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Moodies Group

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Journal Article
Published: 01 June 2024
South African Journal of Geology (2024) 127 (2): 141–162.
...H. Stengel; C. Heubeck; M. Homann Abstract Sandy, microbial-mat-laminated sediments are common in estuarine and tidal environments of the Palaeoarchean Moodies Group ( ca. 3.22 Ga); they are interspersed with numerous expressions of mafic to intermediate (sub-) volcanism, including sills, stockwork...
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Journal Article
Published: 01 September 2023
South African Journal of Geology (2023) 126 (3): 235–260.
... preserved in greenstone belts often hinder geological insights. Exceptionally, the largely siliciclastic Palaeoarchaean ( ca. 3.22 Ga) Moodies Group, uppermost unit of the Barberton Greenstone Belt (BGB) in South Africa and Eswatini, allows a detailed understanding of regional depositional processes...
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Journal Article
Published: 01 March 2021
South African Journal of Geology (2021) 124 (1): 253–278.
...S. Reimann; C.E. Heubeck; P. Fugmann; D.J. Janse van Rensburg; A. Zametzer; S.H. Serre; T.B. Thomsen Abstract The ~3.22 Ga Moodies Group, Barberton Greenstone Belt (BGB), South Africa, provides a unique window into Archaean sedimentary, magmatic and ecological processes. In the central BGB...
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Journal Article
Published: 01 June 2019
South African Journal of Geology (2019) 122 (2): 221–236.
... of putative microfossils dating back as far as 3700 Ma have been described, the syngeneity and biogenicity of many occurrences is debated, and some of the proposed fossils have been found to be either contaminants or abiotic artefacts. The ~3200 Ma Moodies Group of the Barberton Greenstone Belt (BGB), South...
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Journal Article
Published: 01 March 2019
South African Journal of Geology (2019) 122 (1): 17–38.
..., and age dating of the Lomati Delta Complex, a morphologically prominent, wedge-shaped and dominantly arenaceous unit in the middle Moodies Group (~3.22 Ga) of the central Barberton Greenstone Belt (BGB). Subvertical regional bedding allows cross-sectional correlation within a prograding delta complex from...
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Series: SEPM Special Publication
Published: 01 January 2012
DOI: 10.2110/sepmsp.101.065
EISBN: 9781565763142
...Introduction Regional Geologyand Depositional Setting of the Moodies Group Fig. 1. Geological sketch map of the Barberton Greenstone Belt (modified after de Ronde and de Wit 1994 ). Moodies Group strata occur in large synclines. The study area is located on the overturned southeastern...
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Journal Article
Journal: Geology
Published: 01 October 2009
Geology (2009) 37 (10): 931–934.
...Christoph Heubeck Abstract Abundant microbial mats from the Mesoarchean Moodies Group (Barberton Greenstone Belt, South Africa, ca. 3.2 Ga) are densely interbedded with coarse-grained and gravelly sandstones in a nearly mud-free setting. They apparently grew in marginal marine and possibly...
FIGURES
Journal Article
Journal: Geology
Published: 01 April 2006
Geology (2006) 34 (4): 253–256.
...Nora Noffke; Kenneth A. Eriksson; Robert M. Hazen; Edward L. Simpson Abstract Newly discovered sedimentary structures produced by ancient microbial mats in Early Archean sandstones of the 3.2 Ga Moodies Group, South Africa, differ fundamentally in appearance and genesis from Early Archean...
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Journal Article
Journal: Geology
Published: 01 December 2001
Geology (2001) 29 (12): 1159.
... the oldest tidal record: The 3.2 Ga Moodies Group, Barberton Greenstone Belt, South Africa : Geology , v. 28 p. 831 – 834 . Kvale , E.P. , Johnson , H.W. , Sonett , C.P. , Archer , A.W. , and Zawistosky , A. , 1999 , Calculating lunar retreat rates using tidal rhythmites : v...
Journal Article
Journal: Geology
Published: 01 September 2000
Geology (2000) 28 (9): 831–834.
...Kenneth A. Eriksson; Edward L. Simpson Abstract The 3.2 Ga Moodies Group in the Barberton Greenstone Belt, South Africa, contains the oldest preserved record of tides. The tidal record is preserved in a tidal sand-wave deposit in the lower Moodies Group as bundles of sandstone foresets separated...
