferric

    (Fe3+) iron.

    Table 2

    Cala Viola pedotypes

    Pedotype Diagnosis FAO USDA

    Cala Viola Thick and red with clayey

    subsurface (Bt) on alluvium

    Luvisol Alfisol

    Lago di

    Baratz

    Grey-green silty soil with

    some relict bedding and no

    diagnostic subsurface horizons

    Fluvisol Entisol

    Mácchia Variable thickness red

    sometimes with scattered

    drab haloed root traces and

    no subsurface Bt or Bk 

    Cambisol Inceptisol

    Mosca

    Pesca

    Sandy, relict bedding,

    without horizonation

    Fluvisol Entisol

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    surface horizons. Mosca Pesca profiles are AC–C and

    represent a frequently disturbed landscape (Table 3).

    5. Diagenesis

    Paleosols typically undergo a number of diagenetic

    changes including loss of organic matter, burial red-

    dening due to dehydration of oxyhydroxides (e.g.,

    conversion of goethite [Fe(OH)3] to hematite

    [Fe2O3]), and compaction due to burial beneath an

    overburden (Retallack, 1991b). Paleosols of the Cala

    Viola preserve essentially no organic matter (b1%

     by volume in thin section point counts). Studies of 

    Quaternary (Stevenson, 1969) and older (Retallack,

    2001b) paleosols have shown that buried paleosols

    lose up to an order of magnitude of organic carbon

    soon after burial in well-drained soils, whereas water-

    logged (hydromorphic) or peaty paleosols show sig-

    nificantly less to no loss of organic matter (Stevenson,

    1969). Given their red color and low ferrous to ferric

    ratios (see Fig. 6), much of the iron in these paleosols

    has been oxidized, indicating at least a moderatedegree of aeration post-burial, and oxygen promotes

    the breakdown of organic matter. This likely accounts

    for the dearth of detectable organic matter.

    Sheldon and Retallack (2001)   showed that the

    degree of compactibility varies according to the initial

     physical properties of the soil. Regional stratigraphic

    relationships indicate a burial depth of 2–4 km, so the

     paleosols have been compacted to between 61.2% and

    87.8% of their original thickness depending on burial

    depth and soil order (see   Sheldon and Retallack,

    2001). Given that all of these paleosols are developed

    on alluvium, an estimate based on inorganic flood-

     plain silts and muds (see   Sheldon and Retallack,

    2001) of 78.6–86.4% of the original thickness is a

    good first order generalization for the sedimentary

    succession as a whole.

    6. Paleoclimatic reconstruction

    A number of means have been devised to recon-

    struct paleoclimate from paleosols.   Retallack (1994)

    has suggested that the depth to the Bk horizon can be

    related to mean annual precipitation (see Royer (1999,

    2000)   and   Retallack (2000)   for discussion of this

    approach). Although a couple of the Sardinian paleo-

    sols effervesce slightly when hydrochloric acid is

    applied, there is nothing that would qualify Bk ho-

    rizons (Soil Survey Staff, 1998).   Royer (1999)   sug-

    gested that soil carbonate is absent in regions

    receiving precipitation   N760 mm per year, although

    this value varies with seasonality and local evapo-

    transpiration (Retallack, 2000; Royer, 2000). Thisvalue for the western US may be applicable to the

    Sardinian paleosols given their formation within a

    continental interior montane basin.

    A more quantitative approach is to compare the

     precipitation regimes of modern soils with indices of 

    chemical weathering (Sheldon et al., 2002; Sheldon,

    2003). Climatic transfer functions applied to a set of 

     paleosols spanning the Eocene–Oligocene boundary

     produced results that were consistent with indepen-

    dent estimates of mean annual precipitation and mean

    Table 3

    Paleoenvironmental interpretation

    Pedotype Paleoclimate Former vegetation Paleotopography Parent material Timea 

    Cala Viola Humid (1300–1500 mm/yr)temperate

    Eutrophic forest Negligible, but  well-drained siltstones

    Alluvial sandstones,and mud-stones

    1000–10000 years

    Lago di Baratz Insufficiently developed to

    determine, but probably

    humid

    Stream-side early

    successional woody

    and herbaceous vegetation

     Negligible, but poorly

    drained

    Coarse sandstone 100–5000 years

    Mácchia Humid (1300–1500 mm/yr)

