Geochemistry and sedimentary provenance of the Upper Cretaceous Uberaba Formation ( Southeastern Triângulo Mineiro , MG , Brazil )

Manuscript ID: 20170032. Received in: 01/12/2017. Approved in: 04/26/2017. RESUMO: A Formação Uberaba, de idade campaniana e ocorrência restrita à região da cidade homônima, é composta de arenitos líticos e conglomerados de cor esverdeada, com possível contribuição vulcanoclástica. Nessa unidade ocorrem minerais pesados como ilmenita, granada, perovskita e magnetita, além de clinopiroxênio, plagioclásio, quartzo, calcita e apatita. A Formação Uberaba é marcada geoquimicamente por altos teores em Ba, Ta, La, Nb e Th, com padrões de elementos terras raras normalizados ao condrito fortemente fracionados (LaN/YbN = ca. 128) e planos (sem anomalia de Eu). Análises de química mineral das granadas detríticas da Formação Uberaba indicam predominância de chorlomita com afinidade com granadas crustais (G3). A proveniência sedimentar da Formação Uberaba corresponde a uma mistura de materiais de distritos alcalinos do Alto Paranaíba e derivados da erosão da Formação Serra Geral e dos grupos Canastra e Araxá. Os conglomerados produtores de diamante que ocorrem proximamente, em Romaria, foram considerados por alguns autores como correlatos à Formação Uberaba, porém a composição das granadas retiradas desses conglomerados é bastante diferente, plotando no campo de granadas mantélicas (G9/G10). Descarta-se, dessa forma, correlação entre essas duas unidades, e a Formação Uberaba, portanto, não é uma fonte provável dos diamantes aluvionares encontrados no rio homônimo.


INTRODUCTION
The discovery of alluvial diamonds in the Triângulo Mineiro (TM) and Alto Paranaíba (AP) regions, southeast Brazil, most specifically between the cities of Coromandel and Uberaba, has called the attention of researchers on the source area and sedimentary control of these deposits.The fact that some occurrences are located in alluvial deposits of the Uberaba River (Fig. 1), which occurs in the southern portion of the TM above a specific unit denominated Uberaba Formation, has brought some attention to this unit, as in the works of Hasui (1968), Barbosa et al. (1970), Barcelos (1984), Ferreira Jr. (1996), Ferreira Jr. and Gomes (1999), and Gravina et al. (2002).
The Uberaba Formation, with a mean thickness of 70 m and composed of sandstones and conglomerates, was deposited at ca. 80 Ma ago based on fossiliferous content (Huene 1939).It is stratigraphically the base of the Bauru Group, and its sandstones show a considerable amount of detrital perovskite.Some authors interpret a volcaniclastic origin for at least part of the unit, with further sedimentary reworking (Hasui 1968, Barcelos 1984, Fulfaro & Barcelos 1991, Goldberg 1995).Despite its importance for both the reconstruction of Cretaceous paleoenvironments and potential source for diamond-producing, the Uberaba Formation is one of the least studied units in the context of the Bauru Group.
This paper presents novel data on the Uberaba Formation, emphasizing its geological cartography, petrography, mineral chemistry and geochemical aspects.The main objective is to characterize its provenance and source areas.Besides, in the present paper, we analyze for the first time the potential of the unit as a source for the placer-type alluvial diamond deposits of the area, with respect to the great quantity of alluvial diamonds already recovered in the TM and AP (Campos 1891, Hussak 1891, Hussak 1906, Karfunkel et al. 2014).In this respect, it is interesting that some authors correlate the Uberaba Formation to diamond-producing conglomerates, which crop out 95 km to the northeast, in the Romaria region (Ferreira Jr. 1996, Coelho 2010).The study of heavy minerals recovered from the Uberaba Formation, and their mineral chemistry will help in the definition of the provenance and potential for mineralization of this unit.

