The Valley of Lakes is approximately a 500-km elongate depression in Central Mongolia, where Eocene to Miocene continental sediments are long known for their outstanding fossil richness. The palaeontological record of this region is an exceptional witness for the evolution of mammalian communities during the Cenozoic global cooling and regional aridification. In order to precisely elucidate the climatic evolution of the region, we studied the mostly siliciclastic sediments with several levels of paleosols for their sedimentology, mineralogy, major and trace element composition and δ13C and δ18O composition. The obtained results show that temperate hydrothermal fluids induced a strong illitization of the fluvial and lacustrine sediments. This finding contradicts the current conceptual view that the fine fraction of the sediments is of aeolian origin. Moreover, the diagenetic growth of illite resulted in a strong overprinting of the sediments and, subsequently, largely disturbed the pristine mineralogical and geochemical composition of the sediments that could have carried any palaeo-climatic information. An exception is the δ13C (and δ18O) isotope values of authigenic carbonate found in calcrete horizons that still record the ambient climatic conditions prevailing during paleosol formation. Our novel δ13C and δ18O record suggests an early Oligocene aridification in Central Asia at ∼31 Ma, whereas the Oligocene glacial maximum shows no increase in aridification. A second, regional-scale aridification occurs at ~25 Ma and corresponds to a late Oligocene marked mammalian turnover in the Valley of Lakes sediments.
The Valley of Lakes is approximately a 500-km elongate depression in Central Mongolia, where Eocene to Miocene continental sediments are long known for their outstanding fossil richness. The palaeontological record of this region is an exceptional witness for the evolution of mammalian communities during the Cenozoic global cooling and regional aridification. In order to precisely elucidate the climatic evolution of the region, we studied the mostly siliciclastic sediments with several levels of paleosols for their sedimentology, mineralogy, major and trace element composition and δ13C and δ18O composition. The obtained results show that temperate hydrothermal fluids induced a strong illitization of the fluvial and lacustrine sediments. This finding contradicts the current conceptual view that the fine fraction of the sediments is of aeolian origin. Moreover, the diagenetic growth of illite resulted in a strong overprinting of the sediments and, subsequently, largely disturbed the pristine mineralogical and geochemical composition of the sediments that could have carried any palaeo-climatic information. An exception is the δ13C (and δ18O) isotope values of authigenic carbonate found in calcrete horizons that still record the ambient climatic conditions prevailing during paleosol formation. Our novel δ13C and δ18O record suggests an early Oligocenearidification in Central Asia at ∼31 Ma, whereas the Oligocene glacial maximum shows no increase in aridification. A second, regional-scale aridification occurs at ~25 Ma and corresponds to a late Oligocene marked mammalian turnover in the Valley of Lakes sediments.
The Cenozoic climate cooling is well recorded in marine sediments; however, its repercussion on the evolution of continental ecosystems on a global and regional scale remains questionable, as appropriate continental sediment records are rather scarce. Central Asia is certainly a key area for investigating the impact of this global cooling event and particularly the Valley of Lakes in Mongolia. This ~500-km-long sedimentary basin comprises an almost continuous succession of Eocene to Miocene continental sediments that are charac-terised by an outstanding Oligo-Miocene fossil record (see Harzhauser et al. 2016; Daxner-Höck et al. 2017 and other contributions of this special issue and references therein for a palaeontological overview). Three prominent flood basalts crop out at distinct levels in the sedimentary succession and represent stratigraphic marker beds (Höck et al. 1999). Absolute dating of these basalt levels (Höck et al. 1999), fine biostratigraphy of small mammals (Daxner-Höck et al. 2010; Daxner-Höck et al. 2017, this issue) and magnetostratigraphy (Sun and Windley 2015) allow good correlation between the different studied sections and a well-established stratigraphy of the Valley of Lakes sediments (see Harzhauser et al. 2017, this issue and Daxner-Höck et al. 2017, this issue for a more detailed discussion on the stratigraphy). In this contribution, we revise the current model proposed for the climatic and mineralogical evolution of the Valley of Lakes sediments based on mineralogical, major and trace elemental and δ13C and δ18O isotope signatures of the sediments.The Eocene-Oligocene Transition (EOT, ~34 Ma) is the first major cooling phase during the long-term transition from Cenozoic greenhouse to icehouse climate (Zachos et al. 2001; Lear et al. 2008). It is well recorded in δ18O profiles established on the basis of deep-sea benthic foraminifers (Zachos et al. 2001; Coxall et al. 2005). In Central Asia, this transitional phase started in the late Eocene and is marked by a sudden acceleration of the aridification (Dupont-Nivet et al. 2007; Xiao et al. 2010; Abels et al. 2011; Bosboom et al. 2014; Li et al. 2016) and by a dramatic faunal turnover, the “Mongolian Remodeling” (Meng and McKenna 1998; Kraatz and Geisler 2010; Harzhauser et al. 2016). The EOT aridification has been assigned to coupled global cooling, stepwise retreat of the proto-Paratethys Sea (Abels et al. 2011; Bosboom et al. 2014; Caves et al. 2015) and intensified uplift of the Tibetan and Mongolian Plateaus (Wang et al. 2012; Caves et al. 2014). The global climate in the Oligocene is characterised by glacial–interglacial cycles responding to astronomical forcing (Wade and Pälike 2004; Retallack et al. 2004; Pälike et al. 2006; Xiao et al. 2010). During this period, the more pronounced cooling phase, which is the Oligocene Glacial Maximum (OGM), occurred around 28–27 Ma and could correspond to a significant uplift phase of the Himalayan–Tibetan region accompanied by an increase in the rate of silicate weathering (Li et al. 2005), coevolution of grasses and grazers (Retallack 2013) and/or by an important volcanic activity at La Garita caldera (Colorado) (Phillips and Matchan 2013). This OGM is followed by the global Late Oligocene Warming, which is terminated by a renewed glacial episode at the Oligocene–Miocene transition (Miller et al. 1991; Paul et al. 2000). Based on sedimentological evidence, this latter cooling event is thought to have corresponded to a second prominent pulse of aridification expressed by the widespread formation of deserts in Central Asia (Guo et al. 2002, 2008; Sun et al. 2010).At present, there is compelling evidence for two major aridification pulses at the Eocene–Oligocene and Oligocene–Miocene transition in Central Asia that could be related to global cooling events. To date, however, the correlation of the numerous climatic variations observed in the Oligocene marine record with the sedimentological and palaeontological data of Mongolia (presented in this issue and by Harzhauser et al. 2016) remains poorly constrained. We present here a novel and comprehensive mineralogical and (isotope) geochemical dataset of the highly fossiliferous Oligo-Miocene sediments from the Valley of Lakes (Mongolia) and critically re-evaluate the palaeo-climatic evolution of this famous study site.
Geological setting and lithostratigraphy
The Valley of Lakes is an elongate, ~500 km long, ESE-WNW striking Cis-Altaidepression, located in Central Mongolia (Fig. 1). This sedimentary basin is situated between the Gobi Altai Mountains in the south and the Khangai Mountains in the north. It is filled with continental sedimentary rocks of Cretaceous to Quaternary age, deposited above the Proterozoic–Paleozoic basement (Höck et al. 1999; Daxner-Höck et al. 2010, 2014). The mostly siliciclastic Eocene to Miocene sediments are exposed along steep cliffs of mostly dry river beds of the Taatsiin Gol Basin and are long known for their extraordinary fossil richness (e.g. Daxner-Höck et al. 1997, 2010, 2014; Höck et al. 1999; Daxner-Höck and Badamgarav 2007; and other contributions of this special issue). The nomenclature, type area, reference profiles and lithological and sedimentological description of the Eocene Tsagaan Ovoo Fm., the Oligocene Hsanda Gol Fm. and the Miocene Loh Fm. are extensively described by Höck et al. (1999) and Daxner-Höck et al. (2017) in this issue. Three groups of basalt horizons are exposed in the sedimentary succession (Fig. 2) and provide the basis for the chronostratigraphic classification of the Oligo-Miocene sediments (Höck et al. 1999). From the bottom to the top of the sequence, the lower Oligocene basalt I group (~30 to 32 Ma), the upper Oligocene basalt II group (~25–29 Ma) and the middle Miocene basalt III (~13 Ma) (Höck et al. 1999; Daxner-Höck et al. 2014).
Fig. 1
Location of the Taatsiin Gol region (rectangle), which is part of the Valley of Lakes in Central Mongolia. Colour ban indicates altitude in metres
Fig. 2
Stratigraphic overview of the investigated sedimentary succession from the Taatsiin Gol region including the δ18O and δ13C isotope profiles of soil carbonate preserved in calcrete horizons. The stratigraphic and biozone classification follows Daxner-Höck et al. 2017 in this issue. SHG is the upper part of the Hsanda Gol section. TAT corresponds to the Tatal Gol section
Location of the Taatsiin Gol region (rectangle), which is part of the Valley of Lakes in Central Mongolia. Colour ban indicates altitude in metresStratigraphic overview of the investigated sedimentary succession from the Taatsiin Gol region including the δ18O and δ13C isotope profiles of soil carbonate preserved in calcrete horizons. The stratigraphic and biozone classification follows Daxner-Höck et al. 2017 in this issue. SHG is the upper part of the Hsanda Gol section. TAT corresponds to the Tatal Gol sectionFor this study five sections, all located in the Taatsiin Gol und Taatssin Tsagaan Nuur regions of the Valley of Lakes, have been chosen, namely the Taatsiin Gol right (TGR-AB) and south (TGR-C), the Hsanda Gol (SHG-D), the Tatal Gol (TAT-E) and the Hotuliin Teeg (HTE). We concentrate our study on the upper Eocene to lower Miocene interval in these sections (~35 to ~21 Ma including basalt I and basalt II), leaving the main Miocene part. This covers the upper part of the Eocene Tsagaan Ovoo Fm., the Oligocene Hsanda Gol Fm. and the lowermost part of the Miocene Loh Fm. A comprehensive stratigraphic profile is shown in Fig. 2 and represents a rather continuous sedimentation even if the gap cannot be excluded. The geographic details, sedimentological characteristics and stratigraphic position of these sections are reported and discussed by Daxner-Höck et al. 2017 and Harzhauser et al. 2017 in this issue.
Petrography and sedimentology
The coarse clastic Tsagaan Ovoo Fm. is about 150 m thick and comprises predominantly white-greyish, massive to cross-bedded sand and gravel bodies, in which greyish-yellow-green to reddish-brown clay and silt layers are intercalated (Fig. 2). The gravel beds, which have been interpreted as debris flow deposits, following the facies classification of Miall (1996) for fluvial sediments, are up to 5 m thick, poorly sorted and mostly without visible sedimentary structures. Finer clastic beds occur towards the top of this sequence and show trough and planar cross-bedding with up to 1 m thickness, besides lamination, ripples, inverse to normal grading, horizontal bedding and channel fills. These sedimentary structures are indicative of gravel- to sand-bed braided river deposits associated with N to S propagating alluvial fans in a tectonically active basin margin (Miall 1990, 1996; Höck et al. 1999). Bioturbation, roots and plant debris point to the local formation of paleosols. Magnetostratigraphic studies reveal a late Eocene age of the Tsagaan Ovoo Fm. (Kraatz and Geisler 2010).The Oligocene Hsanda Gol Fm. is characterised by a high fossil content and comprises poorly sorted, brick-red to reddish-brown clay with grey sandstone in some places (Fig. 2). The massive, mostly horizontally bedded, clayey and silty beds show non-erosive boundaries and frequently contain irregular marly layers, besides cm- to dm-sized nodules of soil material cemented with secondary calcite. These features have been interpreted as calcrete (also called caliche) developed in paleosols under arid to semiarid climate (McPherson 1979; Reineck and Singh 1986). Root-traces, plant debris and burrows occur in these layers. More rarely, sand and granule lenses can be found, which have been attributed to lacrustrine or fluvial reworking processes. In section SHG, a horizon with greyish-coloured sands and gravels forms a notable interval. The depositional environment was interpreted as semiarid, open steppe with ephemeral rivers and playa lakes (Daxner-Höck et al. 2010; Sun and Windley 2015). At nearly 40–41 m and between 94–100 m, the stratigraphic important basalt I and II groups crop out (Fig. 2).The widespread Loh Fm. is up to 150 m thick and is characterised by a complex lithological variability (Fig. 2), comprising alternating poorly sorted, greenish-yellow-red and widely structure-less sandy clays with pebbles and greyish-white to reddish-brown, trough to planar cross-bedded clayey sands and gravels of fluvial origin (Miall 1990, 1996). Channel and scour infillings, fining upward sequences with inverse to normal grading, small ripple marks and overbank fines can be found and have been interpreted as abandoned channel and waning flood deposits of either a shallow, gravel-bed braided river or a perennial flowing sand-bed braided river with ephemeral character (Reineck and Singh 1986; Miall 1996). Sediments of the Loh Fm. are partly interfingering with those from the Hsanda Gol Fm. and are of late Oligocene to early Miocene age. Burrows and plant debris occur within the fossiliferous calcrete horizons. Imbricated gravel beds, cross-bedded sands and flow structures in the basalt group III (not represented in Fig. 2) point to a palaeo-current direction from N to S (Höck et al. 1999).
Paleosol horizons
Paleosol horizons are frequently developed within the Hsanda Gol and Loh fms. (Fig. 2). These paleosols can be easily identified in the field due to their close association with calcrete horizons (see the above petrological description). Calcretes are ubiquitous features of arid to semiarid and subhumid landscapes, where net evaporation typically exceeds net precipitation (Retallack 1994). The formation of calcretes is generally associated with soil-forming (pedogenic) processes or related to a prolonged interaction with meteoric solutions and/or groundwater (Khadikikar et al. 2000). In the Hsanda Gol and Loh fms., they occur in the form of either laminar (continuous) or irregular and patchy (discontinuous) carbonate nodules and crusts of whitish to pinkish colour. Both types of calcrete consist of almost pure crypto- to microcrystalline calcite. Nodules are often mottled, occasionally arranged in honeycomb-like structures and may contain traces of roots, as well as orange-brown (limonitic) Fe-(oxy)hydroxides and greyish-black Mn-oxides. In some sections, the extensive formation of calcrete affected several metres of the underlying sediments (e.g. TGR-C/10, TGR-C/19, TAT/14-16), suggesting a considerable time of paleosol formation. It is generally accepted that the ambient climatic conditions prevailing during the formation of paleosols may be best preserved in the calcrete horizons and, in particular, in the isotopic and major and trace element composition of the authigenic carbonate. We collected sediment samples from each layer which differed from the underlaying layer by colour, composition, structure, fossil content, etc. All calcrete horizons were sampled in order to identify potential (palaeo-) climatic changes throughout the Oligo-Miocene transition recorded in the Valley of Lakes sediments.