    temperate

    Eutrophic forest Negligible,

     but moderately

    to well-drained

    Alluvial sandstones,

    siltstones, and

    mud-stones

    500–5000 years

    Mosca Pesca Insufficiently developed to

    determine

    Stream-side early

    successional herbaceous

    vegetation

     Negligible Coarse sandstone   b100 years

    a  Estimated semi-quantitatively after   Retallack (1997)  and references therein.

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    annual temperature (Retallack et al., 2000; Sheldon et 

    al., 2002; Sheldon and Retallack, 2004). Although the

     paleosols in this study are much older, bulk rock 

    geochemical data for the Sardinian paleosols canalso be used to reconstruct the paleoenvironmental

    conditions under with they formed, because the pres-

    ence of root traces, rhizoliths, and burrows indicates a

    formerly vegetated landscape for which modern ana-

    logues can be identified. Mean annual precipitation

    can be related to the chemical index of alteration

    without potash as follows (Sheldon et al., 2002):

    MAP in mmð Þ ¼ 221:12e:0197 CIAK ð Þ ð3Þ

    with an   R2= 0.72 where CIA K is 100 times the

    molar rat io of aluminum   to aluminum, calcium, andsodium (Maynard, 1992). Mean annual temperature

    can be related to salinization (Retallack, 1997) where

    MAT   8Cð Þ ¼ 18:5   S ð Þ þ 17:3   ð4Þ

    with a somewhat   low   R2=0.37 (Sheldon et al.,

    2002). As shown in Fig. 7, mean annual precipitation

    increased slightly from 1300 mm/year to about 1500

    mm/year, while mean annual temperature increased

    slightly but held fairly steady at 11–14   8C. That 

    result is consistent with the general lack of soil

    carbonate. Two analyses (CV22 and CV25 on

    Table 1) of Bt horizons are excluded from the anal-

    ysis because of extremely low oxide totals owing to

    high volatile contents (LOI on   Table 1;   26.7 and

    14.2%, respectively).

    At the present time, soils forming under conditions

    of  N1200 mm/year mean annual precipitation and 11– 

    14   8C mean annual temperature are found in Mexico

    on the eastern side of the Gulf of California, in theUnited States on the eastern side of the Appalachians,

    northern India, Greece, and southern Italy (FAO,

    1971–1981). Given the proximity of the Sardinian

     paleosols to the Hercynian chain and their low paleo-

    latitude (10F5 degrees), northern India is probably

    the best modern analogue. Such comparisons are im-

     perfect modern analogues because Permo–Triassic

    CO2   levels far exceeded present levels (Berner and

    Kothavala, 2001; Retallack, 2001c). Nevertheless, it is

    clear that these soils did not form in desert conditions.

    Could they have instead formed in a monsoonal paleoenvironment?

    Modern monsoonal environments are characterized

     by extreme seasonal variation, with a pronounced dry

    season or seasons, and a short, very wet season or 

    seasons. There are two main varieties, namely, wet 

    monsoons as in Southeast Asia, Indonesia, northeast-

    ern Australia, and some of India, and dry monsoons as

    in central Asia, parts of India, northwestern Australia,

    the Arabian peninsula, and the southwestern United

    States, however, there is a spectrum of conditions

     between the main end-members. Soils forming under 

    dry monsoonal conditions are most often Vertisols,

    Aridisols, and rarely, Mollisols (FAO, 1971–1981).

    Soils forming under wet monsoonal conditions are

    most often Ultisols or Vertisols (FAO, 1971–1981).

    Fig. 7. Paleoprecipitation and paleotemperature estimates using transfer functions from regression of climatic data against chemical composition

    of Quaternary soils. The standard error on the precipitation estimate is F182 mm and the standard error on the temperature estimate is F4.4   8C.