Bauru Group and Uberaba Formation
The Bauru Group presents approximately 370,000 km 2 or ca.20% of the Paraná Basin (Barcelos 1984, Fernandes & Coimbra 2000), occurring in the states of Minas Gerais, Goiás, Mato Grosso do Sul, Paraná and São Paulo.This group is limited to the north by the Alto Paranaíba Arch, and corresponds to semi-arid system tract deposits, formed by alluvial fans, ephemeral fluvial systems and an endoreic palustrine zone (Milani et al. 2007).Soares et al. (1980), based on paleontological and stratigraphic studies, suggest that the Bauru Group was deposited in the Aptian-Maastrichtian interval, as also proposed by Bertini (1993).The Uberaba Formation is considered as deposited in the Campanian (83.6 to 72.1 Ma), based on lithostratigraphic relationships with the Vale do Rio do Peixe and Marília formations, in addition to paleontological data (Huene 1939, Santucci & Bertini 2001) and paleomagnetic studies of Tamrat et al. (2002).
The Uberaba Formation belongs to the lower portion of the Bauru Group, in an erosive contact upon the Serra Geral Formation (Fig. 1).This contact is marked by the presence of a polymictic conglomerate with basalt, sandstone and claystone clasts (Hussak 1906).The upper contact with the Marília Formation is considered by some authors as also abrupt, marked by a silexite level and a conglomerate rich in quartz clasts (Seer & Moraes, in press), cimented by calcite (Barbosa 1934, Hasui 1968).Hasui (1968), Barcelos (1984), Goldberg (1995), Ferreira Jr. (1996) and Batezelli (2003) interpret the Uberaba Formation as constituted predominantly by sedimentary rocks with volcaniclastic contribution, mostly coarse sandstones with a local greenish matrix of volcanic origin due presence of Ce oxides, arkoses and lithic sandstones, locally siltstones and mudstones (Fig. 2A), conglomerates and conglomeratic sandstones.Carbonate cementation might occur, as well as carbonate nodules.Macrofossils are common (Santucci & Bertini 2001), as well as bioturbation (Fig. 2B), cross bedding (Fig. 2C), plane-parallel bedding and some syn-depositional deformational structures such as flame structures and convolute fold structures . Ferreira Jr. (1996) andFerreira Jr. andGomes (1999) describe the presence of clay minerals such as detrital illite and authigenic esmectite in the intergranular spaces and suggest their formation from volcanic ashes.On the other hand, Goldberg (1995) proposes a process of mechanic infiltration of fine-grained sediments transported in high stand periods and deposited by decantation over the sand deposits (sieve effect).Silva et al. (1994) suggest that detrital components of the sandstones were sourced of basalts from the Serra Geral Formation, quartzites and schists from the Canastra, Ibiá and Araxá groups, and alkaline rocks from the Alto Paranaíba region.
The depositional setting of the Uberaba Formation is a matter of high debate, and some work hypothesis have been proposed, e.g., fluvial with little transport (Hasui 1968), fluvio-deltaic (Suguio 1980), meandering (Barcelos 1989) and braided (Ferreira Jr. & Guerra 1993, 1995, Batezelli 2003).However, a detailed sedimentological approach is necessary for this issue to be fully understood.
Besides the Uberaba Formation, the Vale do Rio do Peixe and Marília formations compose the Bauru Group in the studied area.The Vale do Rio do Peixe Formation is composed by fine to medium-grained reddish sandstones, with cross-bedded foresets of up to 3 m (Fernandes & Coimbra 2000).The Marília Formation, according to Almeida & Barbosa (1953) corresponds to conglomerates and coarse sandstones with calcite cementation, divided by Barcelos (1984) in three members: Ponte Alta (conglomerate sandstones and conglomerates, calcretes and silcretes), Serra da Galga (polimictic conglomerates with calcrete clasts) and Echaporã (fine to medium-grained sandstones).Other authors as Fernandes and Ribeiro (2015) and Batezelli and Ladeira (2016) consider only two members in this area (Serra da Galga and Ponte Alta).
The stratigraphic subdivision adopted in this paper is according Barcelos (1984) and Batezelli (2003) following the nomenclature of Vale do Rio do Peixe Formation from Fernandes and Coimbra 2000 (Fig. 3).