Methods
X-ray fluorescence and the chemical index of alteration
The major and minor element composition of rock samples was analysed with a Philips PW2404 wavelength dispersive X-ray fluorescence (XRF) spectrometer. About 0.8 g of finely ground sample was heated to 1050 °C to remove volatiles, such as CO2 and H2O, and then the loss on ignition (LOI) was determined by gravimetric analysis. The residual was fused at 1200 °C using 4 g of LiBO2 as the fluent agent. The tablets produced were run together with a range of USGS standards. The analytical error is ±0.5 wt% for the major elements.Geochemical estimations of weathering intensity and paths were derived from XRF data, assuming that changes in the bulk rock composition reflect distinct alteration features, i.e. hydrolysis and K-metasomatism. For instance, the progressive transformation of feldspar to more stable clay minerals, such as illite and kaolinite, at ambient environmental conditions can be traced by following changes in the ratio of immobile Al2O3 to the more mobile cations K+, Na+ and Ca2+ expressed as oxides. The quantitative measure of chemical weathering is the Chemical Index of Alteration (CIA, Nesbitt and Young 1982), which is defined as: CIA = (Al2O3·(Al2O3 + Na2O + K2O + CaO*)−1)·100. Note that CaO present as carbonate was subtracted from the bulk CaO content (on the basis of TIC values) to obtain CaO* of the silicate fraction. CaO present as phosphate was not considered in the calculation of the CIA values because it increases the CIA by ~2 units if all P2O5 is assigned to apatite.
Carbon and oxygen isotopes
The carbonate present in the calcrete horizons was analysed for their stable δ13C and δ18O isotope composition in order to evaluate potential palaeo-climatic trends recorded in the paleosols. All samples were crushed and analysed as bulk rock. For some delicate samples, carbonate nodules and crusts were separated by hand using a dental drill. Sample powders were reacted with 102% phosphoric acid at 70 °C in a Kiel II automated reaction system, and the evolved CO2 was analysed with a ThermoFinnigan Mass spectrometer MAT Delta at the University of Graz. The δ13C and δ18O values are corrected according to the NBS19 standard and reported in per mill (‰) relative to the Vienna-PeeDee Belemnite (V-PDB) standard. The analytical precision is <0.05‰ for δ13C and <0.1‰ for δ18O, respectively.
X-ray diffraction
X-ray diffraction (XRD) patterns were recorded for quantitative mineral phase analyses using a PANalytical X’Pert PRO diffractometer (Co-Kα radiation) operated at 40 kV and 40 mA and equipped with a Scientific X’Celerator detector, 0.5° antiscattering and divergence slits, spinner stage, primary and secondary soller and automatic sample changer. Representative rock samples were first crushed in a McCrone micronizing mill for 8 min, together with 10% zincite as the internal standard. Subsequently, randomly oriented samples were prepared using the top loading technique. The specimens were examined over the range 4–85 2θ using a step size of 0.008°2θ/s and a count time of 40 s/step. Rietveld-based mineral quantifications were carried out with the PANanalytical X`Pert Highscore Plus software and its implemented pdf-2 database. Assuming the idealised compositions for quartz, albite, orthoclase, illite, hematite and calcite (Baldermann et al. 2013), the accuracy of these results was verified by comparison with mass–balance calculations based on bulk rock XRF data. All mineral phases with an abundance below 1 wt% (chlorite, kaolinite, vermiculite, halite, amphibole and zeolite, if present) were not considered in the quantitative mineral analyses. The deviation between XRD and XRF results was <3 wt%.The clay mineral fraction (<2 μm) was further charac-terised using XRD analysis of oriented preparations performed on a Phillips PW 1830 diffractometer (Cu-Kα radiation, 40 kV and 30 mA) outfitted with automatic slits, a graphite monochromator and a scintillation counter. About 50 mg of the sample was mixed with 5 mL of deionised water, following dispersion for 10 min in an ultrasonic bath. The clay-in-suspension was then sucked through a ceramic tile of about 4 cm2 in order to produce oriented specimens (Baldermann et al. 2014). These clay films were X-rayed from 3 to 30° 2θ with a step size of 0.02° 2θ and a count time of 2 s per step, each at air-dried states and after the solvation of the clay matter with ethylene glycol (EG) and heating of the preparations to 550 °C for 1 h. The percentage of illite layers (%I) in illite–smectite (I-S) mixed layered clay minerals was determined based on EG-solvated patterns with an analytical precision of ±5% (Baldermann et al. 2013).
Scanning electron microscopy
The mineralogy, particle form and particle shape of authigenic versus detrital (clay) minerals were studied by scanning electron microscopy (SEM) using a GEMINI®technology Zeiss Ultra 55 microscope at the FELMI-ZFE (TU Graz). Representative rock chips were therefore prepared on stubs, and the specimens were sputtered with Au/Pd to reduce charging. The SEM is equipped with a high efficiency in-lens secondary electron (SE) detector and an EDAX Si(Li)-detector for energy-dispersive X-ray spectrometry (EDS) analysis and was operated at an accelerating voltage of 5 kV.
Results
In this chapter, special focus is placed on the identification and characterisation of unidirectional alteration and chemical weathering pathways of the sediments (and intercalated basalts). Such processes have to be considered for the interpretation of palaeo-climatic trends that are based on mineralogical and (isotope) chemical signatures of rock samples discussed below.
Bulk and clay mineralogy
The bulk mineralogy of the investigated sedimentary succession is displayed in Fig. 3. Quartz, sheet silicates, calcite, hematite, plagioclase and minor orthoclase are by far the major constituents. Considering the particle size, more than 50% of the population belongs to the clay fraction, whereas less than 1% belongs to the sand fraction or coarser (Höck et al. 1999). In contrast to the mineralogical composition previously reported by Höck et al. (1999), no indication of dolomite, ankerite, anhydrite and pyrite was found in the investigated samples, and more importantly, the proportions of mica and smectite are negligible. Indeed, illite (%I > 95%) with a 1 M polytype structure and, to a minor extent, I-S (%I ~25–30%) with a 1Md polytype structure dominate throughout the entire succession. Such a microstructure suggests an authigenic origin of these clay minerals (Baldermann et al. 2012, 2013) rather than reworking of detrital material from alluvial fan source areas (Tsagaan Ovoo Fm.) and subsequent deposition by dust and/or braided rivers (Hsanda Gol Fm. and Loh Fm.), as proposed by Höck et al. (1999) and Sun and Windley (2015).
Fig. 3
Bulk mineralogy of sediments from the Tsagaan Ovoo Fm., Hsanda Gol Fm. and Loh Fm. (Valley of Lakes, Central Mongolia) based on XRD data. The location and age of the prominent basalt horizons I to II are shown
Bulk mineralogy of sediments from the Tsagaan Ovoo Fm., Hsanda Gol Fm. and Loh Fm. (Valley of Lakes, Central Mongolia) based on XRD data. The location and age of the prominent basalt horizons I to II are shownMore precisely, the Tsagaan Ovoo Fm. consists predominantly of quartz (41–50 wt%) and illite (33–46 wt%), in addition to moderate proportions of plagioclase, orthoclase (feldspar: 7–13 wt%) and hematite (2–10 wt%), with calcite, kaolinite, I-S, chlorite and Ti-oxides being minor constituents (<2 wt%). A similar mineralogical composition is evident for the Hsanda Gol Fm., except for the highly variable calcite content, attributed to calcrete horizons (1–69 wt%), and local restricted occurrences of zeolite, vermiculite and amphibole (each < 1 wt%) found between 32–43 m and 81–93 m adjacent to the weathered horizons of basalt groups I and II. Thus, illite (10–48 wt%), quartz (12–53 wt%), feldspar (3–13 wt%) and hematite ± goethite (1–9 wt%) are the main substituents, besides small admixtures of kaolinite, I-S, chlorite and halite, if present. The predominance of illite (17–45 wt%), quartz (18–46 wt%), calcite (2–59 wt%), feldspar (3–6 wt%) and Fe-(oxy)hydroxides (2–7 wt%) is also valid for the samples from the Loh Fm., which additionally contains minor amounts (<1 wt%) of kaolinite, I-S and chlorite as well as traces of zeolite, vermiculite and amphibole in close vicinity (94–101 m) to a basaltic horizon of group II (Fig. 3).
Petrographic observations
Representative SEM images of rock chips from the Hsanda Gol Fm. collected at 78.5 m (Fig. 4a, b), 59.0 m (Fig. 4c, d) and 33.8 m (Fig. 4e, f) respectively show rock textures typical for immature (arkosic) sandstones that are weakly cemented with quartz and in particular with authigenic pore filling sheet silicates. Most of the quartz grains are diagenetically affected by the syntaxial (over)growth of quartz cement, and original quartz surfaces are not preserved. The clay minerals have either a lath-like morphology, with lath widths of 0.1 to 0.5 μm, <200 nm thickness and lengths ranging up to 20 μm (Fig. 4d, f) or a platy to irregular morphology with an average particle diameter of 2–4 μm and a particle thickness between 0.1 and 0.3 μm (Fig. 4b, d). EDS analyses of these two particle types reveal Si, Al and K as the major constituents, with the platy clays containing less K and Al and more Si and Na than the lath-like clays. In accordance with the mineralogical results, these particle morphologies and chemical compositions correspond either to “hairy” illite or interstratified I-S, respectively (Güven et al. 1980). The association of hairy 1 M illite, 1Md I-S and quartz cement (Fig. 4d, f) is usually restricted to elevated temperatures around 70 to 150 °C and is therefore attributed to the advanced stages of sandstone diagenesis and the related burial diagenetic dissolution of feldspar-rich sediments (Nadeau et al. 1985; Lynch et al. 1997; Haszeldine et al. 2000; Baldermann et al. 2012). However, the shallow burial of the Valley of Lakes sediments (in the range of few hundred metres) is insufficient to create temperatures suitable for illitization (see discussion below).
Fig. 4
SEM-SE images of calcareous and illitized (arkosic) sandstones from the Oligocene Hsanda Gol Fm. collected at 78.5 m (a, b), 59.0 m (c, d) and 33.8 m (e, f). The association of hairy illite, platy I-S and euhedral quartz cement suggests intense alteration of the sediments at elevated temperatures. See text for further explanations. Abbreviations: Qtz detrital quartz, Qtz
authigenic quartz cement, Msc muscovite, Fsp feldspar, Cc calcite, Clay
secondary clay minerals, I hairy illite, I-S interstratified illite-smectite
SEM-SE images of calcareous and illitized (arkosic) sandstones from the Oligocene Hsanda Gol Fm. collected at 78.5 m (a, b), 59.0 m (c, d) and 33.8 m (e, f). The association of hairy illite, platy I-S and euhedral quartz cement suggests intense alteration of the sediments at elevated temperatures. See text for further explanations. Abbreviations: Qtz detrital quartz, Qtz
authigenic quartz cement, Msc muscovite, Fsp feldspar, Cc calcite, Clay
secondary clay minerals, I hairy illite, I-S interstratified illite-smectiteCalcrete occurs mainly as mm- to dm-sized honeycomb-type nodules and continuous hardplan in the Oligo-Miocene sediments, indicating an advanced stage of soil formation (stage III to IV, following the classification scheme of Goudie (1983) and Machette (1985)). The crypto- to microcrystalline nature of the calcite nodules and the absence of calcite spar and secondary dolomite suggest carbonate precipitation in the vadose zone rather than through interaction with groundwater (Quast et al. 2006). This observation is confirmed by both the presence of hematite (instead of goethite) in the carbonate and the comparable low Sr content (90 to 300 ppm) of the calcite, which is largely independent from the calcite content of the bulk rock samples (Fig. 5; Khadikikar et al. 2000). These features suggest that the pristine isotopic composition of the calcite is preserved in calcrete horizons and was virtually not disturbed by the later illitization (see below).
Fig. 5
The Sr (ppm) vs. bulk rock CaCO3 [wt.%] cross plot points to precipitation of the soil carbonate (i.e. calcrete nodules and lenses) from meteoric solution
The Sr (ppm) vs. bulk rock CaCO3 [wt.%] cross plot points to precipitation of the soil carbonate (i.e. calcrete nodules and lenses) from meteoric solution
Major, minor and trace element geochemistry
The element composition of samples from the Tsagaan Ovoo to Loh fms. is highly variable (Table 1) and follows mainly the changes in the ratio of the silicate relative to the carbonate fraction. Accordingly, the Al2O3 + MgO, SiO2 and CaO contents can be directly attributed to abundances of (sheet) silicates, such as illite and minor orthoclase, as well as quartz and calcite, respectively, complying with the petrographic and mineralogical results (Figs. 3 and 4). Na2O, Fe2O3 and TiO2 contents reflect variations in minor amounts of plagioclase, Fe-(oxy)hydroxides and Ti-oxides, i.e. rutile and anatase. MnO and P2O5 occur only in minor amounts.
