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Australia: The Land Where Time Began |
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Ross Ice Shelf Response to Climate Driven by Tectonic Imprint on
Bathymetry of Sea Floor
Over the past 2 decades ice shelves in Antarctica have been thinned by
ocean melting at an increasing rate which has led to a loss of grounded
ice. It is indicated by geological records that the Ross Ice Shelf can
rapidly disintegrate, which would accelerate the loss of grounded ice
from catchments and this could produce equivalent to 11.6 m of global
sea level rise, though the Ice Shelf is currently close to steady state.
For this study data from the ROSETTA-Ice airborne survey and ocean
simulations was used in order to identify the principal threats to the
stability of the Ross Ice Shelf. Tinto et
al. located the tectonic
boundary between East and West Antarctica from magnetic anomalies and
the use of gravity data to generate a new high resolution map of the
bathymetry beneath the ice shelf. Sub-ice shelf circulation is
constrained by the tectonic imprint on the bathymetry, which protects
the grounding line of the ice shelf from moderate changes in the heat
content of the global ocean. In contrast with this, local, seasonal
production of upper ocean warm water near the ice front drives rapid
melting of the ice shelf east of Ross Island, where more rapid loss of
grounded ice would result from thinning of the ice sheets in West as
well as East Antarctica. Tinto et
al. confirm high melt rates in this region by the use of ROSETTA-Ice
radar data. The significance of both the framework and local
ocean-atmosphere exchange processes near the ice front in the
determination of the future of the Antarctic Ice Sheet is highlighted by
these findings.
Though the current contribution to sea level rise by the Antarctic Ice
Sheet is small, it is the largest reservoir of potential global sea
level rise, and it is the component with the greatest acceleration (Nerem
et al., 2018; Shepherd et
al., 2018). Rapid thinning
that is driven by the ocean of small ice shelves that buttress (Dupont &
Alley, 2005) the Amundsen Sea sector of the West Antarctic Ice Sheet
(WAIS) (Pritchard et al.,
2012), coincides with the largest recent losses of grounded ice (Gardner
et al., 2018). The Ross,
Filchner-Ronne and Amery ice shelves are the largest ice shelves, all 3
being in approximately steady state (Rignot et
al., 2013; Depoorter et
al., 2013), though they
buttress grounded ice catchments that contain more than half of the
entire potential Antarctic contribution to global sea level rise, which
highlights a need to understand their stability for future climates that
have been predicted.
The geology, glaciology and climatology of the Ross Embayment control
the stability and structure of the Ross Ice Shelf, which has an area of
~480,000 km2 (Depoorter et
al., 2013). Convergent
tectonics within ancient
Gondwana (500 Ma) and the protracted breakup of
this supercontinent (Dalziel & Lawver, 2001; Veevers, 2012) (190-70 Ma)
were the origin of the regional geology and physiography, which produced
the thinned, subsided lithosphere beneath West Antarctica that at
present is adjacent to the thick lithosphere that supports the
East
Antarctic Ice Sheet (EAIS). Ice from 2 catchments: 1 from the WAIS, that
has 2.0 m of potential sea level rise flowing as broad ice streams, and
1 from the EAIS, that has a potential of 9.6 m of sea level rise that
flows as narrow glaciers through the Transantarctic Mountains, forms the
Ross Ice Shelf that is typically a few hundred m thick. The ice takes
something like 1,000 years to flow from the grounding line to the ice
front. Currently, the ice shelf is stable (Paolo, Fricker & Padman,
2015) though repeated collapse of the ice shelf (Naish et al., 2009) is
documented by geological evidence, as well as large-scale retreat of the
grounding line near the margin of the continent at the
Last Glacial
Maximum (LGM) (Anderson et al., 2014) and more recent substantial
changes in the position of the grounding line and the extent of the ice
shelf during the Later Holocene (Yokoyama et al., 2016).