Diamonds in the Uberaba region
The diamond occurrences of the TM and AP regions are known for more than 250 years and correspond mostly to placer type deposits in the drainage gravels.There are some occurrences in rocks like Romaria's conglomerate and the Capacete Formation of the Mata da Corda Group (Fernandes et al. 2014).Some satellite minerals have been reported on the Uberaba Formation, such as Cr-diopside, picro-ilmenite and pyrope (Gravina et al. 2002).However, diamonds properly have not yet been found in the Uberaba Formation rocks, only within alluvium sediments such as along the Uberaba River.One of the authors (L.C.B.R.) saw a 9 carat diamond at the end of the 70's north of the Uberaba city recovered from gravels of the Uberaba River.According to information from garimpeiros (diggers) a 42 ct diamond has also been recovered from an alluvial deposit.To one of the co-authors (J.K.), several diggers reported the largest recovered stone in the headwaters of the Uberaba River gravel in the 60's ties that weigh 42 ct, and a second one of 34 ct.Karfunkel et al. (2014Karfunkel et al. ( , 2015) ) discuss and put forwards some hypotheses to explain the origin of these gems, from local sources, or transported from long distances by extrusive rocks.Ferreira Jr. (1996) proposes that kimberlitic intrusions were important in providing those minerals.In fact, they could represent some of the sources, but not the main source because up to now no diamondiferous kimberlite or lamproite intrusions were found with a volume that could provide the ca.40 million carats of diamonds already recovered from drains in the TM (Karfunkel et al. 2015).Besides, most kimberlites and related rocks in the TM are of small size, sterile or with non-economic diamond concentrations (Karfunkel et al. 2015).Thus, the provenance of these gems and satellite minerals from kimberlites and lamproites for this region as main suppliers is contentious.

MATERIALS AND METHODS
Fieldwork for data and sample collection was conducted within the context of the Triângulo Mineiro CODEMIG/ UFMG 2015-2017 mapping project, specifically within the context of Veríssimo/Miguelópolis and Uberaba 1:100.000sheets.All of the authors were involved in the fieldwork stage.During the fieldwork, stratigraphic sections were made by L.M., H.S., D.Q. and F.C., with the collection of samples for petrographic, heavy minerals and chemical analyses.
Cartography of the Uberaba Formation was greatly aided by the utilization of aerogeophysical maps, mainly gamma spectrometric maps (U, Th and ternary K-Th-U maps in Fig. 4), from the program Levantamento Aerogeofísico do Estado de Minas Gerais 2010/2011 of CODEMIG, in a 1:500.000scale.Also, scintillometric transects were produced by D.Q. and J.K. (Fig. 1).Those transects were made near the geological contacts between the various units in order to identify possible radiometric variations which could aid in the individualization of the units.A SC-132 hand scintillometer of Mount Sopris Instrument Co. was used for this purpose.
Separation of heavy minerals from selected samples was conducted at the Laboratório de Tratamento de Minérios, CEFET-MG -Campus Araxá.Samples were dried at 300ºC for two hours, then crushed in a jaw crusher, sorted, and then sieved utilizing 70# (210 μm) and 120# (125 μm) sieves.Samples were panned, and then magnetite was removed using a hand magnet.Finally, acid attack with 10% HCl has been carried out for 24 hours in Erlenmeyers.Heavy minerals were then separated by H.S., L.M. and F.V. using a binocular lens.
Twenty-four samples were selected for petrographic analysis, from which five samples were selected for mineral chemistry analysis (samples V634, V620A and B, V631 and 7C).After covering of the polished thin sections with a fine carbon powder, they were subjected to quantitative and semi-quantitative analysis in a JEOL JXA-8900RL (WDS) microprobe at the Centro de Microscopia, Universidade Federal de Minas Gerais, using an acceleration tension of 15 kV and a beam current of 20 nA.Twelve oxides were determined for each analyzed point, and the grades were obtained using Ian Steele and Astimex collection standards.
After crushed and pulverized, 17 samples were sent for whole rock chemistry analysis at GEOSOL Laboratories, Brazil, and two other samples were sent to ACME Analytical Laboratories Ltda., Canada (sample location in Fig. 1).Major element grades were analyzed by ICP-MS (ACME) or ICP-OES (GEOSOL), and trace element grades were analyzed by ICP-MS in both laboratories after fusion with lithium metaborate/tetraborate and digestion with diluted nitric acid.Analytical errors are within 5% for oxides and 10-15% for trace elements.Base and precious metal grades were determined by digestion in Aqua Regia followed by ICP-MS analysis.The Loss On Ignition (LOI) was determined by the weighing difference after ignition at 1,000ºC.

