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SCAR Report No 16
Appendix 7
THE LATE MESOZOIC AND CENOZOIC PLATE TECTONIC AND CRUSTAL HISTORY OF ANTARCTICA:
IMPLICATIONS FOR MARINE AND TERRESTRIAL SEQUENCES
D.H. Elliot, Byrd Polar Research Center and Department of Geological Sciences,
Ohio State University
Much of the Late Mesozoic and Cenozoic geologic history
of Antarctica is contained in the sedimentary sequences on the continental shelves.
That history, however,
in large measure reflects the evolution of the Antarctic Plate, both its
plate tectonic and its crustal development.
The Antarctic Plate was created by the break-up of Gondwanaland and today, except
for the Scotia Sea region, is bounded by spreading ridges. The Antarctic
continental shelves rimming the East Antarctic craton are passive margins resulting
from
the separation of southeastern Africa, India and Australia. The remaining
part of the continent has a complex history which includes fragmentation into
microcontinents
or blocks, rotations and displacements of those blocks, and subduction and
passive margin evolution.
In general, the post-breakup history can be divided into: the mid Jurassic
to mid Cretaceous, by which time the Antarctic continent had attained its
present configuration and polar location (Grunow et al., 1991); and the mid
Cretaceous
(100 Ma) to Recent. During the latter time interval break-up between Antarctica
and Australia/New Zealand occurred, the link between South America and the
Antarctic
Peninsula was broken, and events leading up to the present day rift system
through West Antarctica took place.
The mid Cretaceous (100 Ma.) setting
During the 75 m.y. between Mid Jurassic
break-up and the mid Cretaceous, Africa and India separated from Antarctica,
and South America from Africa;
in addition,
rifting had begun between Australia and Antarctica but no oceanic crust had
formed. The Antarctic rim of the Gondwana Plate was an active convergent
margin throughout
most of this interval, although in the backarc region there was extension
associated first with break-up and emplacement of the Ferrar tholeiites and
second following
New Zealand/Pacific-Phoenix Ridge collision in mid Cretaceous time.
Regions rifted during Middle Jurassic break-up were of longstanding by 100
Ma, and included the Weddell Embayment, Pensacola Basin, Lambert Graben,
and probably
the Jutulstraumen embayment and Lützow-Holm Bay region; other rifts may
well be present. These rifts were likely the sites of epicontinental seaways
into the interior of Antarctica. Marine incursions may well have occurred
in other locations as well.
Initial disruption of the Gondwana Plate margin was probably accompanied
by local crustal thinning, and hence seaways may have been established through
the Ross-Weddell
embayment region and connected to the Panthallasan Ocean. Fission track data,
however, suggest significant Early Cretaceous (ca. 141-117 Ma) uplift of
the Ellsworth Mountains (Fitzgerald and Stump, 1991), possibly as a result
of "docking" against
southern Palmer Land, thus blocking any major shallow passages in this region.
Uplift of the southern Transantarctic Mountains started at about 125 Ma (Fitzgerald
and Stump, 1997), but must have had a different cause. Initial extension
in the Ross Embayment-Campbell Plateau region, with accompanying development
of the
Ross Sea sedimentary basins, and uplift were doubtless linked (Lawver et
al., 1994). The underlying driving force for all the Ross Embayment events
was probably
related to extension in the backarc region of the active plate margin.
Plate tectonic events of the last 100 m.y.
Plate tectonic events of the last 100
m.y. brought about the physical isolation of the Antarctic continent. Arguably
this is one of earth's most important
events in that it precipitated conditions leading to the inception and evolution
of
Cenozoic glaciation.
The fragmentation of East Gondwanaland was initiated with the development
of the Pacific-Antarctic Ridge between Campbell Plateau and West Antarctica,
at
about 85-90 Ma. (Cristoffel and Falconer, 1972; Cande et al., 1982) and the
SE Indian Ocean-Antarctic Ridge between Australia and East Antarctica, at
about 90 Ma (Cande and Mutter, 1982). The boundary connecting those two is
complex and also involves the opening of the Tasman Sea at the same time
(Weissel and
Hayes, 1977). Pacific-Antarctic spreading involved a dextral component of
motion whereas the initial opening between Australia and Antarctica was more
orthogonal
but very slow until the mid Eocene (C20 time) when there was a significant
increase in rate (Cande and Mutter, 1982). Transform fractures linked the
two
principal
ridges but complete crustal separation did not occur until the Late Oligocene
when the South Tasman Rise finally cleared north Victoria Land.
The other Gondwanaland link, that with South America, was finally broken
at about 29 Ma with the formation of ocean floor in Drake Passage (anomaly
C10). Shallow
water connections may have existed earlier although deepwater circulation
was not possible till about 23 Ma when the South American continental crust
cleared
Peninsula crust at the Shackleton FZ (Barker and Burrell, 1977).
Continental crustal events of the last 100 m.y.