Table 1
Major, minor and trace element composition of sediments from the Tsagaan Ovoo Fm., Hsanda Gol Fm. and Loh Fm. (Valley of Lakes, Central Mongolia) based on XRF data and percent in major minerals
Sample ID
Position(m)
Feldspat(wt%)
Illite (wt%)
Quartz(wt%)
Hematite(wt%)
Calcite(wt%)
SUM(wt%)
SiO2(wt%)
Al2O3(wt%)
Fe2O3(wt%)
MnO(wt%)
MgO(wt%)
CaO(wt%)
Na2O(wt%)
K2O(wt%)
TiO2(wt%)
P2O5(wt%)
LOI(wt%)
SUM(wt%)
TIC(wt%)
TAT/33b
96.11
9.4
36.2
40.6
5.3
8.6
100.00
55.43
15.61
6.37
0.14
2.61
3.68
1.52
2.89
0.74
0.11
10.90
100.00
TAT/32d
94.71
5.8
15.4
11.7
2.6
64.5
100.00
17.31
4.85
1.91
0.05
1.14
37.58
0.42
0.86
0.23
0.06
35.60
100.00
TAT/32b
93.66
8.2
36.9
40.7
6.1
8.2
100.00
55.38
15.09
6.08
0.11
2.26
5.00
1.25
2.67
0.74
0.12
11.32
100.00
TAT/31
93.07
7.9
37.7
42.4
6.0
6.1
100.00
57.48
15.10
6.01
0.14
2.23
3.95
1.09
2.72
0.75
0.10
10.43
100.00
TAT/30a
92.39
8.4
39.4
43.3
7.1
1.8
100.00
61.71
15.80
6.17
0.12
2.17
0.74
1.06
2.91
0.84
0.05
8.45
100.00
TAT/29b
92.09
8.8
40.3
42.5
7.3
1.1
100.00
60.24
16.19
6.45
0.12
2.38
0.55
1.21
3.18
0.79
0.06
8.83
100.00
TAT/28
91.22
6.7
26.7
25.3
4.1
37.3
100.00
36.79
9.63
3.79
0.08
1.67
22.17
0.75
1.82
0.48
0.20
22.64
100.00
TAT/27b
91.09
8.2
37.8
38.8
6.9
8.3
100.00
56.21
14.78
5.91
0.15
2.18
5.34
1.01
2.80
0.74
0.13
10.76
100.00
TAT/27a
90.76
7.8
15.2
16.8
1.7
58.4
100.00
22.11
5.29
2.04
0.04
1.18
34.40
0.92
0.98
0.28
0.11
32.65
100.00
TAT/26
90.38
8.4
21.6
26.9
2.8
40.3
100.00
35.39
8.63
3.40
0.08
1.39
23.89
1.15
1.62
0.46
0.12
23.87
100.00
TAT/25
90.01
10.0
36.5
44.3
7.0
2.3
100.00
60.64
15.39
6.05
0.11
2.12
1.27
1.35
2.90
0.83
0.06
9.28
100.00
TAT/24a
89.85
7.3
17.9
17.3
2.1
55.5
100.00
24.95
6.54
2.57
0.06
1.48
31.36
1.07
1.28
0.31
0.10
30.29
100.00
TAT/22c
87.94
10.4
37.5
34.5
5.4
12.2
100.00
51.85
13.75
5.48
0.15
2.33
8.05
1.52
2.83
0.67
0.07
13.31
100.00
TAT/22a
86.54
12.9
33.5
38.6
4.7
10.2
100.00
54.10
14.77
5.92
0.16
2.35
4.64
2.57
3.20
0.70
0.07
11.53
100.00
TAT/21a
86.24
11.2
47.9
32.8
7.0
1.1
100.00
58.10
16.51
6.46
0.09
2.35
0.53
1.62
3.86
0.74
0.08
9.68
100.00
TAT/20b
85.94
10.1
38.5
41.9
6.7
2.7
100.00
57.66
16.07
6.76
0.20
2.52
0.77
1.12
2.82
0.77
0.12
11.19
100.00
TAT/19a
84.92
9.5
40.6
42.6
6.3
1.0
100.00
59.13
16.20
6.40
0.15
2.42
0.56
1.54
2.98
0.78
0.06
9.78
100.00
TAT/18a
83.87
8.4
24.0
18.2
3.5
45.9
100.00
30.51
7.92
3.11
0.06
1.72
26.59
1.28
1.51
0.38
0.05
26.87
100.00
TAT/17b
83.24
8.0
24.6
26.4
4.0
37.0
100.00
36.63
9.54
3.76
0.09
2.00
21.23
1.22
1.88
0.46
0.06
23.13
100.00
TAT/16a
82.11
8.7
29.0
37.9
4.2
20.2
100.00
49.82
13.18
5.25
0.13
2.23
10.45
1.19
2.68
0.64
0.06
14.37
100.00
TAT/15c
81.84
10.8
32.7
33.0
4.0
19.6
100.00
46.69
12.37
4.93
0.11
2.28
12.14
1.58
2.55
0.60
0.06
16.70
100.00
TAT/15a
80.67
9.9
35.8
33.8
4.2
16.3
100.00
48.98
13.16
5.22
0.11
2.18
10.55
1.34
2.82
0.63
0.23
14.79
100.00
TAT/14b
80.09
12.5
36.9
34.8
4.4
11.4
100.00
51.23
13.74
5.49
0.13
2.28
7.75
1.90
2.86
0.67
0.09
13.88
100.00
TAT/13
79.24
11.3
35.5
43.7
5.1
4.5
100.00
58.44
15.77
6.28
0.13
2.33
1.54
1.87
3.25
0.76
0.09
9.53
100.00
TAT/12b
78.47
12.2
29.1
33.0
3.9
21.9
100.00
46.09
12.28
4.84
0.08
2.09
12.93
1.74
2.57
0.59
0.07
16.71
100.00
TAT/11
69.86
10.1
23.2
29.2
3.4
34.1
100.00
41.43
10.99
4.32
0.09
1.91
17.41
1.48
2.33
0.54
0.13
19.37
100.00
TAT/10
69.59
12.1
33.8
38.7
4.4
11.0
100.00
52.17
13.88
5.49
0.13
2.30
7.27
1.98
2.93
0.68
0.08
13.09
100.00
TAT/9
69.22
13.1
30.8
31.2
3.8
21.0
100.00
45.55
12.08
4.77
0.11
2.09
12.87
2.23
2.55
0.59
0.22
16.95
100.00
TAT/8b
68.66
12.4
37.7
42.9
4.8
2.3
100.00
59.00
15.38
6.07
0.12
2.66
1.64
2.13
3.40
0.76
0.08
8.77
100.00
TAT/7b
67.99
12.9
36.9
37.8
4.5
7.9
100.00
54.98
14.38
5.71
0.12
2.39
5.20
2.20
3.22
0.71
0.18
10.92
100.00
TAT/6b
67.24
11.5
25.4
30.1
3.5
29.5
100.00
43.75
11.43
4.50
0.09
2.06
14.70
2.15
2.53
0.56
0.30
17.93
100.00
TAT/5
66.77
10.7
40.8
32.9
5.3
10.2
100.00
54.35
14.14
5.61
0.17
2.27
6.22
2.02
3.41
0.70
0.48
10.63
100.00
TAT/4a
66.29
8.2
35.7
31.5
5.8
18.9
100.00
50.18
12.77
5.01
0.09
2.18
10.05
2.10
3.12
0.63
0.13
13.74
100.00
TAT/3b
65.79
10.1
46.6
34.0
4.5
4.9
100.00
59.00
14.92
5.88
0.08
2.47
2.25
2.21
3.76
0.75
0.08
8.59
100.00
TAT/2
65.08
10.6
39.5
30.6
5.4
13.8
100.00
53.66
13.70
5.40
0.07
2.23
7.43
1.67
3.38
0.67
0.13
11.66
100.00
TAT/1b
64.47
9.6
31.5
32.3
4.8
21.8
100.00
47.04
11.88
4.82
0.08
2.23
13.22
1.42
2.64
0.58
0.09
16.00
100.00
HTE/15
110.13
6.2
44.8
40.3
5.7
3.0
100.00
61.21
16.12
6.02
0.07
2.56
1.11
0.51
3.17
0.79
0.25
8.21
100.00
0.2
HTE/14
109.78
5.8
43.8
43.0
5.5
2.0
100.00
61.04
16.02
6.28
0.17
2.63
1.11
0.44
3.12
0.78
0.17
8.25
100.00
0.3
HTE/13b
108.98
5.4
41.2
43.4
6.1
4.0
100.00
61.30
16.19
6.23
0.10
2.93
1.12
0.30
3.07
0.79
0.21
7.76
100.00
0.3
HTE/12
107.65
2.7
17.1
22.0
2.1
56.1
100.00
27.72
6.97
2.69
0.13
1.52
30.34
0.28
1.31
0.34
0.10
28.60
100.00
23.1
HTE/11b
105.78
3.9
17.3
18.2
2.1
58.6
100.00
25.54
6.62
2.58
0.13
1.37
32.18
0.23
1.29
0.32
0.54
29.22
100.00
24.5
HTE/11a
104.98
4.5
25.8
40.5
7.2
22.0
100.00
49.55
11.76
6.99
0.11
2.04
12.43
0.23
2.11
0.60
0.10
14.07
100.00
2.4
HTE/9b
101.38
4.7
22.0
30.9
4.9
37.4
100.00
40.41
10.08
4.56
2.49
1.79
18.17
0.49
1.86
0.53
0.12
19.50
100.00
13.2
HTE/9a
100.97
4.9
36.9
41.9
6.3
9.9
100.00
58.26
14.83
6.11
0.09
2.08
3.70
0.32
2.74
0.78
0.07
11.02
100.00
2.5
HTE/8
100.40
6.0
38.2
46.2
2.6
7.0
100.00
66.63
11.90
3.93
0.07
1.23
3.98
0.76
3.53
0.64
0.15
7.20
100.00
2.8
HTE/7b
100.00
4.0
23.5
24.0
3.4
45.1
100.00
32.36
8.07
2.97
0.29
1.41
26.70
0.34
1.48
0.41
0.08
25.91
100.00
20.8
HTE/7a
98.73
5.0
34.9
45.6
6.6
8.0
100.00
61.68
15.47
6.13
0.06
2.12
3.11
0.35
2.75
0.81
0.06
7.46
100.00
2.0
HTE/6
97.90
6.5
30.8
41.2
5.4
16.2
100.00
54.51
13.07
5.27
0.09
1.76
8.49
0.28
2.37
0.73
0.40
13.04
100.00
5.9
HTE/5a
96.83
5.6
39.4
45.3
6.3
3.4
100.00
61.72
16.07
6.31
0.06
1.83
1.10
0.30
2.78
0.83
0.05
8.94
100.00
0.4
HTE/4b
94.90
6.0
40.2
44.0
7.2
2.6
100.00
60.60
16.28
6.28
0.06
2.06
1.44
0.37
2.89
0.81
0.05
9.16
100.00
0.7
HTE/3a
94.20
4.8
35.7
35.7
4.8
19.0
100.00
50.60
13.40
5.17
0.41
1.74
10.66
0.22
2.38
0.67
0.32
14.44
100.00
7.8
HTE/2b
93.63
8.0
38.5
46.0
4.9
2.6
100.00
63.33
15.44
5.91
0.05
1.57
1.19
0.56
3.10
0.85
0.07
7.93
100.00
0.5
HTE/2a
92.73
5.9
39.5
45.1
6.9
2.5
100.00
63.31
16.14
6.11
0.11
1.76
0.62
0.42
3.38
0.79
0.07
7.31
100.00
0.2
HTE/1d
91.07
6.1
40.2
39.2
4.7
9.9
100.00
61.16
14.32
4.93
0.09
1.74
4.41
0.56
3.35
0.62
0.07
8.77
100.00
3.3
HTE/1c
90.63
5.2
18.3
14.6
1.4
60.5
100.00
22.19
5.32
1.85
0.18
0.96
35.57
0.27
1.23
0.24
0.09
32.10
100.00
28.4
HTE/1b
90.07
4.8
45.0
42.3
6.2
1.7
100.00
64.96
16.27
5.65
0.07
2.04
0.75
0.58
3.80
0.73
0.06
5.09
100.00
0.3
HTE/1a
89.30
3.6
17.3
12.4
2.1
64.6
100.00
18.85
4.38
1.48
0.25
0.96
37.92
0.18
1.14
0.20
0.14
34.50
100.00
30.4
TGR-C/20b
94.61
8.7
36.8
44.4
7.6
2.4
100.00
60.34
15.98
6.73
0.05
2.57
0.79
0.62
2.91
0.78
0.06
9.17
100.00
TGR-C/20a
93.78
7.1
34.5
48.5
7.8
2.0
100.00
62.60
16.55
6.98
0.05
2.66
0.82
0.62
3.01
0.81
0.06
5.83
100.00
TGR-C/19b
93.36
6.8
28.6
35.3
5.3
24.0
100.00
47.00
12.56
5.15
0.18
2.07
14.33
0.59
2.28
0.62
0.20
15.03
100.00
TGR-C/19a
92.49
6.3
26.3
30.9
4.0
32.6
100.00
40.16
10.63
4.32
0.25
1.69
19.39
0.52
1.88
0.52
0.08
20.56
100.00
TGR-C/18
91.84
6.7
27.3
33.7
4.3
28.0
100.00
45.19
11.85
4.79
0.18
1.81
15.07
0.58
2.06
0.60
0.18
17.70
100.00
TGR-C/17a
91.18
5.9
28.3
38.8
6.4
20.6
100.00
50.84
12.92
5.19
0.16
1.76
10.86
0.48
2.16
0.66
0.06
14.91
100.00
TGR-C/16b
90.49
8.2
34.6
47.8
7.3
2.0
100.00
62.08
15.74
6.28
0.07
1.86
1.04
0.64
2.47
0.83
0.04
8.96
100.00
TGR-C/15
89.24
9.1
29.8
47.8
7.3
6.0
100.00
59.27
15.42
6.20
0.08
1.78
2.74
0.51
2.39
0.78
0.04
10.79
100.00
TGR-C/14b trav
88.49
4.4
12.8
15.3
1.7
65.9
100.00
19.90
5.35
2.02
0.09
0.88
36.61
0.04
0.79
0.26
0.13
33.94
100.00
TGR-C/14b
87.96
4.7
13.6
27.9
3.9
49.8
100.00
32.43
8.62
3.40
0.09
1.03
26.75
0.40
1.22
0.43
0.14
25.49
100.00
TGR-C/13d
86.91
5.9
38.8
45.2
7.1
3.0
100.00
60.91
16.99
6.85
0.03
1.59
0.90
0.47
2.66
0.82
0.06
8.73
100.00
TGR-C/13b
85.86
11.3
39.1
41.7
5.1
2.9
100.00
58.44
15.77
6.28
0.13
2.33
1.54
1.87
3.25
0.76
0.09
9.53
100.00
TGR-C/12
84.77
12.2
29.7
30.0
4.9
23.2
100.00
46.09
12.28
4.84
0.08
2.09
12.93
1.74
2.57
0.59
0.07
16.71
100.00
TGR-C/11b
84.69
8.2
36.4
45.5
6.9
3.0
100.00
60.43
16.61
6.49
0.15
1.75
1.47
0.89
2.82
0.79
0.05
8.56
100.00
TGR-C/11a
84.32
12.1
28.2
25.1
4.4
30.2
100.00
41.43
10.99
4.32
0.09
1.91
17.41
1.48
2.33
0.54
0.13
19.37
100.00
TGR-C/10b
84.14
6.3
10.4
13.0
2.4
67.9
100.00
16.79
4.42
1.68
0.07
1.01
38.65
0.53
0.78
0.21
0.07
35.79
100.00
TGR-C/10a
83.24
12.1
35.6
33.7
5.4
13.2
100.00
52.17
13.88
5.49
0.13
2.30
7.27
1.98
2.93
0.68
0.08
13.09
100.00
TGR-C/9
82.66
12.1
32.5
26.5
5.8
23.0
100.00
45.55
12.08
4.77
0.11
2.09
12.87
2.23
2.55
0.59
0.22
16.95
100.00
TGR-C/8b
82.39
11.4
42.7
36.9
6.1
3.0
100.00
59.00
15.38
6.07
0.12
2.66
1.64
2.13
3.40
0.76
0.08
8.77
100.00
TGR-C/8a
81.12
6.1
30.2
34.9
5.1
23.8
100.00
47.32
12.64
5.01
0.04
1.96
13.32
0.75
2.52
0.61
0.05
15.79
100.00
TGR-C/7b
80.01
11.9
39.8
32.2
5.5
10.5
100.00
54.98
14.38
5.71
0.12
2.39
5.20
2.20
3.22
0.71
0.18
10.92
100.00
TGR-C/6
78.97
12.5
32.3
26.1
4.5
24.6
100.00
43.75
11.43
4.50
0.09
2.06
14.70
2.15
2.53
0.56
0.30
17.93
100.00
2.0
TGR-C/5
78.74
10.5
42.8
29.9
5.3
11.4
100.00
54.35
14.14
5.61
0.17
2.27
6.22
2.02
3.41
0.70
0.48
10.63
100.00
1.9
TGR-C/4b
78.57
7.6
29.5
38.3
5.4
19.2
100.00
49.24
13.54
5.44
0.16
1.97
10.75
0.93
2.73
0.65
0.06
14.53
100.00
8.4
TGR-C/4a
77.87
12.2
37.7
30.5
3.8
15.9
100.00
50.18
12.77
5.01
0.09
2.18
10.05
2.10
3.12
0.63
0.13
13.74
100.00
8.7
TGR-C/3A
77.48
6.8
19.1
16.1
2.2
55.9
100.00
24.84
6.80
2.72
0.04
1.19
32.36
0.39
1.40
0.32
0.07
29.88
100.00
25.7
TGR-C/3b
76.80
12.1
44.6
34.0
5.5
3.9
100.00
59.00
14.92
5.88
0.08
2.47
2.25
2.21
3.76
0.75
0.08
8.59
100.00
TGR-C/2
75.47
9.6
40.5
31.6
5.2
13.0
100.00
53.66
13.70
5.40
0.07
2.23
7.43
1.67
3.38
0.67
0.13
11.66
100.00
TGR-C/1
75.13
9.6
30.5
31.3
4.8
23.8
100.00
47.04
11.88
4.82
0.08
2.23
13.22
1.42
2.64
0.58
0.09
16.00
100.00
0.8
SHG-D/30
91.20
5.3
18.9
22.4
2.5
50.8
100.00
29.82
7.89
3.06
0.32
1.35
28.91
0.41
1.38
0.37
0.05
26.46
100.00
3.4
SHG-D/29a