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    Only the Cala Viola and Mácchia pedotypes are

    sufficiently developed to use in comparisons with

    modern environments. Both pedotypes developed

    on areas of little or no topographic relief, had similar 

     parent material, and indicate similar paleoclimatic

    conditions (Table 3). The primary differences wer e

    formation time and vegetative covering (Table 3),

    though it could be argued that Cala Viola pedotypes

    represent later stage succession of Mácchia pedo-

    types, however there is not sufficient evidence to

    conclude this robustly.

    A dry monsoon is considered first. In Vertisols,

    large precipitation differences or seasonal soil mois-

    ture deficits between wet and dry seasons change the

     physical volume of smectite clay minerals in soils.

    During the wet season, clays swell with the addi-

    tional water. In the dry season, the clays lose the

    water that they have gained and the parting between

    layers shrinks. These shrink-swell cycles lead to

    deep cracks in the soil. The behavior of the clay

    minerals and colloids also gives rise to mukkara

    structure and gilgai microrelief that readily distin-

    guishes Vertisols (Coulombe et al., 1996; Coulombe,1997; Retallack, 1997; Driese et al., 2000, 2003).

     None of these features (deep vertical to sub-vertical

    cracks, mukkara structure, gilgai microrelief) are

     present in any of the Sardinian paleosols (Table 4).

     Nor do the Sardinian paleosols have pedogenic cal-

    crete and salts of Aridisols, or the abundant crumb

     peds, organic matter, and fine root traces of Molli-

    sols (Table 4).

    Wet monsoons are characterized by Vertisols and

    Ultisols. Ultisols are similar to Alfisols; the primary

    difference is in base saturation. Alfisols are base-rich

    soils that typically have forest vegetation, while Ulti-

    sols are base-poor forest soils. Because of this diffe-

    rence, modern Alfisols and Ultisols are distinguishedon the basis of their base status (e.g., percentage base

    saturation), which is not always recorded (or measur-

    able) in paleosols. A statistically significant method of 

    differentiating Alfisols from Ultisols has been derived

    for paleosols. The B horizons of Alfisols have molar 

    ratio of bases (CaO, Na2O, MgO, K 2O) to alumina

    (Al2O3) greater that 0.5, whereas the B horizons of 

    Ultisols have base /alumina ratios less  than 0.5, typi-

    cally much less (Sheldon et al., 2002).  Fig. 8   shows

    the base/alumina ratios of paleosols in the Cala Viola

    section; most have base/alumina ratios greater than0.5, thereby confirming the field diagnosis of these

     paleosols as Inceptisol-like (Mácchia) and Alfisol-like

    (Cala Viola) rather than Ultisol-like. Only one of Cala

    Viola paleosols plots within the Ultisols field, though

    others are   bnear-Ultic, Q  perha ps indicating some weak 

    monsoonal influence (Fig. 8).

    Retallack (1991a)   studied Miocene monsoonal

     paleosols and soils of Pakistan and found that they

    typically have concretions (rather than nodules) of 

    hematite, calcite, or interlayered calcite and hematite,

    and diffuse carbonate in small nodules throughout the

     profile, including the A horizon. There is essentially

    no carbonate in the Sardinian paleosols and the rare

    Fig. 8. Molar ratio of total bases to alumina for Cala Viola paleosols.

    Only one Cala Viola paleosol (at 24.9 m) plots within the Ultisol

    field, though others are   bnear-Ultic. Q 

    Table 4

    Paleoclimates compared

    Features Desert Wet  

    monsoon

    Dry

    monsoon

    Cala viola

    Salts Yes No No No

    CaCO3 nodules Yes No Yes No

    MAP (1300–1500 mm) No Yes Maybe Yes

    MAT (11–148) No Maybe Maybe Yes

    Soil Types Aridisols Ultisols Vertisols Alfisols

    Vertisols Aridisols Inceptisols

    Mollisols Entisols

    Layered

    Fe(OH)3 –CaCO3

     No Yes Yes No

    Mukkara/gilgai

    gilgai

     No Yes Yes No

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    observed nodules are unlayered, and silica- or iron-

    oxyhydroxide cemented. There are no nodules or 

    concretions consistent with a monsoonal paleoclimate.