Except for the Antarctic Peninsula, the continent
has been rimmed by passive margins for the last 100 m.y. Those from the head
of the Weddell Sea round
to about 90EE are progressively younger, from Middle Jurassic to Early Cretaceous;
the Australia-Antarctica sector dates from mid Cretaceous time, and the rest
from the Late Cretaceous. All presumably have been subsiding at normal rates.
The Antarctic Peninsula remained a convergent margin, where the Phoenix Plate
was subducted, until Miocene time (Larter and Barker, 1991); since then the
principal
crustal motions there have been vertical.
In the rest of the continent, uplift and subsidence, together with extension
and associated volcanism, have dominated crustal events. Uplift in the Lambert
Graben region is thought to have occurred in Miocene to Recent time (Wellman
and Tingey, 1982; McKelvey et al., 1995). The present elevation of the East
Antarctic craton in the Queen Maud Land-Enderby Land sector may reflect the
same episode
of uplift. The Lambert Graben contains a number of small highly alkaline
intrusive and extrusive bodies (Sheraton, 1983), suggesting the extensional
regime is of
longstanding and is probably still active. The sub-glacial Gamburtsev Mountains
are possibly a major alkaline volcanic field related to the Lambert Graben
(Elliot, 1994).
Uplift in the Ellsworth Mountains in the late Cretaceous and Cenozoic was
limited (Fitzgerald and Stump, 1991). Nevertheless, the magnitude of the
rifts between
those mountains and the base of the Antarctic Peninsula suggests more recent
continental block readjustments.
Episodic uplift is inferred from fission track data for the Transantarctic
Mountains (Fitzgerald, 1992, 1994; Fitzgerald and Gleadow, 1988; Fitzgerald
and Stump,
1997). The two principal episodes are Late Cretaceous and Eocene, the latter
being the best documented and most widespread. Fission track data provide
only a date on the inception of more rapid denudation and do not yield information
on its termination. Thus the fission track data do not constrain the denudation/uplift
history during the Late Cenozoic, except that in the lower Beardmore Glacier
region there appears to have been as much as 4 km of denudation in the last
30
m.y. (Fitzgerald, 1994).
Episodic uplift is also inferred for Marie Byrd Land (Richard et al., 1994),
with initial denudation at 100-94 Ma and a later event at about 80-70 Ma.
Subsequent tectonic quiescence allowed the formation of a regional erosion
surface in Marie
Byrd Land, interpreted to be correlative with a similar surface in New Zealand
and offshore on the Campbell Plateau and given a Late Cretaceous (75 Ma)
age (LeMasurier and Landis, 1996). In Marie Byrd Land the surface is found
at elevations
up to 2,700 m. The cause of the uplift is thought to be a Late Cenozoic (<30
Ma) mantle plume which lead to eruption of the alkaline volcanic rocks of
Marie Byrd Land.
The principal region of active extension in the last 100 m.y. is West Antarctica.
The regionally thin crust (20-30 km) of the Ross Embayment was most likely
formed following the mid Cretaceous Pacific-Phoenix ridge-crest collision
with the trench
off New Zealand and the Campbell Plateau (Bradshaw, 1989). Initial development
of the elongate basins located on the shelf and extending beneath the Ross
Ice Shelf occurred at this time. An extensional regime is also suggested
by 100-105
Ma anorogenic granites in Marie Byrd Land (Weaver at al., 1994). This episode
of extension, basin formation, and basin filling was terminated by rifting
between Marie Byrd Land and Campbell Plateau. The Eocene changes in plate
motions and
the major episode of denudation in the Transantarctic Mountains may correlate
with formation of the Ross Sea regional unconformity U6 (Davey and Brancolini,
1995). Late Cenozoic extension appears to be confined to the Terror Rift
in south Victoria Land but contemporaneous alkaline volcanism is widespread
in the Transantarctic
Mountains and West Antarctica.
The age of the inferred rift basins in central West Antarctica - Byrd Subglacial
Basin and the Bentley Subglacial Trench - is unclear but their development
may also have a significant Late Cenozoic component. Magnetic data for the
whole region have been interpreted to suggest the presence of a major subglacial
flood
basalt province of Late Cenozoic age (Behrendt et al., 1994).
The remaining region of possible crustal extension lies in Wilkes Land (about
90E-160EE) and includes the Wilkes Sub-glacial Basin, with its continuation
into the Pensacola Basin, the Aurora Basin, and the graben-like setting of
Lake Vostok
and other narrow troughs. The Wilkes and Aurora Sub-glacial Basins may be
the counterpart of the Cretaceous depression in Australia (Veevers, 1982).
The Wilkes
Basin may have been reactivated during the Cenozoic on uplift of the Transantarctic
Mountains. The Wilkes-Pensacola Basin contains at least scattered evidence
for marine incursions, as indicated by the reworked floras and faunas in
the Sirius
Group deposits.
Implications Of The Plate Tectonic And Crustal History
Antarctica's role in biotic evolution and dispersal.