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Published: 01 March 1999
DOI: 10.1130/0-8137-2329-9.259
Image
Representative outcrop photographs of Moodies Group lithologies and sedimentary structures in the central BGB. (A) View from Shokohlwa Mountain northeastward along strike of the southeastern limb of the Saddleback Syncline. All beds dip steeply to the right and young to the left (cp. Figure 4A). They consist of thick- to medium-bedded, in places gravelly and commonly microbially laminated silicified sandstones. (B) Rippled, silicified and FeOx-altered sandstone. The Heights Syncline. (C) Gravelly, cross-bedded, silicified sandstone. Saddleback Syncline. (D) Mudcracked shale coating on bedding plane. Saddleback Syncline.
Published: 01 March 2021
Figure 2. Representative outcrop photographs of Moodies Group lithologies and sedimentary structures in the central BGB. ( A ) View from Shokohlwa Mountain northeastward along strike of the southeastern limb of the Saddleback Syncline. All beds dip steeply to the right and young to the left (cp
Image
Microbially laminated quartzose Moodies Group sandstone in outcrop and thin section, illustrating preservation of fine detail and a lack of compaction. Stratigraphic younging is to the top. (A) to (D) from the Saddleback Syncline (north of the Inyoka Fault zone). (E) is from the The Heights Syncline, (F) is from the Masenjane Homocline, both south of the Inyoka Fault zone. (A) Undulatory, domed, tufted kerogenous mats. Black-chert-filled cavities are interpreted as early-diagenetic gas bubbles formed shortly after surficial sealing (Homann et al., 2016). (B) Microbial mat-chip conglomerate, showing rigid and firm microbial-mat shreds in a shallow and wide tidal channel. (C) Slumped tidal-channel margin, showing tilted, apparently surficially stiffened bed of gravel, sand, and microbial mats in a tilted position. Tidal channel is to the left. (D) Thin-section photomicrograph, showing “floating” fine-grained quartz grains in dark kerogenous matrix (sample 08-848, parallel nicols). (E) Fenestral porosity in horizontally bedded sandstone, with fluid-escape structure; these are observed only in Moodies Group microbially laminated sandstone. Originally carbonate-cemented microbial mats have been leached, resulting in a fenestral porosity. This is a common facies in hydrothermally altered Moodies Group sandstone south of the Inyoka Fault zone. (F) Sawed hand sample (17-142) of microbially laminated sandstone from the Masenjane Homocline, within the region of mafic stockwork dykes. Coin for scale.
Published: 01 March 2021
Figure 3. Microbially laminated quartzose Moodies Group sandstone in outcrop and thin section, illustrating preservation of fine detail and a lack of compaction. Stratigraphic younging is to the top. (A) to (D) from the Saddleback Syncline (north of the Inyoka Fault zone). (E) is from
Image
Schematic relationship of the Lomati River Sill to the Moodies Group (legend as in Figure 4). The hydrothermal halo around the sills preserved microbial mats in Moodies Group sandstones but preservation south of the Inyoka Fault zone was largely compromised by subsequent faulting and stockwork dyke intrusions.
Published: 01 March 2021
Figure 5. Schematic relationship of the Lomati River Sill to the Moodies Group (legend as in Figure 4 ). The hydrothermal halo around the sills preserved microbial mats in Moodies Group sandstones but preservation south of the Inyoka Fault zone was largely compromised by subsequent faulting
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Aspects of sericitic alteration in Moodies Group sandstones in the central BGB. (A) Photomicrograph of highly birefringent pyrophyllitic and sericitic pseudomatrix grain with large muscovite laths, probably resulting from feldspar breakdown (sample SR17-09A, crossed nicols). (B) μ-XRF element maps of a matrix-rich, medium-grained Moodies Group sandstone. Right: Al (magenta), K (orange) represent the sericitic matrix, Si (black) represents quartz. Left: Ti (violet) occurs in rutile and anatase. Fe (red) is represented by hematite and alumohematite. Euhedral Fe domains largely consist of accessory pyrite (sample SR17-09A). (C) Electron-backscatter image of altered grain composed of sericite (white, loc. 2-4) and chlorite (grey, loc. 2-3) within a silica-cement-dominated matrix (sample 15*068). (D) Electron-backscatter image showing heterogeneous FeOx-altered matrix. Monocrystalline quartz and chert (Qz), both light grey, represent the major framework grains. The matrix is dominated by muscovite (Mc), hematite (Hem) and chamosite (Cha, sample SR17-03). (E) Representative Raman spectra and microprobe analyses of sericite (pyrophyllite) and chlorite (chamosite), respectively; locations cp. Figure 11D. First-order polynomial baseline correction was applied to measured Raman spectra to reduce the effect of fluorescence. Both spectra are compared to the reference spectra of RRUFF database (R070728 and R050051).