    Taken together, these various lines of evidence sug-gest that the Sardinian paleosols were not subject to a

    strongly   monsoonal paleoclimate, either wet or dry

    (Table 4).

    Although the Lago di Baratz and Mosca Pesca

     paleosols of the Lago di Baratz section show little

    significant reddening, the Mácchia and Cala Viola

     paleosols of both the Lago di Baratz and Cala Viola

    sections are both characterized by very red color.

    Intensity of color and degree of clay remobilization

    are two-fold indicators of development, and can be

    supported with chemical and petrographic data. Degreeof drainage also plays a role in soil color and can be

    inferred from the degree of chemical gleization (molar 

    ratio of Fe2+ / Fe3+), soil redoximorphic features (e.g.,

    reduction spots, grey/green paleosols with red mot-

    tles), and trace fossils of organisms requiring oxygen

    (animal burrows and root traces). The red paleosol

    types (Mácchia and Cala  Viola)  are characterized by

    low gleization ratios (e.g.,  Fig. 6) and nearly uniform

    red color, with the exception of rare drab-haloed root 

    traces. Drab-haloed root traces are commonly created

     by micro-reducing conditions, which occur around

    decaying organic matter shortly after burial (Retal-

    lack, 1991b), and as such, would be unrelated to the

     past water table depth. There are no other soil re-

    doximorphic features (iron-manganese nodules, ferric

    nodules) and the deeply penetrating root traces and

     burrows (Fig. 4C–D) indicate good drainage as does

    the degree of chemical weathering and clay illuviation

    into subsurface horizons. The root traces are drab

    from the inside out, as in surface water gley, rather 

    than groundwater gley, yet there is no high density or 

    impermeable layer within the paleosols that would

     perch the water table.The sequence, as a whole, goes from weakly de-

    veloped grey paleosols to more strongly developed

    red paleosols, which is consistent with a dropping

     base level or increased distance from a stream

    (Kraus, 1999), and has no evidence significant paleo-

    topography (Table 3). The Cala Viola Nord section of 

    red paleosols is capped by a thick, areally extensive

    conglomerate with centimeter-sized, well-rounded

    cobbles that may represent a sequence boundary be-

    cause the overlying paleosols in the Cala Viola Sud

    section are again weakly developed (Retallack, 1998;

    Kraus, 1999). This suggests a long-term cyclicity in

    the alluvial delivery system that could be related to

    either tectonics or minor climate change, but not todesertification or monsoonal conditions. The red color 

    of these paleosols appears to be primarily related to

    the hydrological conditions in which they formed.

    7. Conclusions

    Continental red beds should be studied outcrop by

    outcrop as they can form in a variety of settings, rather 

    than generalized to a single genetic model. Red paleo-

    sols form in environments ranging from tropical fo-rests to deserts. Red color, in and of itself, is not 

    diagnostic. Paleoclimatic reconstruction of Late Perm-

    ian paleosols on the basis of the degree of chemical

    weathering and pedological features indicates humid,

    temperate conditions with no evidence of either desert 

    conditions or precipitation seasonality pronounced

    enough to be called a monsoon. The change from

    grey paleosols to red paleosols is attributable to

    changes in hydrological drainage, rather than desert-

    ification or increased seasonality. Low latitude Late

    Permian paleoclimate of Sardinia was warm, tempe-

    rate and perhaps mildly seasonal, but certainly not 

    desertic or strongly monsoonal.

    Acknowledgements

    The author would like to acknowledge financial

    support from a Geological Society of America student 

    research grant to him for this project while he was a

    Ph.D. student. An earlier version of the manuscript 

     benefited from reviews by Steve Driese and Greg

    Retallack, and this version has benefited from twoanonymous reviews and a review by Lee Nordt.

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