Paleobiogeography: Antarctica is central to
the issue of migration of vertebrates to Australia. Should reptiles, including
dinosaurs, of Triassic through Early
Cretaceous age be found in Australia, land bridges must have been maintained
across Antarctica. With the inferred rifting and marine incursions in the
Ross Embayment, the Ellsworth Mountains would have been a critical stepping
stone
between the Antarctic Peninsula and the Transantarctic Mountains. Marsupial
migration (Woodburne and Case, 1996) occurred after the start of Tasman Sea
opening and
prior to about 64 Ma by which time the South Tasman Rise was submerged, although
the submerged Rise did not clear Antarctica till about 30 Ma; similarly,
the land connections must have included the Ellsworth Mountains.
The physical isolation and polar position of Antarctica are crucial factors
in evolution of the present marine biota. The presence or absence of shallow-water
paths across the Antarctic continent would have played an important role
in dispersal
and endemism.
Significant questions include: What were the the timing, duration, and elevations
of the stepping stones that constituted the land bridges? Where will records
of vertebrate dispersal be found and in what sort of sequences? Are there
remnants of pre-glacial sedimentary sequences along the flanks or on the
shoulders of
outlet valleys of the Transantarctic Mountains? How did the evolving shallow
and deep seaways influence the evolution of marine biota?
Climate history
Oceanic circulation: The reorganization of oceanic circulation to a thermo-haline driven system occurred during the Cenozoic. Today it is governed by processes occurring around Antarctica. The evolution to a thermo-haline driven system is not well documented but presumably is related to the development of the circumantarctic currents and the upwelling that is a consequence of the ice sheets.
Significant questions include: when was present day thermo-haline circulation initiated? What is the relationship between the evolving shallow and deep-water passages and the development of that circulation?
Glacial history: Glacial onset occurred in the Paleogene. Eocene (>49.5 Ma) glaciation has been reported from King George Island in the South Shetland Islands (Birkenmajer, 1991), but such early glaciation is in conflict with most paleoclimatic data (see Elliot, 1997); based on Sr isotope data, that glaciation is possibly Late Oligocene (Dingle and Lavalle, 1998). Kerguelen Plateau and Maud Rise data have been interpreted to suggest glacial conditions at about 46 Ma (Ehrmann and Mackensen, 1992), however the reported Eocene IRD is now thought to be downhole contamination (S. Wise, this workshop report). In the Ross Embayment, striated clasts in drill core (Hambrey and Barrett, 1993) suggest nearby glaciation in early late Eocene time (Wilson et al., 1998), but there remains the question of whether it reflects mountain glaciation rather than continent-wide ice sheets. Evidence for initiation of substantial ice sheets comes from Prydz Bay and suggests ice down to sea level by Eocene-Oligocene time (Barron et al., 1991; Hambrey et al., 1991). By Late Oligocene time ice-sheet glaciation was widespread and in the Miocene the marine ice-sheets of West Antarctica were first formed. The marine record suggests there have been major fluctuations since then.
The older terrestrial record of glaciation comes from King George Island off the Antarctic Peninsula where the only well documented sequences indicate glaciation (Polonez and Melville glaciations) in Early Miocene time (Smellie et al, 1998). The record from West Antarctica is no older than about 10 Ma. In East Antarctica the antiquity and subsequent fluctuations of glaciation is a matter of on-going debate (see GSA Today, 1998).
Significant questions include: when did ice sheets evolve from wet-based to the present day cold-based condition? To what extent have there been fluctuations in that aspect of the ice-sheets? What role has Cenozoic uplift played in the initiation of ice sheets and in the change to cold-based conditions? Can the timing of uplift, and its duration and amount, be better constrained for the various now-uplifted crustal blocks in and around the margin of the continent?
Key Issues
The timing and kinematics of tectonic events is critical for understanding cause and effect relationships. Paleo-oceanographic history is dependent on knowing the onset and duration of shallow and deepwater circulation patterns, which themselves are dependent on the tectonic history. The uplift and subsidence of crustal blocks, together with crustal extension, control the nature, extent and infilling of sedimentary basins. These vertical movements likewise exerted a major control on the location of centers for glaciation which affected at least regional climate. The patterns of biotic evolution in the South Polar region are similarly dependent on tectonic, glacial and paleo-oceanographic events.
Summary
In broad outline, the significant mid Cretaceous to Recent tectonic
events were:
- vertical movements of crustal blocks, starting in the Early Cretaceous that created stepping stones for faunal and floral dispersal but barriers to surface water flow, and which also influenced sedimentary basin development and infilling,
- Late Cretaceous fragmentation of East Gondwanaland, marked by major sedimentary basin development in the Ross Sea-Campbell Plateau region, and in Wilkes Land,
- development of deepwater circumpolar circulation as first the South Tasman Rise cleared north Victoria Land and then the Drake Passage opened,
- physical isolation and vertical tectonism with associated glaciation.
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