Application of geophysics in the cartography of the Uberaba Formation
In the ternary K-Th-U gamma spectrometric map of the region an E-W trending area in the central portion exhibits high Th and U contents (Fig. 4A), corresponding to the outcrop area of the Uberaba Formation (whiter colors in Fig. 4A).In the Th channel map, the Uberaba Formation is characterized by values above 23,844 ppm (purple and pink shades in Fig. 4B), mainly due to the high perovskite content of the unit.In the U channel map, values above 1,430 ppm (red and pink shades in Fig. 4C) characterize the unit.
Another resource utilized in the mapping of the Uberaba Formation is scintillometric transects (Fig. 5).During the realization of those transects, the Uberaba Formation has shown high radiometric activity, with 250-350 cps (counts per second), while basalts of the Serra Geral Formation show average values around 50 cps and rocks of the Marília Formation around 110 cps.Thus, geophysical data improved considerably the cartography and recognition of the Uberaba Formation outcrop area.For geological mapping in flat lying  Fernandes and Coimbra (2000).rock sequences with different backgrounds in vast regions covered by plantations like sugar cane and soya, this auxiliary method has been of great help.
In a ternary gamma spectrometric map of the eastern TM and AP (Fig. 5), the signature of the Uberaba Formation is comparable to that of the Mata da Corda Group (Guimarães 1964, Bryon 1999, Sgarbi et al. 2003).Both units show high Th and U grades as shown by the bluish colors in the map.

Sedimentological aspects
Three schematic stratigraphic columns were measured for a preliminary study of the Uberaba Formation sedimentary features.For each column, a group of sedimentary facies was described as follows.
In the MP01 column (Fig. 6), located in Randolfo Borges Junior Avenue corner with José Marçal Costa Street (190806 E/ 7815657 N; WGS84 23K), predominantly coarse facies can be recognized, marked by the occurrence of clast-and matrix-supported massive conglomerate, massive sandstone with clasts and medium-grained sandstone followed by a claystone bed.In the middle portion of the column, the sedimentary package is characterized by the presence of erosive surfaces.Above these, clast-rich sandstone and massive conglomerate have been observed, followed by a massive clast-rich sandstone that grades upwards to medium-grained sandstone.The top of the column is marked by conglomerate sandstone and medium-grained sandstone.
The MP02 column (Fig. 7), located in Randolfo Borges Junior Avenue closer to Florestan Fernandes Avenue (189948 E/ 7.816.650N; WGS84 23 K), is characterized from base to top by normal graded facies with conglomerates grading to sandstones.Atop basalts of the Serra Geral Formation, massive matrix-supported conglomerates and sandstones with cross bedding are identified.Above an erosive surface, matrix-supported conglomerate occurs, followed by sandstone with cross bedding and claystone beds.Above a second erosive surface, another layer of clast-supported conglomerate is followed by massive and cross-bedded sandstone.In the top of the sequence, also delimited by a basal erosive surface, matrix-supported conglomerate, massive and clast-rich sandstone occurs.
The base of column FU464 (Fig. 8), located in Leopoldino de Oliveira Avenue corner with José Pimentel Camargo Street (194297 E/ 7813016 N; WGS84 23 K), is marked by a claystone bed followed by a conglomerate sandstone  above an erosive surface, showing decreasing-upwards grain size and grading to medium-grained cross-bedded sandstone.The upper portion of the column is marked by another matrix-supported conglomerate covering an erosive surface.

Petrography
The sandstones of the Uberaba Formation show a mean composition of ca.40% quartz, ca.40% lithic fragments and ca.15% feldspars, characterizing them as lithic sandstones or arkoses.Accessory minerals are olivine, pyroxene, titanite, apatite, phlogopite, garnet, perovskite and opaque minerals, generally up to 5%, but locally, in concentrated laminae, reaching up to 36% of the total rock.
Texturally the sandstones show a predominance of subangulous clasts of medium sphericity, with poor selection and carbonate cementation.The contact between the grains is punctual or normal, suggestive of a loose packing.Some of the detrital grains show chemical alterations in the borders and corrosion gulfs (Fig. 9A and B) in varying sizes, from 0.1 mm to 0.5 mm.
Feldspars are usually altered through sericitization and caulinization processes.Plagioclases are more common, but alkali-feldspars also occur.It is common to identify perovskite and garnet in the heavy mineral levels (Fig. 9F).In some samples, an amorphous, very fine greenish mass of clay minerals  is observed, filling the intergranular voids.This groundmass can reach up to ca. 25% of the total rock volume.

