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Palaeontologia Electronica http://palaeo-electronica.org

OLIGOCENE TERRESTRIAL STRATA OF NORTHWESTERN ETHIOPIA: A PRELIMINARY REPORT ON PALEOENVIRONMENTS AND PALEONTOLOGY

Bonnie F. Jacobs, Neil Tabor, Mulugeta Feseha, Aaron Pan, John Kappelman, Tab Rasmussen, William Sanders, Michael Wiemann, Jeff Crabaugh, and Juan Leandro Garcia Massini

ABSTRACT

The Paleogene record of Afro-Arabia is represented by few localities, most of which are coastal. Here we report sedimentological and paleontological data from continental strata in northwestern Ethiopia. These have produced abundant and unique assemblages of vertebrates, thus filling a gap in what is known of Paleogene interior Afro-Arabia. The study area is approximately 60 km west of Gondar, Chilga Woreda; covers about 100 km2; and represents as few as 1 Myr based on radiometric dates and paleomagnetic chronostratigraphy. The sedimentary strata are 150 m thick, and dominated by kaolinitic and smectitic mudstones and airfall tuff deposits. Five main types are interpreted as representing Protosols (gleyed or ferric), , , , and Argillisols. Varied, poor conditions produced lateral variation in , and stratigraphic variation probably resulted from lateral changes in drainage conditions through time. Vertebrate fossils occur in associated with ferric Protosols and occur with fruits, seeds, and leaf impressions. Plant fossils also occur as in situ forests on interfluves, leaf and flower compressions associated with in situ carbonized trees in overbank deposits (Gleyed Protosols), and compressions of leaves, twigs and seeds in tuffs. Plant fossil assem blages document diverse forests, from 20-35 m tall, of locally heterogeneous composi tion, and representing families occurring commonly (legumes) or uncommonly (palms) in forests today. Sedimentological and paleobotanical data are consistent with a nearly flat where a meandering river and ample rainfall supported lush . Over time, the region was subject to intermittent ashfalls. A unique fauna of archaic mammalian endemics, such as arsinoitheres and primitive hyracoids, lived here with the earliest deinotheres.

Bonnie F. Jacobs. Environmental Science Program, Southern Methodist University, P.O. Box 750395, Dal las, 75275-0395, USA. [email protected] Neil Tabor. Department of Geological Sciences, Southern Methodist University, P.O. Box 750395, Dallas, Texas 75275-0395, USA. [email protected] Mulugeta Feseha. Institute of Development Research, Department of Geology and Geophysics, Addis Ababa University, P.O. Box 1176, Addis Ababa, Ethiopia. [email protected] Aaron Pan. Department of Geological Sciences, Southern Methodist University, P.O. Box 750395, Dallas, Texas 75275-0395, USA. [email protected]

Jacobs, Bonnie F., Tabor, Neil, Feseha, Mulugeta, Pan, Aaron, Kappelman, John, Rasmussen, Tab, Sanders, William, Wiemann, Michael, Crabaugh, Jeff, and Garcia Massini, Juan Leandro, 2005. Oligocene Terrestrial Strata of Northwestern Ethiopia: A Preliminary Report on Paleoenvironments and Paleontology, Palaeontologia Electronica Vol. 8, Issue 1; 25A:19p, 852KB; http://palaeo-electronica.org/paleo/2005_1/jacobs25/issue1_05.htm JACOBS ET AL.: OLIGOCENE TERRESTRIAL DEPOSITS FROM ETHIOPIA

John Kappelman. Department of Anthropology, University of Texas at Austin, 1 University Station C 3200, Austin, Texas 78712, USA. [email protected] Tab Rasmussen. Department of Anthropology, Washington University, Campus Box 1114, St. Louis, Mis­ souri 63130-4899, USA. [email protected] William Sanders. Museum of Paleontology, University of Michigan, 1109 Geddes Avenue, Ann Arbor, Mich­ igan 48109, USA. [email protected] Michael Wiemann. Center for Wood Anatomy Research, USDA Forest Service, Forest Products Labora­ tory, One Gifford Pinchot Drive, Madison, Wisconsin 53726-2398, USA. [email protected] Jeff Crabaugh. Oklahoma State University, T. Boone Pickens School of Geology, 105 Noble Research Center, Stillwater, Oklahoma 74078-3031, USA. [email protected] Juan Leandro Garcia Massini. Department of Geological Sciences, Southern Methodist University, P.O. Box 750395, Dallas, Texas 75275-0395, USA. [email protected]

KEY WORDS: Ethiopia; paleosols; paleobotany; vertebrate paleontology, Paleogene, Oligocene

PE Article Number: 8.1.25A Copyright: Paleontological Society May 2005 Submission: 8 January 2005. Acceptance: 6 March 2005

INTRODUCTION ably rich in fossil and have produced unique associations of endemic archaic and derived mam­ The Paleogene fossil record is sparse com­ mals. Abundant paleosols document paleoenviron­ pared with the record for continental trop­ ments independently of the fossils. This wealth of ical , despite the much longer duration of the paleontological and palaeoenvironmental data pro­ Paleogene (43 vs. 23 Ma). The abundance of Neo­ vides information that makes Chilga unique for the gene fossil localities is related to development of African Paleogene. the topographically complex East African Rift, which generated accommodation space Geological Background and created ample opportunities for fossilization. The study site is located in an area of approxi­ However, limited exploration for older sites has 2 also contributed to the shortage of Paleogene mately 100 km , 60 km west of Gondar in Chilga localities. Continuing investigations of pre-rift sedi­ Woreda, Amhara Region, northwestern Ethiopia mentary deposits of eastern tropical Africa aim to (Figure 1). Geologically, the area is characterized fill this gap and have produced significant fossil by massive flood basalts as much as 2000 m thick, sites from the of Tanzania and the Oli­ emplaced approximately 30 million ago, prior gocene of Ethiopia (Herendeen and Jacobs 2000; to rifting (Hofmann et al. 1997). Clastic Harrison et al. 2001; Gunnell et al. 2003; Kappel­ and volcaniclastic sediments occur interbedded man et al. 2003; Murray 2003; Jacobs and Her­ with volcanic deposits in a basin formed by faulting endeen 2004; Sanders et al. 2004). These new of the basalts in the middle to late Oligocene. localities provide unique opportunities to document Approximately 150 m of fossiliferous sedimentary Paleogene plant and vertebrate evolution, paleo­ strata are exposed in outcrops across the basin, , and paleoclimate in interior tropical Afro- but the most complete and best-documented sec­ Arabia, when the biota was evolving in isolation tion occurs along the Guang River. In this section, from those of other continents, and experiencing radiometric dates and paleomagnetic reversal stra­ significant global changes. tigraphy constrain the age of about 100 m of sedi­ In this paper we assess the paleoecological ment to between 27 and 28 Ma, the limits of Chron implications of late Oligocene fossils and sedi­ C9n, or earliest late Oligocene (Feseha 2002; Kap­ ments located in Chilga Woreda (henceforth pelman et al. 2003; Cande and Kent 1995; Figure “Chilga”), west of Gondar, on Ethiopia’s northwest­ 2). ern plateau (Figure 1). These deposits are remark­ Plant and vertebrate fossils occur throughout the Chilga deposits. Faunal assemblages, domi­

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Figure 1. Map of Chilga and surrounding area modified from Kappelman et al. (2003). (a) Map of Afro-Arabia with Chilga (C; red), and Paleogene vertebrate and paleobotanical localities marked P (blue) and V (green) respectively. (b) Location of Chilga in Ethiopia. (c) Detailed map of the Chilga area showing the fossil localities, geological section (see Figure 2) and dated rock samples along the Guang and Hauga rivers.