90.82
6.3
31.2
41.0
5.7
15.9
100.00
54.92
14.30
5.59
0.24
2.52
7.30
0.77
2.43
0.65
0.04
11.23
100.00
SHG-D/28b
90.45
7.3
26.2
32.1
4.8
29.6
100.00
46.65
11.81
4.58
0.20
2.03
15.20
0.65
2.05
0.57
0.04
16.21
100.00
SHG-D/27b
90.05
6.9
37.4
46.0
6.3
3.4
100.00
62.41
16.17
6.38
0.19
2.25
1.72
0.72
2.91
0.78
0.07
6.42
100.00
SHG-D/26b
73.05
6.4
22.5
28.0
3.1
40.0
100.00
36.48
9.41
3.67
0.26
1.64
23.48
0.41
1.81
0.46
0.04
22.34
100.00
SHG-D/25
72.32
7.7
29.5
35.4
4.0
23.5
100.00
47.90
12.33
4.89
0.14
1.88
14.25
0.57
2.45
0.60
0.06
14.94
100.00
SHG-D/24
71.98
5.9
36.7
39.1
5.6
12.7
100.00
55.19
14.31
5.66
0.10
2.24
6.98
0.73
2.84
0.69
0.07
11.18
100.00
SHG-D/23j
71.85
5.9
24.5
28.1
4.2
37.3
100.00
39.69
10.29
4.02
0.12
1.72
20.88
0.48
2.08
0.49
0.09
20.15
100.00
SHG-D/23i
71.38
5.3
23.7
24.9
3.9
42.2
100.00
34.99
9.06
3.57
0.16
1.54
24.74
0.41
1.82
0.44
0.06
23.21
100.00
SHG-D/23 h
70.91
6.2
27.0
24.7
4.2
37.9
100.00
38.51
10.04
4.00
0.13
1.66
21.79
0.52
2.04
0.48
0.07
20.77
100.00
SHG-D/23f
69.97
4.9
25.1
33.8
4.0
32.2
100.00
43.24
11.35
4.44
0.14
1.62
18.02
0.55
2.33
0.55
0.08
17.69
100.00
SHG-D/23d
69.03
5.1
18.7
20.4
3.2
52.6
100.00
26.93
7.01
2.73
0.16
1.24
30.68
0.62
1.45
0.34
0.08
28.75
100.00
SHG-D/23b
68.09
5.7
17.5
25.2
2.5
49.1
100.00
31.58
8.00
3.10
0.24
1.36
27.51
0.57
1.62
0.41
0.06
25.56
100.00
SHG-D/23a
67.62
7.6
38.7
42.6
5.1
6.0
100.00
60.24
15.55
6.17
0.12
2.31
3.31
0.93
3.12
0.78
0.07
7.40
100.00
SHG-D/22
67.05
4.7
16.0
14.7
1.5
63.1
100.00
19.21
4.92
1.88
0.09
1.20
37.02
0.34
1.02
0.24
0.11
33.97
100.00
SHG-D/21
66.70
7.3
39.6
44.2
6.0
2.9
100.00
61.22
15.88
6.23
0.08
2.42
1.53
0.89
3.20
0.79
0.06
7.71
100.00
SHG-D/20a
65.83
6.3
26.6
25.3
3.0
38.8
100.00
37.45
9.64
3.77
0.16
1.64
22.24
0.65
2.00
0.48
0.16
21.81
100.00
SHG-D/19
65.42
9.0
34.3
44.5
5.7
6.5
100.00
59.31
15.12
5.94
0.23
2.39
2.88
1.10
3.18
0.76
0.09
9.01
100.00
SHG-D/18
65.11
5.6
23.7
23.1
2.8
44.8
100.00
35.63
9.00
3.50
0.17
1.56
23.97
0.57
1.92
0.45
0.10
23.13
100.00
SHG-D/17
64.93
7.8
39.4
44.8
5.9
2.0
100.00
61.49
15.60
6.14
0.07
2.41
1.59
0.96
3.28
0.79
0.11
7.57
100.00
SHG-D/16b
64.30
8.6
26.7
27.8
3.1
33.7
100.00
41.09
10.23
3.97
0.17
1.67
19.99
0.81
2.20
0.53
0.14
19.22
100.00
SHG-D/15
63.26
9.5
34.5
46.5
5.7
3.8
100.00
62.35
15.26
5.92
0.09
2.30
2.04
1.17
3.20
0.80
0.13
6.76
100.00
SHG-D/14b
62.73
7.4
20.4
31.0
2.9
38.3
100.00
40.18
9.64
3.63
0.16
1.54
20.90
0.79
1.98
0.51
0.12
20.55
100.00
SHG-D/13
61.98
12.7
30.3
48.3
4.1
4.6
100.00
64.05
14.17
5.11
0.07
1.98
1.96
1.55
2.81
0.78
0.16
7.35
100.00
SHG-D/12
60.80
10.5
33.3
50.2
4.3
1.6
100.00
68.81
14.29
4.37
0.07
1.68
1.08
1.78
2.90
0.81
0.09
4.12
100.00
SHG-D/11b
58.45
7.6
36.6
47.0
7.1
1.7
100.00
61.56
16.81
7.27
0.12
2.27
0.83
0.69
3.02
0.79
0.08
6.57
100.00
SHG-D/10
57.28
9.8
37.7
41.6
9.0
1.8
100.00
57.72
16.92
10.23
0.25
2.52
0.74
0.59
3.21
0.77
0.11
6.94
100.00
SHG-D/9d
57.23
9.2
39.4
44.4
6.1
1.0
100.00
61.04
16.46
6.32
1.45
2.39
0.80
0.76
3.18
0.80
0.07
6.75
100.00
SHG-D/9c
56.53
8.6
40.5
43.5
6.3
1.2
100.00
62.72
16.62
6.55
0.07
2.45
0.58
0.81
3.38
0.82
0.06
5.95
100.00
SHG-D/9b
55.83
10.3
39.7
43.6
5.5
0.9
100.00
66.04
15.02
5.70
0.06
2.28
0.48
1.50
3.22
0.79
0.06
4.84
100.00
SHG-D/9a
55.13
9.6
32.5
52.6
3.5
1.8
100.00
69.13
12.69
4.43
0.03
2.08
0.91
1.79
2.55
0.76
0.04
5.61
100.00
SHG-D/8
54.35
6.7
45.9
39.3
6.7
1.4
100.00
60.32
17.68
7.13
0.07
2.89
0.60
0.57
3.69
0.82
0.05
6.19
100.00
SHG-D/7b
54.18
10.0
42.8
39.9
5.7
1.7
100.00
60.39
15.63
6.40
0.07
3.13
0.89
1.22
3.50
0.77
0.07
7.95
100.00
SHG-D/6
51.43
2.8
12.5
13.8
1.9
69.0
100.00
18.42
5.22
2.14
0.08
1.10
37.44
0.22
1.07
0.24
0.59
33.48
100.00
SHG-D/5
50.18
7.7
45.8
37.8
6.9
1.7
100.00
59.38
17.32
7.31
0.09
2.82
0.82
0.83
3.69
0.78
0.07
6.89
100.00
SHG-D/4
49.35
10.2
47.5
35.0
7.1
1.4
101.00
58.70
17.04
7.55
0.10
2.96
0.64
1.00
3.93
0.72
0.08
7.30
100.00
SHG-D/3a
47.55
9.8
40.8
42.4
5.6
1.4
100.00
62.51
16.25
6.63
0.07
2.83
0.32
1.20
3.77
0.77
0.11
5.54
100.00
SHG-D/2
46.68
7.7
33.6
27.6
4.3
26.8
100.00
46.29
12.51
5.46
0.27
2.21
13.83
0.81
3.02
0.56
0.24
14.82
100.00
SHG-D/1
45.76
12.0
41.3
40.0
5.7
1.1
100.00
61.65
15.30
6.00
0.07
3.29
0.57
2.08
3.45
0.74
0.27
6.57
100.00
TGR-AB/35
40.46
11.9
37.5
40.4
5.6
4.6
100.00
61.62
13.44
6.70
0.02
2.82
1.89
1.46
3.01
0.62
0.48
7.94
100.00
0.2
TGR-AB/34b
39.83
9.4
39.4
44.1
5.7
1.3
100.00
64.28
15.37
6.10
0.08
3.59
0.72
1.04
3.65
0.77
0.07
4.35
100.00
0.3
TGR-AB/33b
38.36
8.4
29.0
31.6
4.5
26.5
100.00
45.52
11.53
4.54
0.09
2.39
16.32
0.78
2.69
0.57
0.10
15.47
100.00
12.6
TGR-AB/32 l
37.63
6.7
34.0
33.5
4.6
21.1
100.00
52.43
13.46
5.32
0.10
2.67
10.17
0.95
3.24
0.66
0.21
10.79
100.00
7.9
TGR-AB/32j
35.70
9.7
38.0
31.5
4.5
16.2
100.00
52.43
13.46
5.32
0.10
2.67
10.17
0.95
3.24
0.66
0.21
10.79
100.00
4.6
TGR-AB/32i
34.73
9.4
36.2
36.1
5.3
12.9
100.00
56.72
14.11
5.57
0.11
2.45
6.62
1.03
3.35
0.70
0.13
9.22
100.00
5.6
TGR-AB/32 h
33.76
8.2
32.7
31.6
4.4
23.2
100.00
48.82
12.31
4.80
0.07
2.57
13.16
0.76
2.94
0.57
0.12
13.90
100.00
10.1
TGR-AB/32f
31.83
7.5
34.2
34.5
4.0
19.8
100.00
49.45
12.49
4.86
0.16
2.56
12.18
0.90
2.89
0.58
0.11
13.83
100.00
9.3
TGR-AB/32d
29.90
9.4
38.2
29.4
4.5
18.5
100.00
49.90
12.60
4.70
0.38
2.35
11.28
1.40
3.17
0.59
0.21
13.43
100.00
8.5
TGR-AB/32a
27.00
8.7
38.0
35.9
4.0
13.5
100.00
55.27
13.95
5.19
0.19
2.27
8.07
0.94
3.24
0.68
0.15
10.04
100.00
5.9
TGR-AB/31
25.30
10.9
33.9
46.7
6.8
1.7
100.00
64.72
14.85
7.02
0.12
2.00
1.00
1.58
3.14
0.81
0.11
4.65
100.00
0.2
TGR-AB/13
8.15
8.7
45.6
40.7
3.4
1.6
100.00
66.35
16.54
4.70
0.05
1.33
0.92
1.31
3.39
0.78
0.06
4.57
100.00
0.2
TGR-AB/12
7.98
9.8
37.0
41.8
9.5
2.0
100.00
56.70
16.49
10.57
1.84
1.67
0.88
0.83
2.87
0.81
0.14
7.19
100.00
0.3
TGR-AB/11a
6.82
7.1
39.4
50.3
2.4
0.8
100.00
70.75
13.67
3.77
0.04
1.41
0.47
1.54
3.65
0.52
0.04
4.15
100.00
0.2
TGR-AB/9
3.46
13.2
33.2
43.2
9.8
0.6
100.00
59.27
16.80
10.96
0.05
1.19
0.31
1.65
3.04
0.74
0.16
5.82
100.00
0.2
Sample ID
Position
Ba
Ce
Co
Cr
Cu
Ga
Hf
La
Nb
Ni
Pb
Rb
Sc
Sr
Th
U
V
Y
Zn
Zr
Th/Sc
Zr/Sc
(m)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
(ppm)
TAT/33b
96.11
362
63
<20
79
40
18
<15
30
<20
45
31
129
20
171
15
<20
110
28
92
155
0.8
7.7
TAT/32d
94.71
151
20
<20
36
11
<10
<15
82
<20
<20
<20
38
30
246
14
<20
39
18
28
63
0.5
2.1
TAT/32b
93.66
399
63
<20
67
41
19
<15
62
<20
39
24
129
20
167
13
<20
124
31
95
164
0.7
8.2
TAT/31
93.07
395
88
<20
72
35
21
<15
47
23
46
31
130
20
150
12
<20
102
40
100
171
0.6
8.6
TAT/30a
92.39
424
71
<20
73
41
20
<15
31
<20
35
27
137
20
329
11
<20
100
22
110
186
0.6
9.3
TAT/29b
92.09
421
83
<20
70
44
21
<15
36
<20
44
30
137
20
216
10
<20
115
23
105
176
0.5
8.8
TAT/28
91.22
263
49
<20
44
25
12
<15
30
<20
20
21
81
23
218
9
20
83
20
63
114
0.4
5.1
TAT/27b
91.09
408
91
<20
63
38
20
<15
34
<20
43
31
126
20
174
8
<20
118
25
97
171
0.4
8.5
TAT/27a
90.76
163
30
<20
42
<20
<10
<15
94
<20
<20
<20
45
20
258
7
<20
42
15
40
101
0.4
5.2
TAT/26
90.38
204
50
<20
49
27
10
<15
30
<20
15
<20
73
28
216
6
<20
58
18
58
112
0.2
4.0
TAT/25
90.01
441
90
<20
76
38
20
<15
51
<20
33
<20
132
20
161
5
<20
101
25
101
196
0.3
9.8
TAT/24a
89.85
198
39
<20
43
<20
<10
<15
99
<20
21
<20
55
20
245
4
<20
52
15
44
86
0.2
4.3
TAT/22c
87.94
394
69
22
62
34
18
<15
37
<20
40
30
117
20
208
3
<20
104
24
87
149
0.2
7.5
TAT/22a
86.54
442
50
<20
64
39
20
<15
38
<20
43
30
127
20
149
2
<20
114
21
96
165
0.1
8.3
TAT/21a
86.24
740
76
<20
72
44
20
<15
62
<20
41
31
144
20
203
1
<20
96
25
102
170
0.1
8.5
TAT/20b
85.94
433
81
23
74
34
22
<15
74
<20
37
34
135
20
166
1
<20
131
23
99
177
0.1
8.8
TAT/19a
84.92
450
100
20
69
37
24
<15
53
<20
44
26
138
20
167
1
<20
120
25
92
183
0.1
9.2
TAT/18a
83.87
263
20
<20
52
22
10
<15
82
<20
22
<20
65
22
290
2
<20
67
30
48
119
0.1
5.5
TAT/17b
83.24
287
63
<20
45
27
10
<15
30
<20
24
21
82
21
241
3
<20
64
18
60
113
0.1
5.4
TAT/16a
82.11
400
62
<20
63
38
16
<15
30
<20
40
31
113
20
202
4
<20
97
25
81
149
0.2
7.3
TAT/15c
81.84
358
58
<20
61
32
17
<15
30
<20
33
23
106
20
203
5
<20
87
24
81
124
0.3
6.2
TAT/15a
80.67
364
78
<20
65
32
18
<15
30
<20
32
26
112
20
216
6
<20
91
35
86
152
0.3
7.6
TAT/14b
80.09
367
60
20
96
40
19
<15
63
<20
50
22
115
20
157
7
<20
98
25
84
148
0.4
7.4
TAT/13
79.24
479
88
<20
68
41
22
<15
68
<20
44
31
133
20
149
8
<20
109
25
98
161
0.4
8.0
TAT/12b
78.47
341
52
<20
53
33
16
<15
41
<20
29
20
103
20
188
9
<20
94
26
75
142
0.5
7.1
TAT/11
69.86
282
56
<20
51
29
12
<15
30
<20
29
<20
91
20
197
10
<20
92
21
70
136
0.5
6.8
TAT/10
69.59
424
93
<20
63
38
19
<15
30
<20
35
32
117
20
177
11
<20
104
24
87
172
0.6
8.6
TAT/9
69.22
356
76
<20
48
37
16
<15
30
<20
27
25
101
20
227
12
<20
99
23
78
133
0.6
6.6
TAT/8b
68.66
411
74
<20
67
44
20
<15
35
<20
39
25
135
20
193
13
<20
116
21
95
170
0.7
8.5
TAT/7b
67.99
380
64
<20
70
41
19
<15
44
<20
40
26
129
20
136
14
<20
119
26
92
160
0.7
8.0
TAT/6b
67.24
291
70
<20
53
35
14
<15
30
<20
28
23
98
20
235
15
<20
95
29
75
134
0.8
6.7
TAT/5
66.77
1119
69
<20
59
46
18
<15
54
<20
49
30
126
20
235
16
<20
115
31
98
157
0.8
7.9
TAT/4a
66.29
353
74
<20
59
37
18
<15
30
<20
28
23
116
20
166
17
<20
104
21
85
152
0.9
7.6
TAT/3b
65.79
649
75
<20
63
49
19
<15
30
<20
39
27
136
20
140
18
<20
125
22
99
175
0.9
8.8
TAT/2
65.08
347
72
<20
67
45
17
<15
40
<20
32
20
123
20
133
19
<20
116
25
89
158
1.0
7.9
TAT/1b
64.47
325
67
<20
108
77
16
<15
30
<20
46
21
103
20
193
20
<20
92
22
79
142
1.0
7.0
HTE/15
110.13
433
80
<20
74
33
20
<15
46
<20
50
21
128
20
118
20
<20
94
31
102
170
1.0
8.5
HTE/14
109.78
520
75
<20
72
38
24
<15
44
<20
50
32
126
20
122
20
<20
108
29
100
189
1.0
9.4
HTE/13b
108.98
469
89
<20
75
33
21
<15
44
20
50
20
126
20
116
20
<20
108
34
100
160
1.0
8.0
HTE/12
107.65
207
55
<20
41
<20
10
<15
86
<20
23
19.6
56
25.1
239
20
<20
59
16
42
88
0.8
3.5
HTE/11b
105.78
158
56
<20
49
<20
<10
<15
72
<20
29
<20
57
20
164
20
<20
33
27
42
70
1.0
3.5
HTE/11a
104.98
354
88
<20
52
34
13
<15
48
<20
32
31
97
20
211
20
<20
98
34
73
124
1.0
6.2
HTE/9b
101.38
1468
53
<20
59
34
12
<15
39
<20
27
<20
81
20
238
20
<20
123
18
68
125
1.0
6.2
HTE/9a
100.97
398
82
20
74
32
19
<15
46
<20
37
34
124
20
141
20
<20
103
22
83
170
1.0
8.5
HTE/8
100.40
606
88
<20
49
24
13
<15
64
<20
27
36