Heavy minerals
Two samples from MP02 site and three samples from MP04 were selected for separation of the heavy minerals.From those samples, magnetite, pyroxene, ilmenite, perovskite, monazite, epidote, rutile, apatite, and diopside were separated (Tab.1).It is noteworthy that for most samples the magnetite concentration is much higher than the other minerals (ca.75%).The main other heavy mineral is perovskite (ca.70% of the clean concentrates), followed by pyroxene with ca.20% and ilmenite around 7%.Other minerals such as monazite, epidote, rutile and apatite show minor contributions or are lacking in some samples.
Analyses of perovskite (Tab.2) were always performed in the nucleus of the grains, due to its small size.The analyzed perovskites are close to the ideal formule (final member CaTiO 3 with ca.29.48% Ca and 35.22%Ti).
Low grades of Na, between 0.04 and 0.62%, suggest low concentration of components such as loparite (NaCeTi 2 O 6 ) and/or lueshite (Na 2 Nb 2 O 6 ).Considerable amounts of Fe, between 0.64 and 1.41%, might be related to solid solution of latrappite (CaNb 0.5 Fe 0.5 O 3 ).Th can reach up to 0.36% (Tab.2), which reflects the characteristic gamma spectrometric responses of the Uberaba Formation (Fig. 4B).U, on the other hand, might be more correlated to celadonite in the rock matrix.
The most common detrital mica of the Uberaba Formation is phlogopite.Chemistry analyses close between 77.23 e 91.25% because of the water preset in their mineral structure, which is not considered during the analyses.The phlogopites show Mg amounts between 11.74 and 16.84%, Fe between 4.32 and 6.64%, Al between 3.97 and 6.678%, and, lastly, Ti between 1.14 and 1.92% (Tab.2).The majority of the phlogopites analyses belong to a solid solution series between tetra-ferriphlogopite and phlogopite.

Whole rock geochemistry
Nineteen samples were analyzed for whole rock geochemistry, and results are shown in Tables 4 and 5.The spatial distribution of those samples within the Uberaba Formation is shown in Fig. 1.Chondrite-normalized (Thompson 1982) incompatible element plots for the Uberaba Formation (Fig. 10A) show a distinctive enrichment in Ta-Nb (positive Ta-Nb anomaly) and also Th enrichment (due to the presence of perovskite).P and Sr show, on the other hand, negative anomalies.North American Shale Composite (NASC)-normalized patterns (Taylor & McLennan 1995) present the same anomalies verified on the chondrite-normalized plots (Fig. 10B and 10C).
In the plots of Figs.11 and 12, besides the samples of the Uberaba Formation, the fields which correspond to the plotting area of the alkaline complexes of the AP (Tapira, Araxá, Catalão I, Serra Negra and Salitre) are also plotted for comparison.In general, samples from the Uberaba Formation plot within the patterns of the AP complexes in Fig. 11, and there is a high overlap between the complexes, generally showing highly fractionated LREE and a positive Nb-Ta anomaly.The patterns which are closer to the Uberaba Formation are those of Tapira and Catalão.Fig. 12A shows a bi-variant plot of SiO 2 × MgO.Those two variables are not correlated, and MgO is constant with higher SiO 2 .In this diagram, some samples plot within the Serra Negra / Salitre and Tapira / Araxá fields, but away from Catalão I.
Figure 12B corresponds to a diagram proposed by Foley et al. (1987), which utilize CaO and Al 2 O 3 grades.The Uberaba Formation samples are characterized by low Ca and high Al 2 O 3 as compared with the alkaline complexes, although the Serra Negra/Salitre complexes plot closer to the samples.Figure 12C correlates the quantities of TiO 2 with SiO 2 .This diagram shows elevated values for the Uberaba Formation, plotting closer to the Serra Negra/Salitre complexes, compared to the other alkaline complexes.The elevated SiO 2 and TiO 2 contents can again be correlated with detrital input from sandstones, quartzites and schists of the basement (SiO 2 ) and alkaline complexes (TiO 2 ).
Unlike major element-based diagrams, a trace-element diagram using the Th/Yb vs. Ta/Yb ratios (Wilson 1989) show a high geochemical affinity of the Uberaba Formation to the AP alkaline complexes, with an enriched-mantle like composition (Fig. 12D).