nated by the weathering-resistant teeth of larger of a marked change in lithology or sedimentary fea­ , show little change during the time inter­ tures, whereas profile bases were delineated at the val represented at Chilga. The plant assemblages, highest occurrence of unaltered . some of which occur in direct association with ver­ Field descriptions of paleosols (e.g., thickness, tebrate fossils, provide an excellent record of the color, type, and distribution of mottling; struc­ environment in which the lived and, with ture and mineralogy; size, morphology, and distri­ sedimentological data, provide a fine-scale assess­ bution of authigenic minerals) follow the methods ment of spatial and temporal environmental varia­ of Retallack (1988). Paleosol and lithologic colors tion. Below, we document and integrate were identified in the field with dry samples using sedimentological and paleontological data in order Munsell color charts (Munsell Color 1975). In order to better understand the landscape and climate at to avoid recent weathering, outcrop faces were dug Chilga. back minimally 60 cm to provide a fresh surface for describing and sampling the paleosols. Approxi­ METHODS mately 500 g of paleosol matrix was collected from each paleosol horizon and stored in either canvas Both sediments and plant fossils were sys­ or plastic bags. tematically collected for paleoenvironmental analy­ The mineralogical composition of -size sis. Paleosols were logged and described in the and coarser grains, as well as soil microfabrics, field following previously established methods were determined petrographically from doubly-pol- (Tabor et al. 2002; Tabor and Montañez 2004). ished thin sections following the methods of Moor- Pedogenic horizons within the Chilga strata were house (1959) and Brewer (1976). Powdered bulk recognized using the criteria of Kraus and Aslan samples were analyzed by X-ray diffractometry to (1993). Paleosol tops were identified on the basis determine the mineralogical composition of several

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Figure 2. The Chilga section including the upper sedimentary strata and underlying weathered basalt modified from Kappelman et al. (2003). The Ages to the immediate right of the Geomagnetic Polarity Time Scale panel are in Myr. V, vertebrate localities. VGP, virtual geomagnetic pole. White circles, paleomagnetic samples; black circles, site polarity means. Black bars, normal polarity; white bars, reversed polarity. Arrows refer to minor variations in the paleomagnetic record (Cande and Kent, 1995).

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different paleosol horizons. X-ray diffraction and -size particles were the primary sedi­ analyses were performed on a Rigaku Ultima III X- ments deposited in this basin. Sandstones are rel­ ray diffraction configured with a vertical atively rare and, where present, consist primarily of Theta:Theta wide angle goniometer, using CuKα at very fine-grained reworked airfall tuffs, feldspars, 40Kv and 30mA. Measurements were performed reworked siderite nodules, and and clay with step-scan increments of 0.01° 2θ, counting aggregates similar in appearance to sandstones times of 2s per increment, 0.5/1.0 mm for the pri­ composed of pedogenic mud aggregates that have mary slits and 0.2/0.3 mm for the receiving slits. been described from other basins of various ages Mineralogical composition of the samples was (Gierlowski-Kordesch and Gibling 2002 and refer­ determined following the methods of Moore and ences therein). These observations suggest that Reynolds (1997). allochthonous sand-sized sediment likely entered Plant fossils were collected at 50 localities the basin as airfall deposits. Nevertheless, there is across the basin in the course of surveying, but evidence for reworking and transport of Chilga sed­ systematic excavations at three localities have pro­ iments by and pedogenic alter­ duced the majority of >1100 specimens. One local­ ation on the floodplains. ity, exposed laterally along 60 m of one Stream Channel Deposits. Relatively few stream stratigraphic level at the Guang River section, was channels have been recognized in the Chilga subdivided and excavated at four sublocalities. To strata. The general absence of these features may minimize collecting bias, even fragmentary exca­ reflect, in part, the generally very fine-grained vated plant fossils were collected if there was any nature of the Chilga sediments and our inability to chance of identification. When necessary, fossils discern channel-like structures within rocks with were prepared with a fine-point airscribe. Cuticle these grain-size characteristics. However, trough- was collected from fossil specimens by chipping off cross bedding and inclined heterolithic cross strati­ an approximately 1 cm2 sample, which was then fication, similar to point-bar deposits in meandering prepared using hydrofluoric acid to dislodge inor­ streams (e.g., Walker and Cant 1984), were ganic matrix and a weak solution of bleach or observed within the very fine and fine-grained hydrogen peroxide to oxidize the to sandstone deposits of reworked airfall tuffs, sug­ transparency. Specimens were digitally imaged gesting that alluvial processes were an important using one or all of the following: a high resolution means of sedimentary transport in the Oligocene single lens digital reflex camera, a digital camera sedimentary strata. mounted on a reflected or transmitted light micro­ Overbank Deposits. Overbank deposits in the scope, and a LEO 1450 variable pressure scan­ Chilga region consist primarily of claystones and ning electron microscope. mudstones. Very fine are locally present as Plant fossil specimens were compared with thin tabular beds with sharp, non-scoured bases modern representatives from herbarium and live and are typically structureless, but may exhibit pla­ collections at Missouri Botanical Garden, Royal nar laminations and asymmetrical ripple cross-lam- Botanic Gardens, Kew, or Fairchild Tropical Gar­ inations. Individual sandstone beds range in dens, and in consultation with botanists who spe­ thickness from a few centimeters to ~40 cm. These cialize in the relevant plant groups (see thin sandstone units are interpreted as crevasse Acknowledgments). splay and levee deposits or airfall tuffs. Large vertebrate fossils were located by sur­ Mudstone and claystone beds consist of face prospecting, and all bone and dental frag­ structureless to finely laminated units ranging from ments were collected. Many localities were suitable a few centimeters up to 5 m thick. However, some for excavation, and some of these sites produced claystones and mudstones exhibit ripple cross- associated postcranial remains. Specimens were lamination, and many units contain abundant car­ subsequently prepared with an airscribe as bonaceous material and plant fossils that grade needed. In an effort to locate small vertebrate fos­ upward into organic-rich lignite layers (Figure 3C). sils, fine-grained sediments were screen-washed Most overbank lithologies of the Chilga sedimen­ at several promising localities. However, the tary strata were subject to varying degrees of deposits did not yield small bones or teeth. . Because of their abundance, paleo­ sols are an important component of the overbank RESULTS lithofacies architecture in the Chilga strata. Lithologies Chilga sedimentary strata are primarily com­ posed of claystone and mudstone, indicating that

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Figure 3. A. Tabular and branching lignitic root impression from a Type A paleosol (Protosol). Long axis of hand lens is 5 cm across. B. Laterally extending lignitic root in a medium to coarse angular blocky silty claystone horizon from a Type C paleosol (). Hammer is 40 cm long. C. Organic rich O horizon (black layer) overlying a massive to coarse angular blocky silty claystone in a Type B paleosol (). The thin white layer (8 cm thick) is interpreted to be an altered ashfall layer that briefly halted in situ accumulation of plant material. D. Transition zone between a Type C paleosol (Gleysol) with a thin lignite layer at upper surface (left) changing to Type D paleosol (, right). The dark line denotes mukkara subsurface structure, which forms from periodic shrink-swell of expansible clay minerals during wet-dry cycles. The lignite layer pinches out toward the right side of the diagram. However, approximately 70 meters to left of this photograph, the lignite layer becomes ~50 cm thick and defines the upper surface of a Type B paleosol (Histosol). Jacob staff in upper center of photograph is 150 cm long. See Text for discussion. E. Medium wedge-shape aggregate structure from a Type D paleosol (Vertisol). See text for discussion. F. Medium angular blocky silty claystone with thick, continuous argillans (shiny, reflective surfaces) along ped surfaces within an argillic Bt horizon from a Type E paleosol (Argillisol). See text for discussion.

