Otavi Group is a 1.5−3.5-km-thick epicontinental marine carbonate succession of
Neoproterozoic age, exposed in an 800-km-long Ediacaran−Cambrian fold belt that rims
the SW cape of Congo craton in northern Namibia. Along its southern margin, a contiguous
distally tapered foreslope carbonate wedge of the same age is called Swakop Group.
Swakop Group also occurs on the western cratonic margin, where a crustal-scale thrust
cuts out the facies transition to the platformal Otavi Group.
Subsidence accommodating Otavi Group resulted from S−N crustal stretching (770−655
Ma), followed by post-rift thermal subsidence (655−600 Ma). Rifting under southern
Swakop Group continued until 650−635 Ma, culminating with breakup and a S-facing
continental margin. No hint of a western margin is evident in Otavi Group, suggesting a
transform margin to the west, kinematically consistent with S−N plate divergence. Rift related
peralkaline igneous activity in southern Swakop Group occurred around 760 and
746 Ma, with several rift-related igneous centres undated. By comparison, western Swakop
Group is impoverished in rift-related igneous rocks.
Despite low paleoelevation and paleolatitude, Otavi and Swakop groups are everywhere
imprinted by early and late Cryogenian glaciations, enabling unequivocal stratigraphic
division into five epochs (period divisions): (1) non-glacial late Tonian, 770−717 Ma; (2)
glacial early Cryogenian/Sturtian, 717−661 Ma; (3) non-glacial middle Cryogenian,
661−646±5 Ma; (4) glacial late Cryogenian/Marinoan, 646±5−635 Ma; and (5) non-glacial
early Ediacaran, 635−600±5 Ma. Odd numbered epochs lack evident glacioeustatic
fluctuation; even numbered ones were the Sturtian and Marinoan snowball Earths. This
study aimed to deconstruct the carbonate succession for insights on the nature of
Cryogenian glaciations. It focuses on the well-exposed southwestern apex of the arcuate
fold belt, incorporating 585 measured sections (totaling >190 km of strata) and >8,764
pairs of δ13C/δ18Ocarb analyses (tabulated in Supplementary On-line Information).
Each glaciation began and ended abruptly, and each was followed by anomalously thick
‘catch-up’ depositional sequences that filled accommodation space created by synglacial
tectonic subsidence accompanied by very low average rates of sediment accumulation. Net
subsidence was 38% larger on average for the younger glaciation, despite its 3.5−9.3-times
shorter duration. Average accumulation rates were subequal, 4.0 vs 3.3−8.8 m Myr−1,
despite syn-rift tectonics and topography during Sturtian glaciation, versus passive-margin
subsidence during Marinoan. Sturtian deposits everywhere overlie an erosional
disconformity or unconformity, with depocenters ≤1.6 km thick localized in subglacial rift
basins, glacially carved bedrock troughs and moraine-like buildups. Sturtian deposits are
dominated by massive diamictite, and the associated fine-grained laminated sediments
appear to be local subglacial meltwater deposits, including a deep subglacial rift basin. No
marine ice-grounding line is required in the 110 Sturtian measured sections in our survey.
In contrast, the newly-opened southern foreslope was occupied by a Marinoan marine
ice grounding zone, which became the dominant repository for glacial debris eroded from
the upper foreslope and broad shallow troughs on the Otavi Group platform, which was
glaciated but left nearly devoid of glacial deposits. On the distal foreslope, a distinct
glacioeustatic falling-stand carbonate wedge is truncated upslope by a glacial
disconformity that underlies the main lowstand grounding-zone wedge, which includes a
proximal 0.60-km-high grounding-line moraine. Marinoan deposits are recessional overall,
since all but the most distal overlie a glacial disconformity. The Marinoan glacial record is
that of an early ice maximum and subsequent slow recession and aggradation, due to
tectonic subsidence. Terminal deglaciation is recorded by a ferruginous drape of stratified
diamictite, choked with ice-rafted debris, abruptly followed by a syndeglacial-postglacial
cap-carbonate depositional sequence. Unlike its Sturtian counterpart, the post-Marinoan
sequence has a well-developed basal transgressive (i.e., deepening-upward) cap dolomite
(16.9 m regional average thickness, n=140) with idiosyncratic sedimentary features
including sheet-crack marine cements, tubestone stromatolites and giant wave ripples. The
overlying deeper-water calci-rhythmite includes crystal-fans of former aragonite benthic
cement ≤90 m thick, localized in areas of steep sea-floor topography. Marinoan sequence
stratigraphy is laid out over ≥0.6 km of paleobathymetric relief.
Late Tonian shallow-neritic δ13Ccarb records were obtained from the 0.4-km-thick
Devede Fm (~770−760 Ma) in Otavi Group and the 0.7-km-thick Ugab Subgroup
(~737−717 Ma) in Swakop Group. Devede Fm is isotopically heavy, +4−8‰ VPDB, and
could be correlative with Backlundtoppen Fm (NE Svalbard). Ugab Subgroup post-dates
746 Ma volcanics and shows two negative excursions bridged by heavy δ13C values. The
negative excursions could be correlative with Russøya and Garvellach CIEs (carbon isotope
excursions) in NE Laurentia.
Middle Cryogenian neritic δ13C records from Otavi Group inner platform feature two
heavy plateaus bracketed by three negative excursions, correlated with Twitya (NW
Canada), Taishir (Mongolia) and Trezona (South Australia) CIEs. The same pattern is
observed in carbonate turbidites in distal Swakop Group, with the sub-Marinoan falling stand
wedge hosting the Trezona CIE recovery. Proximal Swakop Group strata equivalent
to Taishir CIE and its subsequent heavy plateau are shifted bidirectionally to uniform
values of +3.0−3.5‰.
Early Ediacaran neritic δ13C records from Otavi Group inner platform display a deep
negative excursion associated with the post-Marinoan depositional sequence and heavy
values (≤+11‰) with extreme point-to-point variability (≤10‰) in the youngest Otavi
Group formation. Distal Swakop Group mimics older parts of the early Ediacaran inner
platform δ13C records, but after the post-Marinoan negative excursion, proximal Swakop
Group values are shifted bidirectionally to +0.9±1.5‰. Destruction of positive and negative
CIEs in proximal Swakop Group is tentatively attributed to early seawater-buffered
diagenesis (dolomitization), driven by geothermal porewater convection that sucks
seawater into the proximal foreslope of the platform. This hypothesis provocatively implies
that CIEs originating in epi-platform waters and shed far downslope as turbidites are
decoupled from open-ocean DIC (dissolved inorganic carbon), which is recorded by the
altered proximal Swakop Group values closer to DIC of modern seawater.
Carbonate sedimentation ended when the cratonic margins collided with and were
overridden by the Atlantic coast-normal Northern Damara and coast-parallel Kaoko
orogens at 0.60−0.58 Ga. A forebulge disconformity separates Otavi/Swakop Group from
overlying foredeep clastics. In the cratonic cusp, where the orogens meet at a right angle,
the forebulge disconformity has an astounding ≥1.85 km of megakarstic relief, and kmthick
mass slides were displaced gravitationally toward both trenches, prior to orogenic
shortening responsible for the craton-rimming fold belt.