Mass is lost equally through basal melting and calving from the East
Antarctic side of the Ross Ice Shelf, while on the west Antarctic side
mass loss is dominated by calving (Rignot et
al., 2013). Melt rates that
are derived from satellite are close to zero for much of the shelf,
though near the deep grounding lines of large EAIS glaciers as well as
along the ice front it can exceed 2 m/yr (Rignot et
al., 2013; Paolo, Fricker &
Padman, 2015; Horgan et al.,
2011; Moholdt, Padman & Fricker, 2014). The largest melt rates that have
been observed are about 12 m/yr near the grounding line of Byrd Glacier
(Kenneally & Hughes, 2004), and rates have been measured at 8 m/yr,
though only in summer, close to Ross Island (Stewart et
al., 2019). Delivery of heat
to the base of the ice shelf is controlled by ocean circulation that is
driven by winds over the ocean to the north of the ice front, exchanges
of heat and freshwater at the surface of the ocean and tides (MacAyeal,
1984; Dinniman et al., 2018;
Assmann, Hellmer & Beckmann, 2003).
Included in the ROSETTA-Ice project is a comprehensive airborne survey,
with a line spacing to 10-20 Km, of the Ross Ice Shelf that was
conducted during 2015-2017. The survey was designed to increase the
resolution of seafloor bathymetry for ocean and ice sheet models, as
well as to develop new insights the evolution of ice flow and tectonic
development in the Ross Embayment. Tinto et
al. used the Ice Pod
instrument on a New York National Guard LC-130 aircraft in order to
acquire gravity, magnetic, ice-penetration radar and laser altimetry
data. These measurements, together with new ocean model simulations,
revealed the interconnected systems that control the stability of the
Ross Ice Shelf on timescales that range from months to millennia.
Geological Structure controls bathymetry beneath ice shelves
An abrupt transition in character across a boundary that is oriented
approximately north-south through the centre of the embayment was shown
by magnetic anomalies from the ROSETTA-Ice surveys. The West Antarctic
side is dominated by high-amplitude anomalies and low amplitude
anomalies dominate the East Antarctica side. Immature sedimentary rocks,
magmatic ark materials and extended, thinned continental blocks make up
the crust of West Antarctica (Siddoway, 2008). It is suggested by Tinto
et al. that high amplitude
magnetic anomalies could be due to ark magmatism during convergence of
Gondwana or the exposure along faults during extension of highly
magnetised metamorphic rocks (Luyendyk, Wilson & Siddoway, 2003). The
crust of East Antarctica comprises ancient cratonic and orogenic
material that has magnetic signatures that are highly variable, which
includes a unit of low susceptibility that was identified within the
Transantarctic Mountains (Goodge & Finn, 2010) with characteristics that
are very similar to the East Antarctic side of the Ross Ice Shelf. Tinto
et al. interpret the sharp
boundary in magnetic character beneath the middle of the ice shelf,
rather than the prominent Antarctic Mountains front (Dalziel & Lawver,
2001, as a marker of the position of the boundary between the crust of
East and West Antarctica. There is no obvious boundary in the free air
gravity anomaly map, but the difference in character was revealed in the
density model that was gravity-derived. Tinto et
al. modelled density by
inverting the gravity anomaly at sites of known water depth from Ross
Ice Shelf Geophysical and Glaciological Survey (RIGGS) measurements in
order to show the relative variation in density of a column of rock of
constant thickness across the region. The East Antarctic side, that is
denser, reflects the thinner crust and a greater contribution from dense
mantle material compared to the West Antarctic side. In order to attain
the greater seabed depths that were observed on the East Antarctic side,
the East Antarctic crust that was initially thick must have undergone a
greater amount of extension than the West Antarctic crust. Tinto et
al. suggest the different
extensional histories of the 2 sides probably correspond to different
underlying mantle properties. They interrupt the boundary that was
identified in the middle of the Ross Ice Shelf, and extending to the
margin of the continent, as the major tectonic boundary between East and
West Antarctica.