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Paleosols Protosols (Mack et al. 1993), a category that roughly covers the range of characteristics Based on the field inspection of over 141 observed in the USDA Soil Taxonomy soil subor­ paleosol profiles distributed across the western ders Aquents and Aquepts. Profiles composed of region of Chilga strata, we have recognized five very fine sandstone with Fe-cemented horizons are morphologically distinct paleosol types that repre­ Ferric Protosols (Mack et al. 1993), which corre­ sent the majority of the observed variability (e.g., spond to the USDA soil great group Petraquept horizonation, structure, fabric, color, mineralogy; ( Staff 1998). The presence of protosols Table 1; Figures 3A-F, 4A-F). Below, we present in the Chilga strata indicates that sedimentation generalized descriptions of the characteristics of within the basin (i.e., upon the floodplains and the five paleosol types. We also discuss the mor­ along stream channels) ceased long enough for phological variability within a given paleosol type, colonization by terrestrial flora in poorly drained its stratigraphic and lateral distribution within the environments (Buol et al. 1997). study area, and classify each paleosol type accord­ ing to the Mack et al. (1993) paleosol classification Type B Paleosols. Description: Type B paleosols system to indicate the closest estimated soil taxon have two primary components, a lower mineral within the context of the USDA layer of fine-grained siliciclastic material and an System (Soil Survey Staff 1975, 1998). In order to upper layer composed mainly of organic material avoid genetic terms that relate to the character of (Figure 3C). The mineral layers consist of primarily the paleosol types, we arbitrarily refer to these five drab (5Y 5/1), structureless to very coarse, angu­ paleosol-types as A through E. The paleosol types lar, blocky kaolinitic claystone or mudstone with are vertically and laterally distributed through the mm-scale spherulitic siderite nodules (e.g., Figure Chilga sedimentary strata. Horizon descriptions for 4E). These pedogenically altered horizons grade each paleosol type are listed in Table 1. upward from laminated to thinly bedded sediment. The organic layers are laminated to thinly bedded Type A Paleosols. Description: The only signifi­ lignites that range from 10 mm to 700 mm in thick­ cant pedogenic features in Type A paleosols are ness. The lignite beds are (almost entirely) com­ rooting structures, obliteration of original deposi­ posed of monocot leaf and stem compressions, tional features, and very weak development of soil and parting lineations within these layers com­ structures, such as slickensides and wedge- monly exhibit jarosite and gypsum. shaped aggregate structure with little or no horizo­ Type B paleosols are distributed throughout nation (e.g., Figure 3A). These paleosols occur as the Oligocene strata of the Chilga basin within lam­ claystone-or mudstone-rich profiles and very fine inated to thin-bedded claystones and mudstones of sandstone-rich profiles that range from ~20 to overbank depositional environments. The organic- >150 cm thick. Claystones are generally gray (5Y rich horizons define regional “lenticular structures” 4/1) to olive (5Y 5/2), with few, fine and prominent that can be traced over a few 10's of meters to over orange (7.5YR 5/8) mottles and common, medium 2 km, where they pinch-out and change laterally to to coarse, faint gray (5Y 5/2) mottles. Very fine Type A and Type C paleosols. sandstone-rich Type A paleosols are light yellow Interpretation: Paleosol Type B is a Histosol (5Y 7/3) with massive or single-grain (i.e., sand based on an inferred surficial accumulation of grains) structure that may grade upward into mas­ organic material (Mack et al. 1993; Soil Survey sive, reddish-orange (7.5YR 5/4), Fe-cemented Staff 1998). Modern, laterally discontinuous Histo­ horizons. Rooting structures are typically com­ sols form in low-lying, waterlogged regions charac­ posed of lignitic organic material or fine-grained sil­ terized by anoxic pore waters that promote in situ ica (Figure 3A). Type A paleosols that are accumulation of organic horizons (O horizons). Lat­ composed of very fine sandstone are associated erally discontinuous, organic accumulations in with channel and crevasse-splay sandstones, ash- Type B paleosols are interpreted as O- horizons fall tuffs and fine-grained overbank deposits of the (Soil Survey Staff 1975, 1998) that formed by in floodplain facies. Type A paleosols have highly situ accumulation of plant material. The abundance variable lateral continuity throughout the Chilga of fossil root traces that exhibit shallow and tabular strata; these profiles grade laterally into Type B morphology and base-depleted kaolinitic layers and Type C paleosol profiles. immediately underlying O horizons may corre­ Interpretation: Paleosols with these character­ spond to eluvial A-horizons that formed as a result istics are classified as Protosols, which exhibit of intense hydrolysis or acidolysis due to season­ weak development of pedogenically altered hori­ ally poor drainage (cf. van Breeman and Harmsen zons (Mack et al. 1993). Specifically, profiles com­ 1975). However, the presence of spherulitic sider­ posed of grayish-green claystones are Gleyed ite nodules in horizons below the inferred surface

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Table 1. Characteristics of five major types of paleosols represented in the Chilga strata.

Paleosol Type and Horizon1 Thickness (m)* Nodule and Mineralogy2 Interpreted Interpreted Stratigraphic rhizolith Drainage Class Surface Runoff Occurrrence composition A: Protosol A 0-0.12 Lignitic roots and M, K, I Moderately Well to Very Slow to Slow Throughout Chilga silicified rhizoliths Very Poorly Beds Drained AC, BCss 0.13-0.95 Lignitic roots and M, K, I silicified rhizoliths C 0.07->1.50 - M, K, I B: Histosol Oa, Oe, Oi 0.10 to 0.70 Lignitic roots - Very Poorly Ponded Throughout Chilga Drained Beds Ag, Aj 0.05-0.21 Lignitic roots - Bcg 0.09-0.53 Lignitic Roots and K, M, S, I mm-scale spherulitc siderite Cg 0->1.50 - - C: Gleysol Oa, Oe 0-0.10 Lignitic roots Very Poorly to Ponded to very Throughout Chilga poorly drained slow runoff Beds A 0-0.12 Lignitic roots K, M Bcg1 0.14-0.47 mm-scale K, S, M spherulitic siderite and hematite Bcg2, Bcnss 0-0.72 mm-scale - spherulitic siderite and hematite Cg 0- >1.50 - D: Vertisol AB 0-0.23 Poorly to Seasonally Throughout Chilga somewhat poorly ponded to very Beds drained slow runoff Bss 0.21-1.37 Bgss1 0.23-0.47 M, K Bgnss 0.35-0.59 mm-scale M, K, S spherulitic siderite and hematite C 0->1.50 E: Argillisol A 0-0.08 Moderately well to Very Slow runoff Upper 40 m of somewhat poorly Chilga Beds drained ABt 0.10-0.14 Bt, Btss 0.25-0.37 M, K BC, 0-0.47 Bss C 0->1.50

*The range of thicknesses, in meters, of the various pedogenic horizons represented within paleosols. Note that not all horizons shown may be present in every paleosol (i.e., why some horizons have a range that includes 0 m). 1Horizon names and properties follow the USDA Soil Survey Staff (1975; 1998) guidelines. names: O horizon – surface layer dominated by in situ accumulation of organic material, primarily vegetable matter; A horizon – “” layer, zone of organic matter accumulation and mineral removal (eluvial layer); B horizon – “” layer(s), zone of soil structural development and mineral accumulation (illuvial layer) that is derived from overlying eluvial layers; AB horizon – a near surface horizon exhibiting intermediate properties between an A and B horizon; C horizon – subsoil layer(s) composed of barely weathered material; C-horizons occur beneath A or B horizons. Subordinate indicators of soil properties: a – highly decomposed organic matter, very few to no recognizable plant parts; used only with O horizons; c – presence of concretions or hard nodules; e – partly decomposed organic matter, <1/2 of mass composed of recognizable plant parts; used only with O horizons; g – evidence for strong gleying, or highly reducing and wet soil conditions. Generally Indicated by chromas < 2.; i – slightly decomposed organic matter, >1/2 of mass composed of recognizable plant parts used only with O horizons; j – accumulation of jarosite; ss – presence of slickensides. Numerical descriptors (e.g., Bgc1, Bgc2 denote two horizons with similar morphologies, but at different depths from the paleosol surface. 2 Mineralogical composition of bulk fraction as determined from powder X-ray diffraction. M = Montmorillonite; K = , I = Illite, and S = Siderite.