135
20
184
20
<20
71
17
53
146
1.0
7.3
HTE/7b
100.00
560
30
<20
51
<20
11
<15
63
<20
29
<20
68
27
212
20
<20
72
19
46
90
0.7
3.3
HTE/7a
98.73
391
83
24
83
44
20
<15
44
<20
42
26.5
126
21.1
142
20
<20
105
20
88
167
0.9
7.9
HTE/6
97.90
352
126
<20
63
26
20
<15
44
<20
33
30
110
20
177
20
<20
93
31
79
175
1.0
8.7
HTE/5a
96.83
369
88
<20
87
31
21
<15
43
<20
36
23
133
20
108
20
<20
100
23
97
187
1.0
9.3
HTE/4b
94.90
384
54
<20
78
33
24
<15
42
<20
38
28
139
20
109
20
<20
118
19
97
160
1.0
8.0
HTE/3a
94.20
600
79
<20
72
29
20
<15
30
<20
38
23
111
20
152
20
<20
96
22
81
144
1.0
7.2
HTE/2b
93.63
402
114
<20
74
33
18
<15
30
<20
38
32
148
20
114
20
<20
126
22
92
204
1.0
10.2
HTE/2a
92.73
446
65
21
67
31
22
<15
30
<20
53
25
149
20
102
20
<20
114
27
96
186
1.0
9.3
HTE/1d
91.07
453
79
<20
90
28
18
<15
38
<20
40
27
141
20
167
20
<20
91
22
75
158
1.0
7.9
HTE/1c
90.63
169
37
<20
44
<20
<10
<15
92
<20
<20
<20
51
24
151
20
<20
32
13
34
86
0.8
3.6
HTE/1b
90.07
505
83
<20
55
59
19
<15
44
<20
34
28.5
155
20
122
20
<20
89
19
102
182
1.0
9.1
HTE/1a
89.30
333
30
<20
34
<20
<10
<15
79
<20
<20
<20
45
25
192
20
<20
35
15
32
68
0.8
2.8
TGR-C/20b
94.61
332
59
<20
82
33
21
<15
56
<20
47
30
129
20
106
20
<20
106
26
90
189
1.0
9.5
TGR-C/20a
93.78
378
77
<20
79
38
23
<15
36
<20
53
34
133
20
110
20
<20
110
27
94
173
1.0
8.6
TGR-C/19b
93.36
332
77
<20
57
30
16
<15
34
<20
39
25
102
25
117
20
<20
90
31
71
152
0.8
6.0
TGR-C/19a
92.49
503
59
<20
54
27
15
<15
30
<20
29
<20
85
20
134
20
<20
78
26
58
141
1.0
7.2
TGR-C/18
91.84
338
49
<20
48
25
17
<15
32
<20
30
<20
95
20
152
20
<20
77
28
62
150
1.0
7.5
TGR-C/17a
91.18
407
91
<20
52
29
17
<15
30
<20
33
35
106
20
144
20
<20
70
23
67
185
1.0
9.2
TGR-C/16b
90.49
379
81
<20
81
37
23
<15
51
<20
34
31
129
20
119
20
<20
113
24
77
192
1.0
9.6
TGR-C/15
89.24
355
51
<20
74
26
21
<15
32
<20
29
31
124
20
120
20
<20
106
23
88
190
1.0
9.5
TGR-C/14b trav
88.49
240
51
<20
36
<20
<10
<15
101
22
<20
<20
48
26
214
20
<20
35
54
32
56
0.8
2.1
TGR-C/14b
87.96
263
71
<20
48
27
<10
<15
80
<20
27
26
72
30
167
20
<20
69
17
51
115
0.7
3.8
TGR-C/13d
86.91
329
82
<20
90
38
22
<15
55
<20
33
31
140
20
95
20
<20
120
21
95
180
1.0
9.0
TGR-C/13b
85.86
479
88
<20
68
41
22
<15
68
<20
44
31
133
20
149
8
<20
109
25
98
161
0.4
8.0
TGR-C/12
84.77
341
52
<20
53
33
16
<15
41
<20
29
20
103
20
188
9
<20
94
26
75
142
0.5
7.1
TGR-C/11b
84.69
578
76
23
78
37
24
<15
61
<20
45
26
140
20
108
20
<20
118
23
90
184
1.0
9.2
TGR-C/11a
84.32
282
56
<20
51
29
12
<15
30
<20
29
<20
91
20
197
10
<20
92
21
70
136
0.5
6.8
TGR-C/10b
84.14
204
30
<20
42
<20
<10
<15
92
<20
<20
<20
39
29
189
20
<20
33
15
29
61
0.7
2.1
TGR-C/10a
83.24
424
93
<20
63
38
19
<15
30
<20
35
32
117
20
177
11
<20
104
24
87
172
0.6
8.6
TGR-C/9
82.66
356
76
<20
48
37
16
<15
30
<20
27
25
101
20
227
12
<20
99
23
78
133
0.6
6.6
TGR-C/8b
82.39
411
74
<20
67
44
20
<15
35
<20
39
25
135
20
193
13
<20
116
21
95
170
0.7
8.5
TGR-C/8a
81.12
314
72
<20
70
30
18
<15
34
<20
29
25
109
24
121
20
<20
93
23
81
152
0.8
6.3
TGR-C/7b
80.01
380
64
<20
70
41
19
<15
44
<20
40
26
129
20
136
14
<20
119
26
92
160
0.7
8.0
TGR-C/6
78.97
291
70
<20
53
35
14
<15
30
<20
28
23
98
20
235
15
<20
95
29
75
134
0.8
6.7
TGR-C/5
78.74
1119
69
<20
59
46
18
<15
54
<20
49
30
126
20
235
16
<20
115
31
98
157
0.8
7.9
TGR-C/4b
78.57
578
72
20
68
36
16
<15
30
<20
38
37
121
20
127
20
<20
103
28
90
171
1.0
8.5
TGR-C/4a
77.87
353
74
<20
59
37
18
<15
30
<20
28
23
116
20
166
17
<20
104
21
85
152
0.9
7.6
TGR-C/3A
77.48
171
33
<20
49
<20
<10
<15
77
<20
20
22
61
20
148
20
<20
44
19
46
103
1.0
5.1
TGR-C/3b
76.80
649
75
<20
63
49
19
<15
30
<20
39
27
136
20
140
18
<20
125
22
99
175
0.9
8.8
TGR-C/2
75.47
347
72
<20
67
45
17
<15
40
<20
32
20
123
20
133
19
<20
116
25
89
158
1.0
7.9
TGR-C/1
75.13
325
67
<20
108
77
16
<15
30
<20
46
21
103
20
193
20
<20
92
22
79
142
1.0
7.0
SHG-D/30
91.20
732
47
<20
50
<20
12
<15
72
<20
27
<20
67
25
227
20
<20
93
25
46
88
0.8
3.5
SHG-D/29a
90.82
609
72
<20
58
36
17
<15
30
<20
46
26
122
20
280
20
<20
137
22
77
155
1.0
7.7
SHG-D/28b
90.45
576
39
<20
46
30
17
<15
30
<20
27
22
97
20
216
20
<20
110
21
64
150
1.0
7.5
SHG-D/27b
90.05
558
81
<20
70
36
23
<15
30
<20
42
33
136
20
192
20
<20
143
24
92
171
1.0
8.6
SHG-D/26b
73.05
547
56
22
45
25
13
<15
30
<20
35
26
81
20
302
20
<20
75
32
59
112
1.0
5.6
SHG-D/25
72.32
444
51
<20
54
35
14
<15
30
<20
32
22
104
20
191
20
<20
101
25
80
131
1.0
6.5
SHG-D/24
71.98
437
60
<20
57
42
16
<15
30
<20
43
29
121
20
197
20
<20
113
23
89
167
1.0
8.3
SHG-D/23j
71.85
386
45
<20
55
29
12
<15
30
<20
29
26
87
20
186
20
<20
88
24
67
136
1.0
6.8
SHG-D/23i
71.38
395
61
<20
58
27
10
<15
30
<20
28
<20
79
20
203
20
<20
71
17
59
104
1.0
5.2
SHG-D/23 h
70.91
399
46
<20
142
22
14
<15
30
<20
53
<20
83
20
214
20
<20
85
24
63
105
1.0
5.3
SHG-D/23f
69.97
432
68
<20
62
30
14
<15
30
<20
24
23
95
20
184
20
<20
79
25
74
107
1.0
5.4
SHG-D/23d
69.03
338
46
<20
54
<20
10
<15
97
<20
28
<20
60
20
213
20
<20
49
18
50
97
1.0
4.8
SHG-D/23b
68.09
475
44
<20
53
27
<10
<15
66
<20
28
22
68
21
180
20
<20
71
22
52
96
1.0
4.7
SHG-D/23a
67.62
483
82
<20
73
37
18
<15
29
<20
41
31
134
20
162
20
<20
124
23
92
173
1.0
8.7
SHG-D/22
67.05
196
33
<20
38
<20
<10
<15
80
<20
21
<20
42
31
247
20
<20
31
16
38
77
0.7
2.5
SHG-D/21
66.70
484
78
<20
93
39
21
<15
41
<20
50
32
135
20
179
20
<20
120
24
99
173
1.0
8.6
SHG-D/20a
65.83
424
55
<20
48
24
15
<15
30
<20
27
23
84
23
152
20
<20
72
19
61
109
0.9
4.8
SHG-D/19
65.42
652
96
31
68
43
21
<15
68
<20
44
30
131
20
170
20
<20
122
22
96
165
1.0
8.3
SHG-D/18
65.11
473
37
<20
47
27
12
<15
30
<20
27
<20
79
24
161
20
<20
77
19
56
95
0.8
4.0
SHG-D/17
64.93
463
64
<20
72
37
20
<15
45
<20
40
31
135
20
152
20
<20
114
25
97
184
1.0
9.2
SHG-D/16b
64.30
472
69
<20
52
25
13
<15
30
<20
28
<20
90
20
159
20
<20
83
21
63
134
1.0
6.7
SHG-D/15
63.26
463
88
<20
73
31
17
<15
55
<20
39
32
135
20
191
20
<20
112
28
95
174
1.0
8.7
SHG-D/14b
62.73
425
65
<20
45
25
13
<15
31
<20
24
23
86
20
167
20
<20
67
29
61
130
1.0
6.5
SHG-D/13
61.98
423
86
<20
54
34
19
<15
74
21
32
28
133
20
210
23
<20
89
34
85
205
1.1
10.3
SHG-D/12
60.80
475
103
<20
55
28
17
<15
60
<20
25
26
138
20
183
20
<20
65
31
76
249
1.0
12.4
SHG-D/11b
58.45
481
101
21
82
40
23
<15
39
21
43
30
155
20
264
23
<20
149
32
113
156
1.1
7.8
SHG-D/10
57.28
636
59
26
88
45
24
<15
47
<20
46
28
157
20
252
21
<20
200
25
119
143
1.1
7.1
SHG-D/9d
57.23
2439
99
<20
68
39
21
<15
65
22
72
27
150
20
283
20
<20
139
37
107
170
1.0
8.5
SHG-D/9c
56.53
414
81
<20
76
32
23
<15
53
<20
35
<20
151
20
173
20
<20
109
27
103
176
1.0
8.8
SHG-D/9b
55.83
435
81
<20
67
28
22
<15
59
<20
40
41
134
20
170
20
<20
89
30
90
189
1.0
9.4
SHG-D/9a
55.13
332
88
<20
60
31
15
<15
61
<20
31
<20
110
20
291
20
<20
72
28
69
273
1.0
13.6
SHG-D/8
54.35
456
56
22
87
43
22
<15
64
<20
49
36
159
20
242
20
<20
122
27
115
171
1.0
8.5
SHG-D/7b
54.18
444
100
<20
69
40
21
<15
59
<20
49
26
136
20
268
20
<20
108
30
102
164
1.0
8.2
SHG-D/6
51.43
185
51
<20
46
<20
<10
<15
106
26
<20
<20
49
22
183
20
<20
39
65
36
71
0.9
3.2
SHG-D/5
50.18
496
71
<20
80
38
22
<15
49
<20
45
37
159
20
216
20
<20
120
33
114
133
1.0
6.7
SHG-D/4
49.35
503
100
<20
76
34
23
<15
45
<20
43
<20
151
20
160
20
<20
122
25
109
153
1.0
7.7
SHG-D/3a
47.55
484
68
<20
82
38
20
<15
30
<20
47
20
141
20
169
20
<20
109
29
104
184
1.0
9.2
SHG-D/2
46.68
693
51
<20
71
29
17
<15
32
<20
40
24
110
20
169
20
<20
97
24
84
152
1.0
7.6
SHG-D/1
45.76
465
83
<20
67
36
19
<15
48
20
42
26
133
20
127
20
<20
117
35
98
199
1.0
9.9
TGR-AB/35
40.46
492
49
24
75
66
24
<15
30
26
72
25
79
20
273
20
<20
56
13
63
165
1.0
8.2
TGR-AB/34b
39.83
445
70
21
67
72
21
<15
44
<20
54
31
155
20
137
20
<20
85
26
111
171
1.0
8.5
TGR-AB/33b
38.36
310
85
<20
63
28
14
<15
30
<20
31
27
117
20
107
20
<20
75
24
72
144
1.0
7.2
TGR-AB/32 l
37.63
380
91
<20
65
32
15
<15
30
<20
34
22
130
20
126
20
<20
89
25
89
176
1.0
8.8
TGR-AB/32j
35.70
380
91
<20
65
32
15
<15
30
<20
34
22
130
20
126
20
<20
89
25
89
176
1.0
8.8
TGR-AB/32i
34.73
424
86
<20
62
27
18
<15
57
<20
34
31
135
20
159
20
<20
107
28
93
160
1.0
8.0
TGR-AB/32 h
33.76
286
63
<20
61
30
16
<15
30
<20
30
<20
119
22
107
20
<20
89
23
79
135
0.9
6.1
TGR-AB/32f
31.83
400
68
<20
61
32
13
<15
49
<20
31
24
119
20
152
20
<20
85
23
78
173
1.0
8.6
TGR-AB/32d
29.90
854
61
<20
61
30
16
<15
30
<20
35
23
125
20
179
20
<20
82
28
82
156
1.0
7.8
TGR-AB/32a
27.00
532
99
<20
61
25
18
<15
49
<20
32
40
144
20
165
21
<20
83
25
84
169
1.1
8.5
TGR-AB/31
25.30
441
93
<20
75
32
20
<15
53
<20
37
25
141
20
186
22
<20
115
25
92
270
1.1
13.5
TGR-AB/13
8.15
495
98
<20
59
22
21
<15
67
<20
<20
20
159
20
153
24
<20
58
28
66
316
1.2
15.8
TGR-AB/12
7.98
4111
62
46
72
40
23
<15
47
<20
50
24
151
20
252
31
<20
250
27
95
230
1.5
11.5
TGR-AB/11a
6.82
481
54
<20
32
<20
16
<15
31
<20
<20
20
145
20
142
20
<20
47
18
51
227
1.0
11.3
TGR-AB/9
3.46
481
62
28
83
46
24
<15
30
<20
64
37
139
20
123
27
<20
160
20
76
274
1.4
13.7
Major, minor and trace element composition of sediments from the Tsagaan Ovoo Fm., Hsanda Gol Fm. and Loh Fm. (Valley of Lakes, Central Mongolia) based on XRF data and percent in major mineralsThe averaged CIA values (left part of Fig. 6) ranged between 70 and 76 and plot slightly below the field of illite (75–90). This indicates that the Tsagaan Ovoo to Loh fms. sediments underwent sustained chemical weathering, considering that fresh basalt, unweathered granite and granodiorite and feldspar have CIA values of 30–45, 45–55 and 50, respectively (Bahlburg and Dobrzinski 2011). Moreover, by transferring the XRF data in Nesbitt and Young`s (1984) A-CN-K (Al2O3-CaO* + Na2O-K2O) diagram (Fig. 6), it becomes clear that the majority of the samples plot either near the compositional range of Post-Archean average Australian Shale (PAAS) and Average Proterozoic Shale (APS) or follow the predicted weathering trend for basalt protolith and Upper Continental Crust (UCC) rocks (von Eynatten 2004; Bahlburg and Dobrzinski 2011 and references herein). This observation demonstrates that sorting, K-metasomatism and frictional variations in palaeo-climate and tectonic setting played only a minor role in affecting the chemical composition of the sediments and basalt groups I to II, in contrast to the pronounced illitization event(s) (Fedo et al. 1995; Armstrong-Altrin et al. 2004; Yang et al. 2004).