DISCUSSION
In order to discuss the possible source areas of the Uberaba Formation, we consider here three main distinct sources, two of them included in the nearby basement (Serra Geral Formation and Proterozoic units of the Canastra and Araxá groups), and the third represented by the alkaline-carbonatite complexes of the AP (Fig. 13).Rocks on the AP became exposed and began suffering erosion during the Meso/Neocretaceous with a positive reactivation (Costa 1963, Hasui 1968, Sad 1970).This reactivated high probably provided the detrital contribution during the Cretaceous sedimentation on the northeastern part of the Bauru Basin.
The Mata da Corda Group is another very important unit of the AP (Fig. 13).This group is composed of alkaline volcanics, pyroclastics and epiclastic rocks, with lamproitic, kimberlitic and kamafugitic intrusions and clastic sedimentary rocks.Some minerals which are abundant in the Uberaba Formation are also common in the volcanic rocks of the Mata da Corda Group, such as olivine, clinopyroxene, magnetite, apatite, phlogopite and perovskite (Sgarbi et al. 2003).Freyberg (1934), studying the Capacete Formation of the Mata da Corda Group near Tiros, described a diamantiferous red conglomerate with fine matrix, which Rimann (1917( , in Freyberg 1934) linked to kimberlite-picritic eruptive events and chrono-correlated with the Uberaba Formation.On the other hand, Batezelli and Ladeira (2016) suggest that the Capacete Formation is chrono-correlated with the Marília Formation.The 206 Pb/ 238 U perovskite ages of kamafugites from the Mata da Corda Group generally cluster in the 80-81 and 75-76 Ma age interval (Sgarbi et al. 2003).Thus, the Mata da Corda Group could be a correlative to the Uberaba Formation.This hypothesis needs to be checked by further geochronological studies.We also discuss the probable chrono-correlation of the Uberaba Formation with the diamond-bearing conglomerates of the Romaria region, which outcrops 95 km to the northeast of Uberaba, in isolated channels carved in the basement.The conglomerates of the Romaria region are very important diamond producers, having yielded thousands of carats, including large stones.The company GAR Mineração, Comércio, Importação e Exportação LTDA.explores diamonds in the so-called Tauá conglomerate of Romaria since 2014.Some authors have proposed that this conglomerate is chrono-correlated to the Uberaba Formation, but this hypothesis remains to be proved (Ferreira Jr. 1996, Gravina et al. 2002).
According to Bizzi et al. (1991Bizzi et al. ( , 1993)), alkaline rocks of distinct ages occur in the AP, based on Rb-Sr phlogopite ages: Santonian (117-119 Ma) and Aptian (87-86 Ma).According to Huene (1939), the Uberaba Formation was deposited during the Campanian, ca.80 Ma ago.Thus, this unit is contemporaneous or slightly younger than the alkaline-carbonatitic intrusion of the AP.
The anomalous concentration of clinopyroxene, plagioclase and Ti-bearing minerals in the Uberaba Formation lithic sandstones seems to be related to the erosion of the Serra Geral Formation, while schist and quartzite fragments are mostly related to the erosion of the Canastra and Araxá groups.Indeed an important component of erosion from the nearby basement, without considerable transport and sorting, is suggested by the subangulous clasts with medium sphericity.
The mineral chemistry of the Uberaba Formation detrital garnets and phlogopites are shown in Figs. 14 and 15, and compared with similar minerals in the alkaline complexes (Barbosa 2009, Brod et al. 2013) of the AP, along with mineral chemistry of samples from the Romaria region (Coelho 2010).
Chemical analyses of the detrital garnets of the Uberaba Formation indicate the presence of Ti-rich andradite, which is a common mineral in alkaline rocks (Keep & Russell 1992).This garnet variety is present in the Tapira (Brod 1999, Eberhardt 2014) and Salitre (Barbosa 2009) complexes.Fig. 14A shows a plot of Mg/(Mg+Fe) × Ca/(Ca+Mg) in garnets (Schulze 2003), and the corresponding fields of crustal versus mantellic garnets.Most of the garnets from Romaria show a mantle affiliation, while the Uberaba Formation and alkaline complexes garnets are mainly crustal.Fig. 14B shows a Mg/(Mg+Fe) × Cr 2 O 3 plot (Schulze 2003), in which most garnets of the Romaria conglomerate shows a peridotitic  Studies of garnet chemistry by Dawson and Stephens (1975), Grütter (1998) and Grütter et al. (2004) led to a classification based on the CaO and Cr 2 O 3 contents in 13 groups (G0 to G12) (Fig. 14C).G0 corresponds to garnets of dubious origin.G1 and G2 are brown megacrystals; G3, G4, G5, G6 and G8 are garnets from eclogite xenoliths; G7, G9, G11 and G12 are from lherzolite xenoliths; G10 are garnets from harzburgite and possibly diamond-bearing rocks.In the diagram of Fig. 14C (Grütter et al. 2004), garnets from Romaria are mostly within the G9 (some within the G10) group, i.e., lherzolite-derived.Garnets from the Uberaba Formation and from the alkaline complexes, on the other hand, show significative quantities of Fe, Ca and Mn (ca.1%), and low Cr, localized in the G3 field, from eclogitic xenoliths.
Plotting the mica analysis in a Mg × Fe × Ca diagram (Fig. 15a) makes possible the classification of the phlogopites.The small differences with respect to the phlogopite-annite series are due to the high Ti concentrations (mean 1.48%).A similar situation is observed for the phlogopites of the Tapira (Brod et al. 2001) and Serra Negra (Grasso 2010) complexes (Fig. 15A).In a Fe × Mg plot (Fig. 15B) the samples plot within the alkaline complexes trend.A subordinate substitution of Mg to Fe can be identified in this plot.According to Cordeiro et al. (2010), this substitution occurs in the Catalão I Complex and indicates distinct zoning patterns in the micas of the different rocks of the complex.The compositional variation of the Al 2 O 3 and TiO 2 grades in micas, plotted in Fig. 15C, reflects the high grades of TiO 2 and low Al 2 O 3 , a signature that is similar to the one of the alkaline complexes.
Finally, a Ti × [Fe/(Fe+Mg)] diagram (Fig. 15D) shows the high Ti grades in analyzed phlogopites.This is accompanied by a raise in Fe/(Fe+Mg), a pattern which is very similar to that of phlogopites of the AP alkaline complexes.Boynton (1984) for the following alkaline complexes: Araxá (Traversa et al. 2000) and Tapira (Brod et al. 2013).
Whole rock chemistry analyses of the Uberaba Formation sandstones also suggest a high influence of the alkaline complexes as source areas.This is mainly expressed in the high overall REE concentrations, heavily fractionated LREE, flat REE chondrite-normalized patterns (no Eu anomaly), Ta-Nb positive anomalies, and high Ti and Th concentrations from perovskite, a rare mineral in detrital rocks, but common in alkaline complexes.
The complexes of Serra Negra, Catalão I, Salitre, Araxá and Tapira share all of those characteristics, with high REE concentrations, fractionated LREE, Nb-Ta positive anomalies, etc. (Fig. 11).The smaller complexes, such as Catalão I, Araxá and Tapira, show little variation of the element concentrations resulting in limited fields in the plots (Fig. 11).The larger complexes, such as Serra Negra and Salitre, on the other hand, show a greater variability, leading to broader plotting fields (Fig. 11A and B).
Thus, between the studied complexes, the ones that most closely resemble the geochemical patterns of the Uberaba Formation are those of Catalão I and Tapira (Fig. 11C and D).The main difference is the negative Sr anomaly of the Uberaba Formation, which might be related to the leaching of this element during the carbonatic/dolomitic cementation.On the other hand, enrichment in Ti and Th is related to detrital perovskite.According to Mitchell (1986), garnets are important indicators in the identification of kimberlites and their magma sources.The results obtained for detrital garnets of the Uberaba Formation confirm the presence of andradite garnet, of the schorlomite variety, which is rich in Ti, thus not indicating a kimberlitic source, as suggested by the plotting of the garnets in the eclogitic xenolith field in Fig. 14B.The contrary is observed in Romaria pyrope garnets, which indicate a kimberlitic source.Compared to the diamond-bearing conglomerates of Romaria, the Uberaba Formation provenance and sourcing is quite distinct (Fig. 14C).