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Figure 4. Cross-Nichols photomicrographs. A. Void-filling argisepitubule soil microfabric (highly birefringent material in center of micrograph) in a Bt horizon from a Type E paleosol (Argillisol) that formed after an airfall tuff. Field of view is 2 mm across. B. Void-filling argilstriotubule soil microfabric in a mudstone matrix from a Bt horizon in a Type E paleosol (Argillisol). Opaque areas in mudstone matrix are hematite-rich grains. Field of view is 5 mm across. C. Lat­ ticesepic soil microfabric in a Type D paleosol (Vertisol). Field of view is 0.5 mm across. See text for discussion. D. Oosepic soil microfabric in a Type C paleosol (Gleysol). Field of view is 2mm across. See text for discussion. E. Sphaerosiderite concretions in a silty claystone from a Type C paleosol (Gleysol). Field of view is 15µm across. F. Blocky siderite crystals from the mineral horizon of a Type B paleosol (Histosol). Field of view is 0.5 mm across.

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of these paleosol profiles indicates a relatively low matrix in these horizons exhibits striated highly ori­ partial pressure of O2, but high concentration of ented, birefringent clays oriented in a “boxwork” 2- (lattisepic) to continuous, highly oriented, birefrin­ CO3 at depth in these (e.g., Mozley 1993). The shallow, tabular distribution of root traces fur­ gent clays oriented in concentric “spheroids” ther reflects the poorly drained conditions under (Oosepic; Brewer and Sleeman 1976). (Figure 4C, which Type B paleosols formed (cf. Retallack 1988, D), micromophology that is typical of modern, clay- 1990). rich soils characterized by seasonal wetting and drying (Brewer and Sleeman 1988). The upper­ Type C Paleosols. Description: Type C paleosols most horizons generally exhibit coarse prismatic consist of massive to medium to coarse, angular structure with secondary medium angular blocky blocky, gray (5Y 5/3) to yellow-green (5Y 5/2) clay- structure. Smectite clays dominate the mineralogy stones and mudstones with fine to medium red- (Table 1), indicating that these soils were not dish-orange (7.5YR 6/4) mottles. These deeply weathered. These paleosols are broadly pedogenically altered layers grade upward from distributed throughout the stratigraphic succession finely laminated to massive sediment or occur and may be traced laterally in excess of 1 km superimposed upon older paleosols. These paleo­ across the Chilga strata. Type D paleosol profiles sols range from ~450 mm to >2 m thick and contain are observed to change laterally to Type C, Type B, abundant mm-scale spherulitic siderite nodules and Type E paleosols. and finely disseminated micritic siderite cements Interpretation: Type D paleosols are Vertisols, that indurate entire horizons (Figures 3B, 4E, and based on their high clay content (>35%), presence F). In addition, the upper 10 to 100 mm of Type C of slickensides, and v-shaped desiccation cracks, paleosol profiles may consist of organic-rich lignitic which together indicate seasonal soil wetting and horizons. Type C paleosols change laterally into drying (Mack et al. 1993; Soil Survey Staff 1998). Type A, B, and D paleosol profiles. Hematitic redox concentrations and low-chroma Interpretation: Paleosols with these character­ matrix colors throughout much of the profile sup­ istics are interpreted as Gleysols, which exhibit port a more specific paleosol classification as morphological characteristics indicative of forma­ gleyed Vertisols (Mack et al. 1993) or the soil sub­ tion in poorly drained areas near the interface with order Aquerts (Soil Survey Staff 1998). Modern the local or regional table (Mack et al. Vertisols typically form on flat terrain with strongly 1993). Gleysols roughly correspond to the USDA contrasted, wet and dry seasonal or monsoonal cli­ soil great group Aquepts (Soil Survey Staff 1998). mates (Buol et al. 1997). Seasonal wetting and dry­ The drab greenish-gray paleosol matrix colors, red­ ing of expandable 2:1 phyllosilicate minerals (e.g., dish mottling, subsurface accumulation of spheru­ smetctite) leads to shearing of plastic soil materi­ litic siderite nodules, and in situ accumulation of als, slickenside formation and development of Ver­ surficial organic matter collectively indicate that tisol morphology. Vertisols require a period of soil- Type C paleosol profiles developed in areas char­ moisture deficit and sparse vegetation to maintain acterized by high water tables and poor soil drain­ a high concentration of basic cations, thereby pre­ age across the Oligocene floodplains. serving expansible clay minerals in the soil matrix Type D Paleosols. Description: Type D paleosols (Retallack 1990; Duchaufour 1982). We interpret are composed of smectite-rich claystones and silty Type D paleosols to have formed under wet condi­ claystones that grade upward from laminated fine- tions, given the presence of gley colors and redoxi­ grained sediments or partially overprint underlying morphic features, with relatively short periods of paleosols, such as Type C paleosols. Type D soil-moisture deficit. Furthermore, Type D paleo­ paleosols generally exhibit weakly developed slick- sols developed in clay-rich overbank deposits of enplanes and wedge-shaped aggregate structures the Chilga floodplains likely characterized by a that range from 50 to 200 mm across, with second­ short period of soil drying. ary coarse angular blocky structure and abundant Type E Paleosols. Description: Type E paleosols clay pressure faces at depth (Buol et al. 1997). The are comprised of several well- developed mud­ lower horizons also typically contain mm-scale stone and claystone horizons. The uppermost hori­ spherulitic siderite nodules. The upper boundaries zon is dusky-red (7.5YR 3/2) mudstone, underlain of these horizons are distinct and wavy (Figure by several yellowish-gray (5Y 5/2) claystone hori­ 3D), grading upward to greenish-gray (5Y 3/5) hori­ zons that grade upward from thinly laminated to zons with well-defined, wedge-shaped aggregate ripple-cross laminated claystones and mudstones. structure (Fig. 4E), slickenplanes and fine to The lowest of the claystone horizons contains medium, prominent, reddish-orange (7.5YR 5/4) slickensides with wedge-shaped aggregate struc­ mottles. Internally, the microfabric of the paleosol ture and secondary, medium to coarse, angular