Fig. 6
A-CN-K (Al2O3-CaO* + Na2O-K2O) diagram of Nesbitt and Young (1984) showing the chemical compositions of intensively weathered (calcareous and illitized) sediments from the Tsagaan Ovoo Fm., Hsanda Gol Fm. and Loh Fm. (Valley of Lakes, Central Mongolia). Compositions of Upper Continental Crust (UCC), Average Proterozoic Shale (APS), Post-Archean average Australian Shale (PAAS) and basalt protolith (1) are included for comparison (Bahlburg and Dobrzinski 2011 and references herein). Note that the lower part of the diagram (A < 40) is not shown. The range and averages (dots) of the CIA values are indicated in the left part of the figure
A-CN-K (Al2O3-CaO* + Na2O-K2O) diagram of Nesbitt and Young (1984) showing the chemical compositions of intensively weathered (calcareous and illitized) sediments from the Tsagaan Ovoo Fm., Hsanda Gol Fm. and Loh Fm. (Valley of Lakes, Central Mongolia). Compositions of Upper Continental Crust (UCC), Average Proterozoic Shale (APS), Post-Archean average Australian Shale (PAAS) and basalt protolith (1) are included for comparison (Bahlburg and Dobrzinski 2011 and references herein). Note that the lower part of the diagram (A < 40) is not shown. The range and averages (dots) of the CIA values are indicated in the left part of the figureThe positive correlation of large-ion lithophile elements such as K, Rb and Ba (also-called LILE) as well as Cr, Zn and V with Al2O3 suggests their incorporation in sheet silicates, i.e. illite and I-S, and/or sorption onto clay mineral surfaces (Table 1). High K2O/Rb ratios, in the range from 165 to 384, point to moderate-to-high weathering intensities and arid to semiarid climatic conditions (Jin et al. 2006), a feature confirmed by the high CIA values. The low but highly variable Sr contents (95–330 ppm; Fig. 5) roughly correspond to variations in the fraction of calcite present in calcrete horizons (Table 1). The patterns of Co, Cu, Ga, Hf, Nb, Ni, Pb and U are mostly inconspicuous. However, positive trends of the heavy rare earth element (HREE) Y, with incompatible TiO2 and the immobile high field strength elements (HFSE) Ce, La, Sc, (Th) and Zr (Table 1), point to their presence in heavy minerals that have been delivered from metamorphosed and magmatic source rocks exposed in the hinterland (McLennan et al. 1993).The δ18O values of carbonates present in calcrete horizons in the lower part of the Hsanda Gol Fm., i.e. below the basalt I group, reveal the heaviest isotopic signatures throughout the entire investigated succession and very high variation in the range from −0.2 to −9.3‰ (see Fig. 2 and Table 2). A significantly lower scatter in the δ18O values, from −7.0 to −9.6‰, is evident above the basalt I group in the Hsanda Gol Fm. In the Loh Fm. at the Hotuliin Teeg section, the δ18O values show again higher variability with values from −12.9 to −8.6‰. Overall, an evolution towards progressively lighter δ18O values of the carbonate is evident up-section in the profile, starting in the upper biozone B.
Table 2
δ13C and δ18O isotope composition of sediments from the Tsagaan Ovoo Fm., Hsanda Gol Fm. and Loh Fm. (Valley of Lakes, Central Mongolia)
BIOZONE
High in profile (m)
SAMPLE
δ13Ccarb, V-PDB
δ18Ocarb, V-PDB
Biozone D
108.42
HTE/13a carb
−8.1
−10.2
Biozone D
107.65
HTE/12 carb
−4.4
−8.6
Biozone D
105.78
HTE/11b carb
−5.4
−8.9
Biozone D
104.98
HTE/11a carb
−7.3
−11.0
Biozone D
101.38
HTE/9b carb
−5.1
−9.5
Biozone D
100.97
HTE/9a carb
−6.3
−11.2
Biozone D
100.40
HTE/8 carb
−6.1
−10.6
Biozone D
100.00
HTE/7b carb
−5.7
−8.9
Biozone D
98.73
HTE/7a carb
−6.4
−11.7
Biozone C1-D
97.90
HTE/6 carb
−6.3
−10.3
Biozone C1-D
97.50
HTE/5b carb
−8.9
−10.2
Biozone C1-D
94.90
HTE/4b carb
−9.0
−12.9
Biozone C1-D
94.43
HTE/4a carb
−6.3
−9.6
Biozone C1-D
94.20
HTE/3A carb
−9.4
−11.0
Biozone C1-D
94.00
HTE/3 carb
−8.8
−11.0
Biozone C1-D
93.36
TGR-C/19b
−3.8
−8.7
Biozone C1-D
92.49
TGR-C/19a
−4.8
−8.5
Biozone C1
91.84
TGR-C/18
−4.7
−7.8
Biozone C1
91.41
TGR-C/17b
−5.0
−8.6
Biozone C1
91.18
TGR-C/17a
−4.5
−8.3
Biozone C1
91.06
TGR-C/16c
−4.9
−8.5
Biozone C1
89.24
TGR-C/15
−6.1
−7.8
Biozone C1
88.49
TGR-C/14b
−6.1
−9.1
Biozone C1
85.86
TGR-C/13b
−5.7
−9.1
Biozone C1
84.77
TGR-C/12
−5.4
−7.7
Biozone C1
84.32
TGR-C/11a
−6.8
−9.1
Biozone C1
84.14
TGR-C/10b
−5.9
−9.6
Biozone C
83.24
TGR-C/10a
−5.7
−7.8
Biozone C
82.66
TGR-C/9
−5.8
−8.8
Biozone C
82.39
TGR-C/8b
−5.6
−7.6
Biozone C
81.12
TGR-C/8a
−5.8
−8.3
Biozone C
80.49
TGR-C/7c
−5.5
−9.1
Biozone C
80.01
TGR-C/7b
−5.4
−9.3
Biozone C
79.52
TGR-C/7a
−5.9
−7.6
Biozone C
78.97
TGR-C/6
−5.9
−9.2
Biozone C
78.74
TGR-C/5
−5.4
−9.2
Biozone C
78.57
TGR-C/4b
−5.6
−8.1
Biozone C
77.87
TGR-C/4a
−5.6
−8.7
Biozone C
77.48
TGR-C/3A
−6.1
−8.8
Biozone C
77.40
TGR-C/3c
−5.1
−7.0
Biozone C
76.80
TGR-C/3b
−5.5
−8.8
Biozone C
76.20
TGR-C/3a
−5.3
−8.6
Biozone C
75.47
TGR-C/2
−5.9
−8.6
Biozone C
75.13
TGR-C/1
−5.9
−9.2
Biozone B
72.32
SHG-D/25
−5.4
−8.8
Biozone B
71.98
SHG-D/24
−5.2
−9.3
Biozone B
71.85
SHG-D/23j
−5.5
−8.5
Biozone B
71.38
SHG-D/23i
−5.3
−8.3
Biozone B
70.91
SHG-D/23 h
−5.4
−8.5
Biozone B
70.44
SHG-D/23 g
−5.0
−8.2
Biozone B
69.97
SHG-D/23f
−5.2
−8.3
Biozone B
69.50
SHG-D/23e
−5.3
−7.9
Biozone B
69.03
SHG-D/23d
−5.4
−8.1
Biozone B
68.56
SHG-D/23c
−4.6
−7.8
Biozone B
68.09
SHG-D/23b
−5.4
−8.3
Biozone B
67.62
SHG-D/23a
−5.0
−8.9
Biozone B
67.05
SHG-D/22
−5.2
−8.8
Biozone B
66.70
SHG-D/21
−5.1
−9.1
Biozone B
66.40
SHG-D/20b
−5.5
−8.3
Biozone B
65.83
SHG-D/20a
−5.8
−7.9
Biozone B
65.42
SHG-D/19
−4.9
−8.1
Biozone B
65.11
SHG-D/18
−5.3
−8.1
Biozone B
64.93
SHG-D/17
−5.1
−9.2
Biozone B
64.73
SHG-D/16c
−5.6
−7.8
Biozone B
64.30
SHG-D/16b
−5.6
−8.3
Biozone B
63.86
SHG-D/16a
−5.5
−7.9
Biozone B
63.26
SHG-D/15
−5.1
−8.6
Biozone B
62.73
SHG-D/14b
−5.9
−8.0
Biozone B
62.43
SHG-D/14a
−5.6
−8.6
Biozone B
61.98
SHG-D/13
−5.3
−7.6
Biozone B
51.43
SHG-D/6
−7.3
−8.5
Biozone B
46.68
SHG-D/2
−7.6
−8.7
Biozone A
38.73
TGR-AB/33c
−9.2
−9.1
Biozone A
38.36
TGR-AB/33b
−8.3
−8.6
Biozone A
38.00
TGR-AB/33a
−7.2
−9.3
Biozone A
37.63
TGR-AB/32 l
−7.5
−8.4
Biozone A
36.66
TGR-AB/32 k
−7.0
−8.9
Biozone A
35.70
TGR-AB/32j
−7.0
−4.6
Biozone A
34.73
TGR-AB/32i
−6.8
−1.5
Biozone A
33.76
TGR-AB/32 h
−6.9
−7.2
Biozone A
32.80
TGR-AB/32 g
−6.6
−8.6
Biozone A
31.83
TGR-AB/32f
−6.8
−2.6
Biozone A
30.86
TGR-AB/32e
−6.8
−0.2
Biozone A
29.90
TGR-AB/32d
−6.7
−5.8
Biozone A
28.93
TGR-AB/32c
−6.4
−8.4
Biozone A
27.96
TGR-AB/32b
−7.2
−6.1
Biozone A
27.00
TGR-AB/32a
−7.0
−6.9
Biozone C1
91.20
SHG-D/30
−5.5
−8.1
Biozone C1
91.00
SHG-D/29b
−5.7
−8.2
Biozone C1
90.82
SHG-D/29a
−5.4
−8.8
Biozone C1
90.18
SHG-D/28a
−5.4
−8.4
Biozone C1
89.55
SHG-D/26b
−5.6
−8.8
Biozone C1
89.15
SHG-D/26a
−5.5
−10.3
Biozone C1-D
96.11
TAT/33b
−5.3
−9.6
Biozone C1-D
95.18
TAT/33a
−4.9
−9.7
Biozone C1-D
94.71
TAT/32d
−4.7
−8.8
Biozone C1-D
94.19
TAT/32c
−5.1
−9.6
Biozone C1-D
93.66
TAT/32b
−5.4
−9.5
Biozone C1-D
93.14
TAT/32a
−5.1
−9.0
Biozone C1-D
93.07
TAT/31
−5.4
−8.9
Biozone C1-D
92.99
TAT/30b
−5.6
−9.4
Biozone C1
91.22
TAT/28
−4.9
−9.0
Biozone C1
91.09
TAT/27b
−5.4
−9.5
Biozone C1
90.76
TAT/27a
−5.2
−9.3
Biozone C1
90.01
TAT/25
−5.0
−8.4
Biozone C1
88.81
TAT/23
−5.2
−9.0
Biozone C1
88.64
TAT/22d
−5.2
−9.3
Biozone C1
87.94
TAT/22c
−4.9
−9.2
Biozone C1
87.24
TAT/22b
−4.9
−8.9
Biozone C1
86.54
TAT/22a
−4.9
−9.2
Biozone C1
83.87
TAT/18a
−5.0
−9.3
Biozone C
83.54
TAT/17c
−4.7
−8.8
Biozone C
83.24
TAT/17b
−4.8
−9.0
Biozone C
82.94
TAT/17a
−4.8
−9.2
Biozone C
82.64
TAT/16b
−4.8
−9.7
Biozone C
82.11
TAT/16a
−4.9
−9.6
Biozone C
81.84
TAT/15c
−4.8
−9.2
Biozone C
81.26
TAT/15b
−4.2
−8.6
Biozone C
80.67
TAT/15a
−5.5
−9.7
Biozone C
80.09
TAT/14b
−4.9
−9.2
Biozone C
79.59
TAT/14a
−4.9
−9.0
Biozone C
79.04
TAT/12c
−4.8
−8.8
Biozone C
78.47
TAT/12b
−4.8
−8.6
Biozone C
77.91
TAT/12a
−4.8
−8.9
Biozone B
68.99
TAT/8c
−4.7
−8.7
Biozone B
68.32
TAT/8a
−4.5
−8.9
Biozone B
67.99
TAT/7b
−4.7
−8.8
Biozone B
67.62
TAT/7a
−4.6
−8.7
Biozone B
67.44
TAT/6c
−4.5
−8.8
Biozone B
67.24
TAT/6b
−4.6
−8.8
Biozone B
67.04
TAT/6a
−4.6
−8.9
Biozone B
66.77
TAT/5
−4.6
−8.7
Biozone B
66.62
TAT/4b
−4.6
−8.7
Biozone B
66.29
TAT/4a
−4.7
−9.1
Biozone B
66.12
TAT/3c
−4.8
−9.4
Biozone B
65.79
TAT/3b
−4.5
−8.3
Biozone B
65.08
TAT/2
−4.8
−8.8
Biozone B
65.00
TAT/1c
−4.7
−8.7
Biozone B
64.47
TAT/1b
−4.9
−9.3
Biozone B
63.93
TAT/1a
−4.8
−9.1
δ13C and δ18O isotope composition of sediments from the Tsagaan Ovoo Fm., Hsanda Gol Fm. and Loh Fm. (Valley of Lakes, Central Mongolia)Below 55 m in the profile (in the lower part of the Hsanda Gol Fm.), the δ13C values vary from −6.4 to −7.6‰, except for the two samples taken immediately below basalt I, which yielded −9.2 and −8.3‰ of δ13C, respectively. The remaining sections of the Hsanda Gol Fm. display heavier δ13C values, ranging from −6.8 to −3.8‰. Only two outliers were recognised, with δ13C value of approximately −7.2‰ (TAT 24 and TGR-C 11). Finally, the Loh Fm. is characterised, as for the δ18O values, by a stronger variability in the δ13C values in the range from −9.4 to −4.4‰.
Discussion
