2015
DOI: 10.1016/j.epsl.2015.03.008
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Records of geomagnetism, climate, and tectonics across a Paleoarchean erosion surface

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Cited by 8 publications
(4 citation statements)
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“…This diverse substrate chemically resembled continental crust and was at least microcontinental in scale. Indeed, if the Vaalbara hypothesis of Kaapvaal-Pilbara cratonic aggregation (Button, 1979;Cheney, 1996) can be extended back to the Paleoarchean (Bradley et al, 2015), then the basement to the Lalla Rookh Sandstone was already truly continental, providing a comparatively cool, buoyant and stable terrestrial platform. The Lalla Rookh Sandstone itself has only been metamorphosed to sub-greenschist facies, as the immediately overlying terrestrial basalts and sediments of the ~2.77 Ga lower Fortescue Group are of prehnite-pumpellyite grade (Smith et al, 1982) and the Lalla Rookh mudrocks themselves are composed of illite and chlorite (Buick et al, 1998).…”
Section: Geologic Settingmentioning
confidence: 99%
“…This diverse substrate chemically resembled continental crust and was at least microcontinental in scale. Indeed, if the Vaalbara hypothesis of Kaapvaal-Pilbara cratonic aggregation (Button, 1979;Cheney, 1996) can be extended back to the Paleoarchean (Bradley et al, 2015), then the basement to the Lalla Rookh Sandstone was already truly continental, providing a comparatively cool, buoyant and stable terrestrial platform. The Lalla Rookh Sandstone itself has only been metamorphosed to sub-greenschist facies, as the immediately overlying terrestrial basalts and sediments of the ~2.77 Ga lower Fortescue Group are of prehnite-pumpellyite grade (Smith et al, 1982) and the Lalla Rookh mudrocks themselves are composed of illite and chlorite (Buick et al, 1998).…”
Section: Geologic Settingmentioning
confidence: 99%
“…Together with paleolatitudes from other poles previously reported from the East Pilbara, the new HEBh pole places new lower bounds on the horizontal drift rate of the East Pilbara between ~3.35 and 2.77 Ga relative to Earth's rotation axis, assuming a geocentric axial dipole field geometry at ~3.2 Ga. The youngest pre-HEBh pole from the East Pilbara is that of the 3350-to 3335-Ma Euro Basalt (EBm), which provides an estimated paleolatitude of 8.09° ± 5.3° (49). This paleolatitude is distinguishable from that of the HEB at 2 and requires that the average latitudinal velocity of the Pilbara exceeded 0.23° ± 0.10°/Ma or ≥2.50 ± 1.15 cm/year between 3.35 and 3.18 Ga (Fig.…”
Section: Tests For Archean Plate Motionmentioning
confidence: 99%
“…These rotations may originate from platetectonic motion of the East Pilbara Craton, true polar wander (TPW), or post-emplacement local block rotations, perhaps during ~2950-to 2930-Ma deformation in the Lalla Rookh-Western Shaw Structural Corridor (LWSC) that sinistrally sheared the majority of the SVS and ESGB (29,30). The region in which the EBm pole was measured (49) would not have rotated substantially during this episode (29,30). Local effects related to the impingement of the nearby Shaw, Yule, and Strelley batholiths apparently both produced the SVS and rotated its central portion CW (29,30), thus potentially accounting for some of the observed EBm-HEBh rotation.…”
Section: Tests For Archean Plate Motionmentioning
confidence: 99%
“…The East Pilbara Craton of Western Australia ( Fig. 1 A ) hosts the most complete pre-2.8 Ga paleomagnetic record ( SI Appendix , Appendix S2 ), with robust paleomagnetic poles at 3.47 Ga [“DFM” ( 5 )], 3.34 Ga [“EBm” ( 6 )], and 3.18 Ga [“HEBh” ( 4 )]. Due to the slow minimum drift rate and the possibility of true polar wander (TPW), it is uncertain whether mobile- or stagnant-lid processes drove a major latitudinal shift between poles EBm and HEBh ( 4 ).…”
mentioning
confidence: 99%