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blocky structure with thin, discontinuous clay skins and paleoclimate. The plant fossils occur in a vari­ (argillans; Figure 4A, B; Brewer 1976). Overlying ety of depositional settings, the majority of which horizons contain medium to fine, angular blocky fall into the following five categories: (1) overbank structure with thick, continuous clayskins and fer­ or pond deposits, which preserve autochthonous rans (2.5YR 5/5) upon ped surfaces and in soil organic litter consisting of leaf, flower, insect, and pores (Figure 3E). Mixtures of kaolinite and smec­ twig compressions associated with pollen and in tite dominate the <2µm fraction in the claystone situ carbonized trees (associated with paleosol layers. In addition, abundant root halos (sensu Type A, Protosols; Figure 5A, C); (2) airfall tuffs, Retallack 1990) are present in the upper horizons which preserve leaf and seed compressions and of Type E paleosols. Type E paleosols are found impressions, in many cases associated with in situ only in the upper ~40 meters of the Chilga silicified tree stumps (Figure 5D); (3) tuffaceous sequence, and they change laterally to Type C and ironstones, which preserve fruit and seed casts Type D paleosols. associated with leaf impressions and vertebrate Interpretation: The clay-enriched horizons fossils (associated with paleosol Type A, Protosols; with abundant clayskins upon ped surfaces likely Figure 5E); (4) lignites, which grade from com­ correspond to an argillic horizon (Retallack 1990; pressed containing leaves and stems to low- Soil Survey Staff 1998). In this regard, Type E grade undifferentiated coal (associated with paleo­ paleosols are Argillisols (Mack et al. 1993), which sol Type B, Histosols); and (5) silicified in situ for­ roughly corresponds to the soil orders and ests in a variety of interfluvial depositional settings (Soil Survey Staff 1998). The dominant (Figure 5B). pedogenic process in soils with these characteris­ In the following sections, we summarize what tics is translocation of clay via of Ca2+ is known from the plant fossils found among these from clay-exchange sites in the soil profile (Fran­ five preservational settings, and then integrate our zmeier et al. 1985). Significantly, argillic horizons results with those from geological and vertebrate form only in seasonal , upon well-drained, paleontological research on the same deposits. stable portions of the landscape, indicating that Overbank or Pond Deposits. These organic-rich these Argillisols must have formed upon drier parts deposits are to date the most productive in terms of of the paleolandscape. Mixtures of kaolinite and density of plant fossils and quality of preservation. smectite clays suggest that these soils underwent One of us (A. Pan) is focusing on the study of a sin­ more significant weathering, possibly attributed to gle depositional unit (~ 30 cm thick) from which better drainage and/or duration of pedogenesis, four sublocalities have been collected along a lat­ than all other paleosol types discussed here. How­ eral exposure of approximately 60 m. Macrofossil ever, the presence of gley colors in Type E paleo­ compressions of at least 30 taxa among 533 speci­ sols likely corresponds to sufficiently long periods mens have been documented along this exposure, of soil saturation and anoxic conditions to facilitate and include palm leaflets, petioles, and flowers rep­ leaching of ferric Fe from the profiles. Vertic fea­ resenting the subfamilies Calamoideae, Cory­ tures in these paleosols indicate seasonal wet-dry phoideae, and Arecoideae; leaflets of cf. Sorindeia cycles, suggesting seasonal precipitation in this (Anacardiaceae), Dioscorea (Dioscoreaceae, sec­ region of tropical Africa. tion Lasiophyton), and (legumes); a We interpret Type E paleosols to have devel­ flower of cf. Rubiaceae, leaves provisionally oped upon the more stable and well-drained areas referred to the families Sapotaceae and Malvaceae of the Chilga region. This interpretation is based on s.l.; and one insect wing. Leaf cuticle and morpho­ the fine-grained nature of the strata associated logical features, such as hairs and glands, have with the profiles and pedologic features, such as been instrumental in providing key characters nec­ argillic horizons, that formed upon older, more sta­ essary for identification. The concentration of palm ble portions of the landscape (Soil Survey Staff fossils and presence of at least three of the five 1975; Buol et al. 1997). extant subfamilies together at this site are unusual Paleobotany compared with the limited diversity of palms usually found in living African forests (Moore 1973). On the A field survey of the Chilga basin in 2001 doc­ other hand, the presence of Dioscorea and umented abundant and widespread plant fossil Fabaceae species is more typical of living African localities, which have now produced over 1000 forest communities. leaf, fruit, seed, flower, and wood specimens. Table 2 allows a comparison of preliminary These specimens allow us to fill a large temporal taxonomic lists among the four sublocalities, which gap in the tropical African plant fossil record, and to range from 11 to 37 m apart from one another. address Paleogene plant evolution, , Between 18% and 75% of the taxa recorded (to

11 JACOBS ET AL.: OLIGOCENE TERRESTRIAL DEPOSITS FROM ETHIOPIA

Figure 5. A. leaf compression from Sublocality CH-40 (leaf litter assemblage), B. Silicified tree trunk from in situ fossil forest, C. pollen grain from leaf litter assemblage matrix, D. palm leaf impression in ash IV, E. seed cast from tuf­ faceous ironstone, 62mm diameter.

date) at each sublocality are unique to that sublo­ composition comparable to that of modern forests cality. Furthermore, neighboring sublocalities share of tropical West Africa (Richards 1996). very few, if any, taxa with each other. The limited Plant community physiognomic information is local distribution of taxa in the small sampling area provided by the presence of two charcoalified and documents heterogeneity of composition within the partially compressed tree trunks lying prone at the original plant community (cf. Burnham 1993). As base of the leaf bed (Sublocality 2). Leaf fossils our study has progressed, both diversity and heter­ were found draped over the trunks, but not below ogeneity have increased, and while the numbers them. Thus, a forest gap was created by tree falls, shown in Table 2 may change somewhat with fur­ perhaps associated with a fire, at a time prior to ther work, we consider this variability of local plant leaf-bed deposition, but not long enough before to allow for decay of the fallen trees. Upright, in situ,

12 JACOBS ET AL.: OLIGOCENE TERRESTRIAL DEPOSITS FROM ETHIOPIA

Table 2. Distribution of plant taxa at four sublocalities, arranged here from south to north, along a 60 m lateral expo­ sure of an organic-rich overbank deposit. The number of specimens from each of the sublocalities is shown in the sec­ ond row (total = 533). Key to text coloration is at base of table. SOUTH NORTH Sublocality 4 Sublocality 3 Sublocality 1 Sublocality 2 Total CH-54 CH-41 CH-40 CH-52 Count No. of Specimens 103 103 195 132 533 Taxa Arecaceae cf. Alismataceae Sapotaceae (cf. Mimusops) Eremospatha Hyphaene Anacardiaceae (cf. ?Celtis/Strychnos 3 Legume taxa Unknown 9 Sorindeia) Dioscorea sect. Lasiophyton ?Celtis/Strychnos Unknown 18 Unknown 12 Fabaceae (cf. Bauhinia) Sapotaceae (cf. Mimusops) Unknown 13 Unknown 17 Unknown 10 Unknown 14 Unknown 1 Flower (cf. Rubiaceae) Unknown 15 Unknown 2 Calamoideae (cf. Unknown 16 Unknown 11 Lepidocaryeae group) Arecoideae 4-5 Legume taxa Arecoideae Unknown 3 Unknown 7 Palm flowers Unknown 4 Palm inflorescence Unknown 8 Unknown 5 Palm flower (cf. calamoid) Unknown 6 Minimum # 4 12 14 11 Taxa ­ Estimate Proportion of 0.75 0.58 0.21 0.18 Unique Taxa

Taxon found at 2 or more sublocalities Taxon unique to one sublocality Taxon may or may not be limited to one sublocality

charcoalified tree stumps also occur along this out­ Chilga. These sediments can be recognized every­ crop (Sublocalities 1, 2, and 4), but appear to be where in the basin by their red and black color rooted in the paleosol below the leaf bed. Thus, derived from iron and manganese oxides. Organic leaves and other forest debris fell around the bases plant material (i.e., cuticle) has not been found, but of the in situ trees following a fire (presumably the some leaf impressions show detailed venation and same fire responsible for the tree falls). the fruit and seed casts preserve diagnostic sur­ Airfall Tuffs. Five ash horizons can be traced lat­ face features. Preliminary identifications include erally within the basin (for - 5 km), and the least Arecaceae (palm) fruits, Fabaceae (legume) fruits weathered of these (ash IV) was fossiliferous at all and leaflets, and the seeds of at least three mor­ locations visited. While these deposits show some phologically distinct species of Anonaspermum sedimentary structures associated with transport (Annonaceae). by water, there is evidence of at least periodic Lignite. Macrofossils preserved in the lignites con­ direct airfall consistent with the preservation of del­ sist of robust stems and shoots. These have not icate fern fronds, which indicate rapid burial without yet been studied, but fieldwork in December 2004 transport more than a short distance. One fern documented the rare occurrence of cuticle in some taxon, Acrostichum, is found in ash IV at several lignite deposits. Thus, there is potential for further locations. This genus grows today in edaphic set­ work on plant cuticle from the macrofossils and for tings associated with high salt content or poorly the assessment of these deposits palynologically. drained, swampy conditions (Mabberly 1993). In Situ Silicified Forests. Trunk diameter mea­ Other plants from ash IV include a small pinnatifid surements from 72 trees at two localities (34 and fern, legume fruits and leaflets, fan palm leaves, 38 trees, respectively) provide tree height esti­ broad-leaved dicot impressions, and in situ silici­ mates (Appendix 1) using the regression formulae fied tree trunks including palms. An Ar40/Ar39 age of Rich et al. (1986) and Niklas (1994). The two of 27.36+/-0.11 Ma on ash IV glass shards pro­ sets of estimates are remarkably similar; however, vides precise time control for the plant fossils (Fig­ estimates based on the formula of Rich et al. ure 2; Kappelman et al. 2003). (1986) may be more accurate because the predic­ Tuffaceous Ironstone. Fruit and seed casts are tive formula was derived from dicotyledonous trees abundant in these deposits, which have also pro­ of modern tropical wet forest (Costa Rica), while duced the majority of vertebrate fossils from the formula of Niklas (1994) was derived from a