CONCLUSIONS
According to the stratigraphic, petrographic, mineral chemistry and whole-rock geochemical data gathered for the Uberaba Formation, three main source areas can be recognized for the provenance of the lithic sandstones and conglomerates of this unit, which probably represents a braided fluvial system: 1. Precambrian rocks of the Araxá and Canastra groups; 2. basalts of the Serra Geral Formation; 3. alkaline rocks of the Catalão I, Catalão II, Serra Negra, Salitre, Tapira, and Araxá cretaceous intrusions and others similar rocks.
All of those units are exposed in the AP Arch, a basement high to the east of the Uberaba Formation outcrop area, which has been active during the Cretaceous.
The chemical composition of the Uberaba Formation rocks, which is very similar to that of the alkaline complexes (highly fractionated REE with La N /Yb N = ca.128; positive Nb-Ta and Ba anomalies), and abundant detrital perovskite, suggests that the third source area was somewhat preponderant over the other two ones.The unit might also involve some syn-sedimentary volcanic or volcanoclastic activity as suggested by a greenish very fine matrix in some samples and fragments of quartz with corroded gulfs.
The chemical analysis of perovskite, garnet and phlogopite confirms that those minerals show similar composition as those ones found in the alkaline complexes of the AP.Garnets of the Uberaba Formation are mainly schorlomite, a Ti-rich variety of andradite, and plot in the field of eclogitic xenoliths (crustal garnets) in discriminatory diagrams.Thus, the unit is not prone to bear detrital diamond grains, as garnets are not indicative of a kimberlitic (mantellic) affiliation.
A chronocorrelation of the Uberaba Formation and the Mata da Corda Group, of around 80-75 Ma (Sgarbi et al. 2003) can be considered for investigation.The diamond-bearing Romaria conglomerate, however, shows a very distinct provenance pattern, bearing pyrope garnets which fall within the kimberlitic field in discriminatory diagrams.Thus, the Uberaba Formation is probably not correlated to the Romaria conglomerate.The geochemical and mineral chemistry features suggest that the Uberaba Formation was not a likely source for alluvial diamonds of the southeastern TM region.Thus, the quest for the source of those diamonds remains open.