Published: 01 March 2021
Figure 11. Aspects of sericitic alteration in Moodies Group sandstones in the central BGB. ( A ) Photomicrograph of highly birefringent pyrophyllitic and sericitic pseudomatrix grain with large muscovite laths, probably resulting from feldspar breakdown (sample SR17-09A, crossed nicols). ( B ) μ
Image
Aspects of FeOx-altered Moodies Group sandstone at outcrop scale. (A) and (C) from the Maid-of-the-Mists Syncline, (B) and (D) from the The Heights Syncline. (A) FeOx-altered sandstone boulders crosscut by quartz veins. This rock type weathers to crumbly red soil. (B) Quartz microveins in FeOx-altered sandstone. (C) FeOx veins in silicified sandstone. (D) Liesegang rings in Moodies Group sandstone, common near mafic dykes. Recent weathering creates cavities in which redox reactions with percolating acidic fluids has dissolved carbonate cement. Subrecent botryoidal hematite is common in the cavities.
Published: 01 March 2021
Figure 12. Aspects of FeOx-altered Moodies Group sandstone at outcrop scale. (A) and (C) from the Maid-of-the-Mists Syncline, (B) and (D) from the The Heights Syncline. ( A ) FeOx-altered sandstone boulders crosscut by quartz veins. This rock type weathers to crumbly red soil. ( B ) Quartz
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Field photographs of silicified and fractured Moodies Group sandstone. (A) Densely spaced, randomly oriented fractured and quartz-filled veins are typical in “fractured-facies” sandstone outcrops of MMS. Bedding is largely obliterated. Hammer for scale. (B) Fractured quartz veins cross-cutting conglomerate, midsection of the southern slope of MMS. Hammer for scale. (C) Silicified fractured and brecciated sandstone in outcrop. Angle Station Syncline, ca. 250 m south of Inyoka Fault zone. R40 road is visible in the right middle ground. (D) Closeup of rock surface from the same outcrop. Coin for scale. (E) Fractured sandstone clast of quartz sandstone in quartzose matrix, illustrating early silicification, fracturing, and reworking of some Moodies strata.
Published: 01 March 2021
Figure 16. Field photographs of silicified and fractured Moodies Group sandstone. ( A ) Densely spaced, randomly oriented fractured and quartz-filled veins are typical in “fractured-facies” sandstone outcrops of MMS. Bedding is largely obliterated. Hammer for scale. ( B ) Fractured quartz veins
Image
Diagenetic-sequence diagram of Moodies Group sandstone (from Heubeck, 2019), modified to emphasize alteration processes.
Published: 01 March 2021
Figure 17. Diagenetic-sequence diagram of Moodies Group sandstone (from Heubeck, 2019 ), modified to emphasize alteration processes.
Image
Undeformed polymictic basal conglomerate of the Moodies Group on the southern limb of the Eureka Syncline (2.7 km east of Sheba GM in Sheba Creek), showing a variety of pebble types, including granitoid pebbles (centre of photograph), which were found to range in age between ca. 3460 and 3570 Ma (Kröner and Compston, 1988; Sanchez-Garrido et al., 2011; Kröner et al., 2018). Drillhole (black dot) to the left of top centre has a diameter of 30 mm.
Published: 01 December 2019
Figure 3. Undeformed polymictic basal conglomerate of the Moodies Group on the southern limb of the Eureka Syncline (2.7 km east of Sheba GM in Sheba Creek), showing a variety of pebble types, including granitoid pebbles (centre of photograph), which were found to range in age between ca. 3460
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(A) Deformed conglomerate in the Moodies Group and (B) flattened volcaniclastic fragments in the Schoongezicht Formation (Fig Tree Group) underlying the Moodies basal conglomerate in the Ezzy’s Pass road cutting on the northern rim of the Eureka Syncline. The long axes of the pebbles and volcaniclastic fragments plunge subvertically. (C) Tight folds resulting from intense flattening of Fig Tree Group ferruginous shales, cherts and greywackes in the Lily GM. All examples shown are directly south of the Lily West Syncline (Figure 12) which formed during an early D2 deformation event. The deformed rocks shown are all related to flattening caused by the intrusion of the Stentor Pluton. (width of photographs A, B, C, ca. 70 cm).
Published: 01 December 2019
Figure 10. ( A ) Deformed conglomerate in the Moodies Group and ( B ) flattened volcaniclastic fragments in the Schoongezicht Formation (Fig Tree Group) underlying the Moodies basal conglomerate in the Ezzy’s Pass road cutting on the northern rim of the Eureka Syncline. The long axes