Based on a seminal sedimentological, petrographic and chemical description of the Eocene to Miocene sedimentary succession and embedded basalt groups I to III, Höck et al. (1999) discussed the provenance of the sediments from the Valley of Lakes (Mongolia) and proposed a partly aeolian origin for the finest fraction of the Hsanda Gol to Loh fms. Their hypothesis was mainly based on a general coincidence between the grain size distribution patterns of the Valley of Lakes sediments compared with those of modern Loess deposits from Kansas. However, Höck et al. (1999) noticed some discrepancies in the grain size distribution patterns of sediments from the Hsanda Gol and Loh fms. and interpreted them to be attributed either to short distance aeolian transport or coupled aeolian–fluvial transport mechanisms. Sun and Windley (2015) proposed an aeolian origin of the fine fraction based on REE patterns and comparison of grain size distribution patterns with that from the modern Chinese Loess Plateau. They concluded that the finest fraction of the Hsanda Gol and Loh fms. was deposited along with the Cenozoic cooling through long distance transport.The herein obtained mineralogical and petrographic results (Figs. 3 and 4), however, clearly reveal a diagenetic origin of illite, which represents a main constituent of the fine fraction of the Hsanda Gol and Loh fms. Moreover, the association of hairy 1 M illite, flaky 1Md I-S and macroquartz cement in the sediments points to a formation during the advanced stages of sandstone diagenesis at elevated temperatures (70 to 150 °C), which is in contrast to the very low burial (in the range of a few hundred metres) proposed for the Valley of Lakes sediments. Thus, there is an apparent inconsistency between the actual literature and our results, particularly regarding the mineralogical and palaeo-climatic evolution of the Valley of Lakes sediments. We present here a new model for the post-depositional history of this famous study site, besides discussing implications for changes in the palaeo-climatic evolution reflected in the Valley of Lakes sediments.
A revised model for the post-depositional evolution of the Valley of Lakes sediments
The source rock composition, depositional environment and potential recycling processes can be identified using trace element composition data of bulk rock samples. Positive trends of the HREE with TiO2 and HFSE (Table 1) point to their incorporation in heavy minerals present in the Hsanda Gol and Loh fms. sediments. These heavy minerals have been delivered from metamorphic and magmatic source rocks exposed in the hinterland of the Valley of Lakes (McLennan et al. 1993). Based on gravel lithologies, Höck et al. (1999) demonstrated that the samples from the Tsagaan Ovoo to Loh fms. are predominated by quartz, pegmatite, granite, siltstone, basalt and carbonate clasts, with the heavy mineral fraction containing epidote, zircon, tourmaline, garnet, rutile, pyroxene, amphibole and sphene. Such a diamictic composition suggests a heterogeneous provenance of the gravel components being influenced by basic to intermediate, low- to medium-grade metamorphic and magmatic source rocks of Late Proterozoic to Late Permian age, which crop out in the catchment areas of the alluvial fans (Zorin et al. 1993). Despite the fact that the heavy mineral spectra are comparable throughout the entire Tsagaan Ovoo to Loh fms., recycling of older sediments and long transport distances are considered unlikely because multiple reworking-(re)deposition cycles typically result in a strong enrichment of Zr and in a depletion of Sc and Th. The Th/Sc vs. Zr/Sc cross-plot (Fig. 7) is a sensitive indicator for studying the source rock composition. This plot reveals that the investigated sediments have an upper crustal composition and were virtually not affected by post-depositional recycling processes. Even though an aeolian origin of the finest fraction cannot be ruled out based on the trace element data presented here, this finding suggests that the immature (arkosic) mud- to sandstones from the Hsanda Gol and Loh fms. were primarily derived from alluvial fans that have formed the upper Tsagaan Ovoo sediments. The latter feature is confirmed by remarkable lithological changes observed throughout the entire sedimentary succession (Fig. 3), which were interpreted to reflect changes in the depositional environment during the Eocene to Miocene. This is expressed in the Tsagaan Ovvo Fm. being dominated by braided fluvial fan and lake deposits (Höck et al. 1999: 92–100, Daxner-Höck et al. 2017, this issue), whereas the Hsanda Gol sediments represent ephemeral lake to braided fluvial fan deposits that are affected by re-sedimentation of the underlying Tsagaan Ovo Fm. (Badamgarav 1993; Höck et al. 1999). Finally, the Loh sediments are of similar composition but contain reworked lithoclasts from the basalt I and Hsanda Gol sediments (Daxner-Höck et al. 2017, this issue) and thus can be easily differentiated from the former.
Fig. 7
Th/Sc versus Zr/Sc cross-plot of McLennan (1993) demonstrating that the investigated samples from the Tsagaan Ovoo to Loh fms. plot well in the field of the upper crustal rocks and cluster around the compositions of the Upper Continental Crust (UCC), Average Proterozoic Shale (APS) and Post-Archean average Australian Shale (PAAS). This indicates that sediment recycling was insignificant (Bahlburg and Dobrzinski 2011)
Th/Sc versus Zr/Sc cross-plot of McLennan (1993) demonstrating that the investigated samples from the Tsagaan Ovoo to Loh fms. plot well in the field of the upper crustal rocks and cluster around the compositions of the Upper Continental Crust (UCC), Average Proterozoic Shale (APS) and Post-Archean average Australian Shale (PAAS). This indicates that sediment recycling was insignificant (Bahlburg and Dobrzinski 2011)However, a pre-condition required for the accurate interpretation of mineralogical as well as major and trace element signatures of bulk samples is the identification of distinct weathering paths (Zhang et al. 2014). Hydrolysis, leaching, sorting of sediments and diagenesis, for instance, result in distinct chemical, mineralogical and physical changes in the sediments and sedimentary rocks. Such processes have to be considered in the assessment of source rock compositions, depositional settings and sedimentary recycling processes and can be traced by means of the CIA, which provide a quantitative measure for tracing physical and chemical weathering (McLennan et al. 1993; Bauluz et al. 2000; Jin et al. 2006; Bahlburg and Dobrzinski 2011). The obtained CIA values, from 70 to 76, suggest that chemical weathering of the (arkosic) sandstones occurred during illitization (Fig. 4). This unidirectional weathering pathway can also be followed by the A-CN-K diagram (Fig. 6), where sorting, K-metasomatism and frictional variation in the provenance of sediments played only a minor role on affecting the bulk sediment’s mineralogical and geochemical signatures compared with their strong modification associated with the illitization (Nesbitt and Young 1984; Fedo et al. 1995; Yang et al. 2004; Bahlburg and Dobrzinski 2011).The post-depositional alteration of the mostly (arkosic) mud- to sandstones need temperature around 70 to 150 °C. As the geological setting does not allow diagenesis through burying, we propose that hydrothermal fluids were the driving force for this diagenetic pathway. As samples post-basalt group II are affected in the same way than older ones, this hydrothermalism should have been active from Miocene to present. We thus propose that the latest illitization event co-occurred with the deposition of the basalt III during the middle Miocene at ~13 Ma, even if this basalt group has, today, a smaller geographic expansion than the Hsanda Gol Fm. The hydrothermal alteration of K-feldspar provided the K+ and Al3+ ions and the silicic acid to the interstitial solution, which are required both for the growth of discrete illite and I-S and for the syntaxial overgrowth of quartz as soon as a certain supersaturation threshold, with respect to these mineral phases, was reached in the interstitial solution (e.g. Hower et al. 1976; Bauer et al. 2000; Baldermann et al. 2012). This conceptual model is adequate to explain: (i) the predominance of illite and quartz (33 ± 8 and 35 ± 9 wt%, on average), (ii) the very low orthoclase content (2 ± 1 wt%, on average) observed throughout the sedimentary succession and (iii) the local restricted occurrences of zeolite and vermiculite associated with intensively weathered amphibole minerals originally present in basalt (Fig. 3). Kaolinite and chlorite could have also been formed by a dissolution–precipitation mechanism simultaneously and/or soon after the multi-stage illitization event(s), but they can be allochthonous in origin as well (Lanson et al. 1996; Beaufort et al. 2016). Even if we assume an allochthonous origin of kaolinite and chlorite, their occurrence in trace amounts (<2 wt%) contradicts the pronounced large aeolian deposition previously proposed by Sun and Windley (2015). In consequence, we cannot exclude local and short-distance aeolian contribution to the fluvial and lake deposit sedimentation, as it is common in arid to semi-arid environments (e.g. Xiao et al. 2010; Licht et al. 2014, 2016a), but apparently, we found no mineralogical and geochemical evidence for long distance transport and/or large aeolian deposition.
Processes controlling the (isotope) geochemical composition of soil carbonates
The illitization resulted in a strong mineralogical and chemical overprinting of the Hsanda Gol to Loh sediments, implying that any palaeo-climatic information recorded in the paleosols could have been disturbed during post-depositional alteration. Moreover, the pristine δ13C and δ18O isotopic signatures of soil carbonate are often affected by exposure to meteoric or hydrothermal fluids (Marshall 1992), burial diagenesis (e.g. Marshall 1992; Kaufman and Knoll 1995) and oxidation of organic matter (Kent-Corson et al. 2009). Thus, palaeo-environmental reconstructions based on isotopic signatures of carbonate present in calcrete have to be interpreted carefully.We propose, however, that the δ13C and δ18O isotope composition of soil carbonate was not disturbed by the post-depositional illitization event(s) and still records the climatic conditions prevailing during the precipitation of calcite from meteoric solutions, for the following reasons: (i) the δ13C and δ18O profiles should show a covariation in the case of strong diagenetic overprinting, which is apparently not the case here (Fig. 8), and (ii) δ13C and δ18O signatures are more prone to diagenetic alteration in a siliciclastic matrix than in pure carbonates (Kaufman and Knoll 1995). However, our isotopic values show no correlation with the total amount of carbonate present in the bulk samples (Fig. 9).