Figure 1 .
Figure 1.Integrated simplified geological map of the Veríssimo-Miguelópolis and Uberaba sheets (Ferreira et al. and Seer & Moraes, in press), produced within the Triângulo Mineiro mapping project CODEMIG/UFMG 2015-17.Scintillometric transects A-B and C-D and the location of samples collected for whole-rock geochemistry (red stars) are also shown.

Figure 2 .
Figure 2. Field aspects of rocks from the Uberaba Formation: (A) red fine sandstone bed (below) in contact with green lithic green sandstone (above); (B) bone fossils (probably titanosaur ribs) found in excavation in the Uberaba town; (C) cross stratifications in likely channel deposits.Hammer is 42 cm long.

Figure 5 .
Figure 5. Ternary gamma spectrometric map of the eastern portion of the TM and AP regions, showing the outcrop areas of the Uberaba Formation and Mata da Corda Group (data from the Geophysics Airborne Program of CPRM/CODEMIG, 2006, Area 7).
REE: rare earth element; NASC: North American Shale Composite.Dennis Arthuso Quintão et al.Brazilian Journal of Geology, 47(2): 159-182, June 2017 K Nb Ta La Ce Sr Nd P Sm Zr Hf Ti Tb Y TmYb La Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu 100K Nb Ta La Ce Sr Nd P Sm Zr Hf Ti Tb Y TmYb La Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb those from the Uberaba Formation and alkaline complexes are more like eclogitic garnets.

Figure 15 .
Figure 15.Mineral chemistry binary and ternary diagrams of phlogopites from the Uberaba Formation compared to phlogopites from some alkaline complexes of the AP: (A) Mg × Fe × Ca ternary diagram of micas classification; binary diagrams comparing phlogopites chemistry according to (B) Fe × Mg, (C) Al 2 O 3 × TiO 2 e (D) Ti × [Fe/(Fe+Mg)].

Table 5 .
Whole rock analysis -rare earth element and trace elements (ppm).