13 JACOBS ET AL.: OLIGOCENE TERRESTRIAL DEPOSITS FROM ETHIOPIA

combination of woody gymnosperms and hyrax, being well represented. A third species is angiosperm dicots (not exclusively tropical). Both larger in size and is probably related to Pachy sets of estimates indicate that the trees in these hyrax, while a fourth is closely related to Buno forests stood between about 20 and 35 m tall hyrax. Proboscidea are the most diverse order of (Appendix 1). The distribution of trees mapped at mammals and are represented by three families one of these localities, using GPS measurements and five new species. Three of these new probos­ with cm-scale accuracy, documents a density of cideans belong to the family Palaeomastodontidae one tree every 3 m, a minimum considering that (Phiomia major, aff. Palaeomastodon sp. nov. A, and not every tree would have been preserved. Identifi­ aff. Palaeomastodon sp. nov. B), with the Chilga cation of the specimens is in progress, but analysis occurrences representing the youngest known for of thin sections to date indicates forest assem­ this group. Deinotheres are also represented by a blages with richness of - 20 tree species over 6400 new genus and species, Chilgatherium harrisi, and m2. extend back into time the earliest occurrence of this family by 7 Myr. The third family of Probos­ Vertebrate Fossils cidea is the Gomphotheriidae, with the Chilga One of the most interesting and long-standing occurrence of a new species (cf. Gomphotherium sp. observations of Afro-Arabian vertebrate evolution nov.) again representing the oldest known for this concerns the dramatic turnover between the group (Sanders et al. 2004). endemic archaic faunas of the Paleogene and the more modern largely immigrant faunas of the Neo­ DISCUSSION gene (Maglio 1978). Prior to the discovery of the Coexisting fossil plants, vertebrates, and Chilga vertebrates, the general absence of fossil paleosols have seldom been reported from Paleo­ localities dating from between 32-24 Ma offered lit­ gene sites in tropical Africa. At Chilga, the abun­ tle evidence as to the tempo and mode of this con- dance of fossil assemblages, and their association tinental-scale turnover event. Discoveries in the with a range of paleosols, allow us to apply multiple Chilga region have helped to better establish the proxies to reconstruct floral and faunal communi­ circumstances of this turnover and point out new ties all within the context of their paleolandscape. research directions. The most striking characteristics of paleosols Vertebrate localities occur through the entire in the Chilga sedimentary strata are gley colora­ section at Chilga (Figure 2) but are also more con­ tion, or the dominance of low chroma colors (e.g., centrated in tuffaceous ironstones associated with gray or green), and accumulation of organic mate­ Paleosol Type A (Protosols). The remains are usu­ rial (Mack et al. 1993). These features are found ally fragmentary, most commonly represented by within all of the Chilga paleosols, but they are most teeth and jaws, although limb elements are not prominent in paleosol Types A-C. Such soils occur rare, and generally represent medium- to large- most commonly today in areas with a high water sized herbivores. The same depositional and pres­ table, where soil horizons are waterlogged and ervational characteristics of the sediments that undergo anoxic, or aquic conditions for most of the together act to produce such a superb paleobotani­ (Mack et al. 1993; Buol et al. 1997; Soil Sur­ cal record (see above) apparently work to bias the vey Staff 1998). Specifically, the combination of (1) vertebrate record; mammals smaller than about 20 gley colors, (2) diffuse accumulation of organic kg are not represented in our collections and their material, (3) tabular rooting systems, (4) accumula­ absence, along with the absence of , fish, or tion of minerals associated with low redox poten­ other small vertebrates, may be due to diagenetic tial, such as siderite, and (5) lenticular bodies of leaching of bone prior to fossilization (Kappelman organic-matter accumulation at the surface of Type et al. 2003). B and C paleosols, is interpreted to represent the The Chilga vertebrate fauna (Table 3) is com­ poorest soil drainage conditions across the Chilga posed of large paenungulate herbivores that are floodplains, probably corresponding to local pond­ well represented in older Paleogene Afro-Arabian ing of water or very slow surface runoff. In contrast, localities (Sanders et al. 2004). The most distinc­ the presence of redoximorphic features, such as tive form is a new species of Arsinoitherium (Order drab soil matrix colors with red and orange color Embrithopoda), A. giganteum, larger in size than mottling and accumulation of fine hematitic nodules earlier forms, and representing the youngest in some of the Type C and D paleosols, suggests known occurrence for this group. The hyracoids seasonal groundwater-table fluctuation and alter­ are a second group showing moderate diversity at nating periods of reducing and oxidizing conditions. Chilga, with two new species of the common but Furthermore, the wedge-shaped aggregate struc­ conservative genera Pachyhyrax and Megalo

14 JACOBS ET AL.: OLIGOCENE TERRESTRIAL DEPOSITS FROM ETHIOPIA

Table 3. Vertebrate fossils known from Chilga sediments (Kappelman et al. 2003; Sanders et al. 2004). Order Family Subfamily Genus and species Proboscidea Palaeomastodontidae Phiomia major Palaeomastodon sp. nov. A Palaeomastodon sp. nov. B

Deinotheriidae Chilgatheriinae Chilgatherium harrisi

Gomphotheriidae Gomphotherium sp. nov. Embrithpoda Arsinoitheriidae Arsinoitherium giganteum Hyracoidea Saghatheriidae Pachyhyrax sp. nov. Gen. et sp. nov., aff. Pachyhyrax Megalohyrax sp. nov. Bunohyrax sp.

tures and slickenside formation in some of the (the minimum needed to support forest vegetation Type C and all of the Type D paleosols likely indi­ today; e.g., Jacobs 1999). cate periodic wetting and drying of the soil profile, Initial results from collection and study of plant suggesting that these profiles formed upon por­ specimens from the airfall tuffs (e.g., tuff IV) indi­ tions of the landscape that experienced periodic cate that these plants grew in substrates that were fluctuation of the local groundwater table. Finally, very wet, perhaps swampy. The fern genus Acrosti argillic horizons in Type E paleosols require fairly chum, found in ash IV in at least two locations stable, better-drained conditions well above the across the basin, is represented today by three liv­ groundwater table. Thus, we consider most of the ing species. These are pantropical and occur in lateral and stratigraphic variation in the distribution either freshwater or in association with of paleosol profiles to record differences in the mangrove vegetation (Mabberly 1993). Another landscape position of soil-forming processes, with pinnatifid fern occurs in this context at Chilga, respect to the paleo-groundwater table (Figure 6A, associated with the leaves of dicots and legume B). fruits. Elsewhere, the same tuff preserves upright Feseha (2002) summarized the tectonic and tree stumps, including palms, large palmate palm structural details of the basin that captured the fronds, and legume leaves associated with Chilga sedimentary sequence. That summary envi­ pedogenic modification (Type A paleosols), a clear sioned four stages of regional faulting and sedi­ indication of a stratigraphic hiatus within the tuf­ mentation spanning 32-12 Ma. For the Oligocene faceous unit. In addition, tuff IV exhibits trough , the inferred paleosol drainage conditions cross-bedding and sedimentary structures similar across the exposed areas of the basin provide a to those found in point bar deposits today, consis­ meaningful physiographic context for paleoecologi­ tent with deposition of the airfall tuff in meandering cal reconstruction. stream channels. Thus, the airfall tuff bed, which is The composition and physiognomy of plant at least 7 m thick in most places, represents epi­ fossils from Chilga reflect local depositional condi­ sodic ash deposition across a landscape charac­ tions within the context of regional climate. The terized by a range of edaphic settings from plants found in overbank or pond deposits close to swampy to subaerial. a stream (in sediments associated with paleosol The fossil forests at Chilga are a good indica­ Type A) consist of taxa often found in those set­ tion of wet conditions upon interfluvial settings. tings in tropical Africa today. These include palms, This inference is consistent with interpretations particularly calamoid or climbing palms, Sorindeia, based on the plant assemblages known from over- and cf. Alismataceae. However, the entirety of this bank deposits, the presence of waterlogged bog or assemblage, including provisional identifications of deposits preserved as lignites, and the Sterculiaceae, Fabaceae, and Dioscoreaceae, is paleosol data, all of which point to poorly drained indicative of a climate wet enough to support forest conditions in a generally wet climate. vegetation. Thus, a riparian association does not With respect to mammalian assemblages, it is eliminate the necessity for ample rainfall, which interesting to note that despite the somewhat more must have been at least 1100 mm/year on average derived aspect of the individual taxa of the Chilga