Fig. 8
δ13C vs. δ18O cross plot. Soil carbonates collected in close vicinity to the basalt horizons (red squares) show some signs of alteration through interaction with hydrothermal fluids. Samples from the Lower Hsanda Gol Fm. (green squares) indicate formation in a playa-like environment. The majority of the samples (blue rhombs) preserved their pristine δ13C and δ18O isotope signature of paleosol formation and can be used for palaeo-climatic interpretations
Fig. 9
δ13C vs. total calcite (expressed as wt.% CaCO3) cross plot, showing that the vast majority of the soil carbonate is authigenic in origin and resistant to diagenetic overprinting. Red squares represent samples taken in close vicinity to the basalt groups I and II. See text for explanations
δ13C vs. δ18O cross plot. Soil carbonates collected in close vicinity to the basalt horizons (red squares) show some signs of alteration through interaction with hydrothermal fluids. Samples from the Lower Hsanda Gol Fm. (green squares) indicate formation in a playa-like environment. The majority of the samples (blue rhombs) preserved their pristine δ13C and δ18O isotope signature of paleosol formation and can be used for palaeo-climatic interpretationsδ13C vs. total calcite (expressed as wt.% CaCO3) cross plot, showing that the vast majority of the soil carbonate is authigenic in origin and resistant to diagenetic overprinting. Red squares represent samples taken in close vicinity to the basalt groups I and II. See text for explanationsSoil carbonate frequently comprises of authigenic (i.e. calcrete), secondary (i.e. calcite spar) and detrital (i.e. lithoclasts) carbonate that may carry different δ13C and δ18O signatures. From a petrological point of view, the most widely absence of secondary calcite spar and dolomite, and the preservation of the crypto- to microcrystalline, honeycomb-like texture of calcite suggest that there is no other significant source of detrital and secondary calcite that could disturb the bulk δ13C and δ18O signatures of carbonate bound to paleosol horizons. In order to prove that the authigenic calcrete nodules and lenses account for ~100% of the soil carbonate, some samples were analysed for their δ13C and δ18O isotope bulk composition (Table 3). These values indicate that only few samples containing less than 10 wt% of calcite could be influenced by small abundances of detrital carbonate, but they do not blur the δ13C and δ18O signatures of the authigenic soil carbonate.
Table 3
δ13C and δ18O isotope composition measured on bulk rock and on calcrete nodules and lenses extracted from the same samples. These values indicate that only few samples with <10 wt% of calcite may be influenced by detrital and/or secondary carbonate minerals
LECO
Calcrete
Bulk
CaCO3
δ13C
δ18O
δ13C
δ18O
%
(‰), VPDB
(‰), VPDB
(‰), VPDB
(‰), VPDB
HTE/13a
6.9
−8.1
−10.2
−6.4
−9.7
HTE/12
51.2
−4.4
−8.6
−4.6
−8.5
HTE/11b
54.6
−5.4
−8.9
−5.3
−8.8
HTE/11a
3.8
−7.3
−11.0
−7.1
−10.7
HTE/9b
28.4
−5.1
−9.5
−5.2
−9.4
HTE/9a
3.8
−6.3
−11.2
−6.3
−11.3
HTE/8
5.0
−6.1
−10.6
−6.2
−10.9
HTE/7b
46.0
−5.7
−8.9
−5.5
−9.4
HTE/7a
2.8
−6.4
−11.7
−6.6
−11.5
HTE/6
11.8
−6.3
−10.3
−6.5
−10.4
HTE/1e
38.9
−5.9
−10.3
−6.2
−10.3
HTE/1d
4.9
−6.9
−11.7
−7.0
−11.9
HTE/1c
61.2
−6.2
−9.5
−6.0
−10.0
HTE/1a
67.2
−6.2
−10.1
−6.3
−10.1
δ13C and δ18O isotope composition measured on bulk rock and on calcrete nodules and lenses extracted from the same samples. These values indicate that only few samples with <10 wt% of calcite may be influenced by detrital and/or secondary carbonate mineralsThe only exception is the carbonate samples collected in close vicinity to the prominent horizons of basalt groups I and II (Figs. 2 and 8, red squares), which display notably lighter δ13C (and δ18O for basalt II) values, compared with the rest of the calcrete samples (Figs. 2 and 8, blue rhombs). During volcanic activity associated with the development of the basalt groups, 12C–12C bonds break more easily than 12C–13C bonds, and the result is that residual carbonates, after vaporization, typically show more negative δ13C values than their precursor phase (Valley 1986; Richoz 2006). Thus, these samples (two samples taken below basalt I at the Taatsiin section and few samples collected at different levels around basalt II at the Hutuliin Teeg section) have not been considered in the climatic trends discussed below.Considering, however, that most of the calcrete samples preserved their pristine δ18O and δ13C signatures of formation, palaeo-climatic trends can be interpreted based on changes in the δ13C curve (Fig. 2). The δ13C record of the soil carbonate is ultimately linked to variations in the isotopic composition of the soil solution from which the calcrete nodules and lenses have been precipitated (Schön et al. 2016). However, the δ13C isotopic composition of the soil solution can be modified in various ways. For instance, CO2 present in soil is a mixture of two isotopically distinct endmembers, namely atmospheric CO2 and CO2 derived from the in situ oxidation of organic matter present in soils (e.g. Khadikikar et al. 2000). Changes in the relative abundance of these isotopically different carbon pools and subsequent fractionation of the oxygen and carbon isotopes during (re)equilibration of CO2 with the soil solution greatly modify the δ13C signal of the precipitating calcite. Stratigraphic changes in δ13Csoil (and accordingly in the δ13Ccarbonate) values follow the: (i) variations in aridity, (ii) changes in the atmospheric pCO2 and (iii) changes in proportion between the C4/C3 photosynthesis pathways of plants. In our case, this last point cannot have any effect as C4 plants arrived in Mongolia not before late Miocene (Zhang et al. 2009; Edwards et al. 2010). From ~33 to 22 Ma, the atmospheric CO2 concentration decreased from 800 to 200 ppm (Zhang et al. 2013), which should be translated in a trend towards lighter δ13Csoil values. We do not see this trend in our data, and thus, changes in aridification in Central Mongolia may have overprinted this effect.Increases in aridity can increase the δ13C of soil carbonate in three ways: (1) water stress induces a limitation of diffusion during photosynthesis, which increases the δ13C in plants (Kohn 2010); (2) a decrease in plant productivity, which increases the ratio of atmospheric CO2 to soil respired CO2 (Cerling 1984; Takeuchi et al. 2010); and (3) a shallowing of soil carbonate formation due to reduced infiltration, which also increases the ratio of atmospheric CO2 relative to the contribution of δ13Csoil. The abovementioned processes result in an increase in δ13C (Caves et al. 2014), but the decrease in plant productivity is proven to have the largest effect (Cerling and Quade 1993; Caves et al. 2014). In summary, a positive excursion of the δ13C signature of soil carbonate (i.e. calcrete nodules) preserved in the paleosols of the Valley of Lakes sediments is ultimately linked to aridification.δ18O values of pedogenic carbonates are mainly determined by the δ18O composition of the soil water, which in turn is strongly related to the δ18O composition of local meteoric water, being affected by soil temperature and evaporation rate (Cerling 1984; Quade et al. 1989; Li et al. 2016). It has been shown that in semi-arid and arid areas, the ratio soil water evaporation/amount of precipitation has the most significant effect (Quade and Cerling 1995; Li et al. 2016).
Palaeo-climatic trends recorded in the Oligo-Miocene sediments
A palaeo-climatic reconstruction of the Oligocene to Miocene sediments from the Valley of Lakes is mainly established on the δ13Ccarbonate profile (Fig. 2). A distinctive, positive δ13C isotope excursion (approximately −7.6 to −5.4‰ of δ13C, VPDB) occurs in the lower Rupelian (~31 Ma, lower to middle Hsanda Gol Fm., 40 to 62 m in Fig. 2), which can be assigned to a distinct early Oligocenearidification in Central Asia, a feature confirmed by the δ18O data. This aridification step has to be differentiated from the well-known Eocene–Olicocene Transition aridification event at ~33 Ma (Meng and McKenna 1998; Dupont-Nivet et al. 2007; Kraatz and Geisler 2010; Abels et al. 2011; Wang et al. 2012; Bosboom et al. 2014; Caves et al. 2014; Li et al. 2016) as it post-dated it clearly. This shift at ~31 Ma correspond to the boundary between Biozone A and B. The mammal assemblage, however, does not show significant changes in diversities or turnover rates (Harzhauser et al. 2016); the communities seem to be stable. Above a prominent sandstone bed at ~59 to 62 m, the δ13C signatures scatter in the range from approximately −5.9 to −4.6‰ of δ13C, VPDB, during the late Rupelian and the early Chattian without any significant variations in the carbon isotopic record. The transition between the biozones B and C is, however, marked by an important turnover in the mammalian community, mainly the rodents (Harzhauser et al. 2016), and corresponds to the OGM. This major climatic event is not well resolved in our record. Another significant shift towards heavier δ13C values (−6.2 to −4.8‰ of δ13C, VPDB, 88 to 93 m in Fig. 2) occurs at the top of the Hsanda Gol Fm., ~24 Ma, between the biozones C1 and C1-D. This trend is seen in the Taatssiin Gol section (TGR-C) and Hsanda Gol section (SHG), but is less clear in the Tatal Gol section (TAT), where the δ13C values scatter around −4.5 ± 0.4‰ already since the base of biozone C. This emphasises the very local response of the paleosols to climatic changes on different settings in the same area. This latter aridification corresponds to the prominent Late Oligocene Extinction (Harzhauser et al. 2016) and to the global Late Oligocene Warming (Paul et al. 2000). During the latest Oligocene to earliest Miocene, the δ13C (and δ18O) values show very strong variation (−10.5 to −4.5‰ of δ13C, VPDB, above 94 m in Fig. 2), which corresponds to an increased presence of cross-bedded fluvial deposits. This coarser lithology could have been more prone to diagenesis and late cement precipitation than the fine sediments of the Hsanda Gol Fm. Alternatively, a more humid climate during the formation of the Loh Fm. is certified by these fluvial sediments and changes in the gastropod record (Neubauer et al. 2013). These strong isotopic fluctuations could therefore reflect cyclic regional-scale climatic variations associated with the end of the global Late Oligocene Warming and the first Miocene Glacial period. The combination of our (isotope) geochemical, mineralogical, sedimentological and petrographic results leads us to suggest that long-term changes in the global and regional climate are partly well recorded in the investigated sedimentary succession of the Valley of Lakes. However, some global events like the OGM are not well documented in our records, and some aridification events (at ~31 and ~24 Ma) do not seem to correspond to any major global climatic change. Ongoing research and novel climate models are now required to better resolve global and regional scale palaeo-climate changes in Central Asia.Variations in the δ18O values of soil carbonate throughout the lower Hsanda Gol Fm. (biozone A, 25 to 40 m in Fig. 2) are very large ( approximately −9.1 to −0.2‰ of δ18O, VPDB). Alternating extremely high to low evaporation degrees can produce such variability in the δ18O values (green squares in Fig. 8). This is in general agreement with the sedimentological data that point to sediment deposition in playas during the early Rupelian (Badamgarav 1993). Up-section, a trend towards heavier δ18O values (approximately −9.5 to −8.0‰ of δ18O, VPDB) was observed in the Rupelian (lower part of biozone B, 40 to 65 m in Fig. 2), which points to a distinct decrease in precipitation. This corresponds to the increase in aridification seen in our δ13C record. The δ13C peak is not seen at the transition between the Tibetan and the Chinese Loess Plateaus (Li et al. 2016). However, an increase in δ18O could be seen in the Lanzhou basin (Li et al. 2016) and in some section of the south Tarim Basin and of the Qaidam Basin (Kent-Corson et al. 2009). This discrepancy could be explained by changes in air-masses circulation, which have only localy an impact on soil productivity. This is followed by a shift towards progressively lighter δ18O data (approximately −8.0 to −9.0‰ of δ18O, VPDB) in the upper Rupelian (the upper part of biozone B). This could indicate an increase in precipitation which is not seen in the δ13C record or another change in air-masses circulation (Kent-Corson et al. 2009). Due to the large scatter in the δ18O values in the range from approximately −7 to −12‰ above ~75 m in the section (Fig. 2), potential palaeo-climatic changes recorded in the Upper Hsanda Gol to Loh fms. are not distinguishable based on δ18O data. This important scattering could be due to either climatic variability or increased diagenetic influences.
Conclusions
Our novel mineralogical and (isotope) geochemical dataset of the highly fossiliferous Valley of Lakes sediments (Mongolia, Central Asia) suggests that intense illitization resulted in a strong overprinting of the mostly fluvial and lacustrine sediments of the Taatsiin Gol basin. The lath-like morphology and the 1 M polytype structure of the illite particles point to precipitation at elevated temperatures (70 to 150 °C), implying that the illitization was the result of circulating hydrothermal fluids generated during post-Oligocene basalt flood event(s). This hydrothermal circulation resulted in a significant post-depositional alteration and in an accompanying all encom-passing homogenization of the mineralogical and major element composition of the entire Eocene to Miocene succession. The trace element composition, i.e. Th/Sc and Zr/Sc ratios, however, reveals a short transportation distance of the sediments and little, if any, reworking-(re)deposition cycles. This confirms that the sediments of the Hsanda Gol to Loh fms. were mainly derived from the alluvial fans that have formed the later Tsaggan Ovoo sediments (Höck et al. 1999). Such short transportation distance and the huge abundance of authigenic illite and I-S contradict the large aeolian origin previously proposed for the fine fraction of the Hsanda Gol sediments (Sun and Windley 2015).The crypto- to microcrystalline, honeycomb-like calcite present in calcrete nodules and lenses within abundant paleosol horizons shows, by contrast, an outstanding resistance against alteration and is therefore suitable to be used for palaeo-climatic reconstructions. In particular, the excursions towards less negative values in the δ13C record of the authigenic soil carbonate reveal a distinct early Oligocene aridification in the Valley of Lakes at ~31 Ma and a less intense (regional-scale) aridification at ~24 Ma that correlates with the Late Oligocene Extinction in mammalian communities. The Oligocene Glacial Maximum, which corresponds to an important faunal turnover in the Valley of Lakes, did not produce any significant imprint in our geochemical record. The Oligocene to Miocene Transition (OMT) is characterised by a higher variability in climate, which corresponds to the Late Oligocene Warming and the first Miocene Glacial. This record, which post-dates the retreat of the Tarim sea and predates the main tectonic up-lift events, confirm that aridification during Oligocene is a general feature for Central Asia (Licht et al. 2016b). These multiple aridification events generally follow global climatic trends; however, regional scale climatic and faunal variation is also recorded in the sediments of the Valley of Lakes.
Authors: Z T Guo; William F Ruddiman; Q Z Hao; H B Wu; Y S Qiao; R X Zhu; S Z Peng; J J Wei; B Y Yuan; T S Liu Journal: Nature Date: 2002-03-14 Impact factor: 49.962
Authors: A Licht; M van Cappelle; H A Abels; J-B Ladant; J Trabucho-Alexandre; C France-Lanord; Y Donnadieu; J Vandenberghe; T Rigaudier; C Lécuyer; D Terry; R Adriaens; A Boura; Z Guo; Aung Naing Soe; J Quade; G Dupont-Nivet; J-J Jaeger Journal: Nature Date: 2014-09-14 Impact factor: 49.962
Authors: Yi Ge Zhang; Mark Pagani; Zhonghui Liu; Steven M Bohaty; Robert Deconto Journal: Philos Trans A Math Phys Eng Sci Date: 2013-09-16 Impact factor: 4.226
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