15 JACOBS ET AL.: OLIGOCENE TERRESTRIAL DEPOSITS FROM ETHIOPIA

Figure 6. Schematic reconstruction of the Chilga sedimentary basin during Oligocene time. Based on the strati­ graphic and lateral relationships of paleosols and sediments, a proposed facies relationship of the different soils is superimposed upon the paleolandscape. The line A-A’ marks the lower cross section of the soil landscape. Type A paleosols (Protosols) are associated with sediments indicative of environments characterized by frequent sedimenta­ tion, such as stream levees and crevasse splay deposits. Type B paleosols (Histosols) form in local to regional depressions characterized by ponded water or very slow runoff in ever-wet environments, such as swales adjacent to stream levees. Type C paleosols (Gleysols) form in fine-grained sediments characterized by poorly drained and waterlogged environments across the floodplains and interfluves that underwent long periods of anoxia and aquic conditions. However, development of and redoximorphic coloration in the upper horizons of Type C paleosols indicates some periods of better drainage, possibly during periodic fall of the regional groundwater table. Type D paleosols (Vertisols) form in clay-rich sediments characterized by periodic cycles of wetting and drying, possibly related to seasonal fluctuations of the regional . Type E paleosols (Argillisols) formed upon the most stable portions of the landscape, likely in paleogeographic positions most distal from depositional centers (i.e., streams) and topographically well above the position of the groundwater table. See text. fauna, its general composition of arsinoitheres, their overall low species diversities across a long hyracoids, and paleomastodonts largely matches temporal interval. In contrast, the dramatic diversifi­ that of the faunas from older Paleogene localities cation of the Proboscidea in the absence of any found around the continental margins of Afro-Ara- overall changes in faunal composition demon- bia (Kappelman et al. 2003). The occurrence of this strates that other, probably environmental, condi­ fauna in the highlands of Ethiopia suggests that tions were acting to drive their continued evolution. these herbivores enjoyed a very widespread distri- The question as to whether or not the arrival of bution across Afro-Arabia and probably occupied Eurasian immigrants was responsible for driving generalist niches with broad ecological tolerances. the later extinction of the archaic endemics can This observation is especially interesting in light of only be tested by the recovery of new fossil locali­

16 JACOBS ET AL.: OLIGOCENE TERRESTRIAL DEPOSITS FROM ETHIOPIA ties dating closer to the Paleogene-Neogene ACKNOWLEDGMENTS boundary (23 Ma). This paper is dedicated to the memory of W. In summary, we envision an Oligocene land­ Downs, friend and colleague, whose spirit is scape consisting of a generally flat and broad always with us in the field. We thank the Authority floodplain in a humid, tropical climate. Despite lim­ for Research and Conservation of Cultural Heri­ ited relief, landscape position played a primary role tage, the Ministry of Culture and Sports Affairs, in the distribution of plants and in soil development Ethiopia, particularly Ato Jara, for permission to due to variable but poor drainage conditions across conduct our ongoing research in the Blue the basin (Figure 6A, B). Basin, the director and staff of the National We hypothesize that stratigraphic changes in Museum, Addis Ababa, for their assistance with paleosol morphology and plant composition are pri­ collections, and the Gondar ARCCH and Chilga marily a reflection of intrabasinal physiography Ministry of Culture and Sports Affairs for logistical rather than extrabasinal controls, such as regional support. The project was funded by grants from the or global climate change. In addition, episodic ash- National Science Foundation EAR-0001259, the falls were literally superimposed upon these evolu­ National Geographic Society, the Jacob and tionary geomorphic processes and provided a Frances Sanger Mossiker Chair in the Humanities, significant (perhaps primary) source of sedimen­ the University Research Institute of the University tary material. The ash, depending on where it fell, of Texas at Austin, to JK. BFJ, NT, AP, and JGM was reworked to varying degrees, became part of a were supported by National Science Foundation stable land surface upon which vegetation became grant EAR-0240251 to BJ, the Institute for the established, or was incorporated into standing or Study of Earth and Man at SMU, and the Downey flowing water. Family Award for Faculty Excellence to BFJ and Additional, quantitative paleoclimate proxies NT. Museum and field research of WJS was gener­ will provide a basis for evaluating the influence of ously supported by a Scott Turner Award in Earth climate on Chilga fossils and sedimentary charac­ Science from the Department of Geological Sci­ teristics and will allow us to test the hypothesis that ences, University of Michigan, and funding from climate change was not a primary driver of the the Museum of Paleontology, University of Michi­ physical and biotic changes identified in the sedi­ gan. Tillehun Selassie, Misege Birara, Habtewold mentary strata. Fossils and sediments have the Habtemichael, Mesfin Mekonnen and Drs. potential to provide independent estimates of pale­ Ambachew Kebede and Aklilou Asfaw provided otemperature from the stable isotope composition valuable field assistance, and Dr. Melba Crawford of pedogenic minerals and fossil wood anatomical and Ms. Amy Neuenschwander aided with interpre­ characters. Paleotemperature estimates from tation of satellite imagery. We gratefully acknowl­ leaves at tropical sites have been shown to be edge help from Chilga field assistants, Yohannes unreliable (Jacobs 2002), but paleoprecipitation Desta, Yeshiwass Sitotaw, Gebremeskel Ayele, estimates can be derived from fossil leaf assem­ Elias Addissu, and Teshome Yohannes. Finally, but blages and from elemental composition of paleo­ importantly, we thank our neobotanical colleagues, sols. To test for the occurrence of climate change, John Dransfield, William Baker, Paul Wilken, and the accuracy of paleoclimate estimates derived Peter Edwards, Royal Botanic Gardens, Kew. from plant fossils will be evaluated by intrabasinal comparison of estimates from contemporaneous REFERENCES (stratigraphically equivalent) and facies-equivalent localities (Burnham 1994). If the plant fossils prove Brewer, R. 1976. Fabric and Mineral Analysis of Soils. to be reliable climate proxies, then comparisons Krieger, New York, New York. between facies-equivalent assemblages from dif­ Brewer, R. and Sleeman, J.R. 1988. Soil structure and ferent stratigraphic levels can assess the occur­ Fabric. CSIRO Division of Soils, Adelaide. rence of climate changes through the sequence. Buol, S.W., Hole, F.D., McCracken, R.J., and Southard, R.J. 1997. Soil Genesis and Classification. Iowa Further analysis of plant fossil taxonomy will pro­ State University Press, Ames, Iowa. vide greater resolution of temporal and spatial vari­ Burnham, R.J. 1993. "Reconstructing richness in the ability of community composition, yield valuable plant fossil record." Palaios 8: 376-384. biogeographic information, and provide historical Burnham, R. 1994. Paleoecological and floristic hetero­ documentation to complement and test systematic geneity in the plant-fossil record – an analysis based hypotheses generated by molecular phylogenetics. on the Eocene of Washington. USGS Bulletin 2085­ B.

17 JACOBS ET AL.: OLIGOCENE TERRESTRIAL DEPOSITS FROM ETHIOPIA

Cande, S.C. and Kent, D.V. 1995. Revised calibration of B., Ryan, T.J., Seiffert, E.R., Sen, S., Todd, L., Wie­ the geomagnetic polarity timescale for the Late Cre­ mann, M.C., and Winkler, A. 2003. New Oligocene taceous and . Journal of Geophysical mammals from Ethiopia and the pattern and timing of Research, 100:6093-6095. faunal exhcnage between Afro-Arabia and Eurasia. Duchaufour, P. 1982. : Pedogenesis and Clas Nature, 426:549-552. sification. George Allen and Unwin, London. Kraus, M.J. and Aslan, A. 1993. Eocene hydromorphic Feseha, M.Y. 2002. Sequence , petrography, paleosols: Significance for interpreting ancient flood­ and geochronology of the Chilga rift basin sediments, plain processes. Journal of Sedimentary Petrology, northwest Ethiopia. Unpublished Ph.D.Thesis, Uni­ 63:453-463. versity of Texas at Austin, Austin, Texas, USA. Mabberley, D.J. 1993. The Plant-Book. Cambridge Uni­ Franzmeier, F.P., Bryant, R.B., and Steinhardt, G.C. versity Press, Cambridge. 1985. Characteristics of Wisconsinan glacial in Mack, G.H., James, W.C., and Monger, H.C. 1993. Clas­ Indiana and their influence on Argillic horizon devel­ sification of paleosols. Geological Society of America opment. Society of America Journal, Bulletin, 105:129-136. 49:1481-1486. Maglio, V.J. 1978. Patterns of faunal evolution, p. 603­ Gierlowski-Kordesch, E.H. and Gibling, M.R. 2002. 619. In Maglio, V.J. and Cooke, H.B.S. (eds.), Evolu Pedogenic mud aggregates in rift sedimentation. p. tion of African Mammals. Harvard University Press, 195-206. In Renaut, R.W. and Ashley, G.M. (eds.), Cambridge. Sedimentation in Continental Rifts. Society for Sedi­ Moore, D.M. and Reynolds, R.C. 1997. X-ray Diffraction mentary Geology Special Publication 73, Tulsa, Okla­ and the Identification and Analysis of Clay Minerals. homa. Oxford University Press, New York. Gunnell, G.F., Jacobs, B.F., Herendeen, P.S., Head, J.J., Moore, H.E.J. 1973. Palms in the tropical forest ecosys­ Kowalski, E., Msuy, C.P., Mizambwa, F.A., Harrison, tems of Africa and South America, p. 63-88. In Meg­ T., Habersetzer, J., and Storch, G. 2003. Oldest Pla­ gers, B.J., Ayensu, E.S., and Duckworth, W.D. (eds.), cental from Sub-Saharan Africa: Eocene Tropical Forest Ecosystems in Africa and South Microbat from Tanzania–Evidence for Early Evolution America: A Comparative Review. Smithsonian Insti­ of Sophisticated Echolocation. Palaeontologia Elec tution Press, Washington, D.C. tronica, vol. 5, issue 2, art. 3: 10pp., 672KB. Moorehouse, W.W. 1959. The Study of Rocks in Thin http://www-odp.tamu.edu/paleo/2002_2/africa/ Section. Harper and Brothers, New York. issue2_02.htm Mozley, P.S. 1993. Oxygen and isotopic composi­ Harrison, T., Msuya, C.P., Murray, A., Jacobs, B.F., Baez, tion of marine carbonate concretions; an overview. A.M., Ludwig, K.R., and Mundil, R. 2001. Paleonto­ Journal of Sedimentary Petrology, 63:73-83. logical investigations at the Eocene locality of Munsell Color. 1975. Munsell Charts. Munsell Mahenge in north-central Tanzania, East Africa, p. Color, Baltimore, Maryland. 39-74. In Gunnell, G. (ed.), Eocene : Murray, A.M. 2003. A new characiform fish (Teleostei: Unusual Occurrences and Rarely Sampled Habitats. Ostariophysi) from the eocene of Tanzania. Cana Kluwer/Plenum, New York. dian Journal of Earth Science, 40:473-481. Herendeen, P.S. and Jacobs, B.F. 2000. Fossil legumes Niklas, K.J. 1994. Predicting the height of fossil plant from the Middle Eocene (46.0 Ma) Mahenge flora of remains: an allometric approach to an old problem. Singida, Tanzania. American Journal of Botany, American Journal of Botany, 81:1235-1242. 87:1358-1366. Retallack, G.J. 1988. Field recognition of paleosols, p. 1­ Hofmann, C., Courtillot, V., Feraud, G., Rochette, P., Yir­ 20. In Reinhardt J. and Sigleo W.R. (eds.), Paleosols gus, G., Ketefos, E., and Pik, R. 1997. Timing of the and Weathering Through Geologic Time: Principles Ethiopian flood basalt event and implications for and Applications. Geological Society of America Spe­ plume birth and global change. Nature, 389:838-841. cial Paper 216, Boulder, Colorado. Jacobs, B.F. 1999. Estimation of rainfall variables from Retallack, G.J. 1990. Soils of the Past: An Introduction to leaf characters in tropical Africa. Palaeogeography, . Unwin Hyman, Boston, Massachu­ Palaeoclimatology, Palaeoecology, 145:231-250. setts. Jacobs, B.F. 2002. Estimation of low latitude paleocli­ Rich, P.M., Helenurm, K., Kearns, D., Morse, S.R., mates using fossil angiosperm leaves: examples Palmer, M.W., and Short, L. 1986. Height and stem from the Miocene Tugen Hills, Kenya. Paleobiology diameter relationships for dicotyledonous trees and 28: 399-421. arborescent palms of Costa Rican tropical wet forest. Jacobs, B.F. and Herendeen, P.S. 2004. Eocene Dry Cli­ Bulletin of the Torrey Botanical Club, 115:241-246. mate and Woodland Vegetation in Tropical Africa Richards, P.W. 1996. The Tropical Rain Forest. Cam­ reconstructed from fossil Leaves from Northern Tan­ bridge University Press, New York. zania. Palaeogeography, Palaeoclimatology, Palaeo Sanders, W.J., Kappelman, J., and Rasmussen, D.T. ecology, 213:115-123. 2004. New large-bodied mammals from the late Oli­ Kappelman, J., Rasmussen, D.T., Sanders, W.J., gocene site of Chilga, Ethiopia. Acta Palaeontologica Feseha, M., Bown, T.M., Copeland, P., Crabaugh, J., Polonica, 49(3):365-392. Fleagle, J.G., Glantz, M., Gordon, A., Jacobs, B.F., Maga, M., Muldoon, K., Pan, A., Pyne, L., Richmond,

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Soil Survey Staff. 1975. Soil Taxonomy. United States Tabor, N.J., and Montañez, I.P., 2004. Permo-Pennsylva- Department of Handbook, 436, Washing­ nian alluvial paleosols (north-central Texas): High- ton, D.C. resolution proxy records of the evolution of early Soil Survey Staff. 1998. Keys to Soil Taxonomy. United Pangean paleoclimate. Sedimentology, 51: 851-884. States Department of Agriculture Natural Resources van Breeman, N. and Harmsen, K. 1975. Translocation Conservation Service, Washington, D.C. of iron in acid sulfate soils: I, and the Tabor, N.J., Montañez, I.P., and Southard, R.J. 2002. chemistry and mineralogy of iron in a chronose­ Mineralogical and stable isotopic analysis of quence of acid sulfate soils. Soil Science Society of pedogenic proxies in Permo- paleo­ America Journal, 39:1140-1147. sols: Implications for paleoclimate and paleoatmo­ Walker, R.G. and Cant, D.J., 1984. Sandy Fluvial Sys­ spheric circulation. Geochimica et Cosmochimica tems, p.71-90. In Walker, R.G. (ed.) Facies Models. Acta, 66: 3093-3107. Geological Society of Canada Publications, Toronto, Ontario.

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