There is an imprint in the bathymetry beneath the ice shelf of the
tectonic boundary, which was revealed in the new bathymetry map that was
developed by Tinto et al.
through the inversion of the ROSETTA-Ice gravity anomaly field, by use
of the density distribution the RIGGS-constrained model that was
described above. It has been found that the bathymetry beneath the shelf
is typically deeper on the East Antarctic side (670 m mean) and
shallower on the West Antarctic side (560 m mean). It is indicated by
the fact that large-scale asymmetry in bathymetry coincides with the
tectonic boundary, that the asymmetry is a long-term feature that has
persisted throughout multiple glacial cycles. The new bathymetry model
of Tinto et al. resolves the
smaller-scale features that were not present in prior grids, especially
close to the grounding line where the new bathymetry is deeper near the
Kamb Ice Stream and along the grounding line in the EAIS to the south of
Byrd Glacier.
Ocean circulation and basal melting constrained by bathymetry
Tinto et al. ran an ocean
circulation model that incorporated the new bathymetry and an updated
ice draft. The large-scale patterns of circulation that is modelled,
distribution of water mass and melt rate are similar to previous results
(Dinniman et al., 2018;
Assmann, Hellmer & Beckmann, 2003), though we now know better represents
flows into the grounding zones of major outlet glaciers in East
Antarctica. Tinto et al. used
dyes to track the flow and modification of water masses from deep ocean
to the north of the continental margin to the grounding line of the ice
shelf. Antarctic Surface Water (AASW), modified Circumpolar Deep Water
(mCDW), Ice Shelf Water (ISW) and High Salinity Shelf Water (HSSW) (Orsi
& Wiederwohl, 2009) are the principal water masses present along the ice
front. The distributions of these water masses vary on a seasonal basis,
has been reported previously (Assmann, Hellmer & Beckmann, 2003;
Jendersie et al., ?). The
simulation identified the relative importance to ice shelf melting of
CDW, which is part of the global thermohaline circulation, and HSSW,
which is formed locally in polynyas.
Beneath the ice shelf the dominant inflow by volumes is HSSW that flows
beneath the ice front near Ross Island, then moving to the south along
the base of the Transantarctic Mountains. This water is responsible for
high rates of melting at deep grounding lines of major glaciers in EAIS
including the Byrd Glacier, even though HSSW is at the surface freezing
temperature (about -1.9oC),
due to the suppression by pressure of the freezing temperature. Tinto et
al. found that the mixture of
HSSW and ISW does not cross the tectonic boundary because of dynamic
constraints that are imposed by the thinner water column on the West
Antarctic side. Instead, it continues flowing to the north and exits the
ice shelf cavity in the vicinity of Glomar Challenger Trough.
Hayes Bank steers a subsurface layer of mCDW southwards across the
continental shelf to the ice font. It is shown by the simulation of
Tinto et al. that some mCDW
circulation and basal melting beneath the ice shelf to the west of
Roosevelt Island. The penetration of the mCDW is limited, however, to a
region within about 100 km of the ice shelf front. Further to the south,
the WAIS side of the ice shelf is isolated from the source of oceanic
heat and is dominated by a sluggish pool of very cold ISW, and this
leads to negligible rates of melting at that location.
Modelled melt rates that are relatively high along the ice front are
consistent with estimates based on satellite data (Horgan et
al., 2011; Moholdt, Padman &
Fricker, 2014). Rapid melting in summer due to warmer inflows of mCDW
along Hayes Bank, as well as the presence of AASW that has been
seasonally warmed along the ice front, dominate annual-average rates.
The highest seasonal melt rates are located on the EAIS side close to
Ross Island where flows of AASW under the ice shelf are permitted by
thinner ice at the front (Stewart et
al., 2019; Assmann, Hellmer &
Beckmann, 2003; Stern et al.,
2013).
Radar observation of basal melt near the ice shelf front
Tinto et al. used
cross-sections of ice shelf vertical structure from the ROSETTA-Ice
Shallow Ice Radar in order to identify thinning along the flowlines of
East Antarctica, which provided a direct measurement of changing ice
thickness, which was interpreted as basal melt, averaged over timescales
of decades to centuries. The internal boundary between the lower layer
of ice that formed on the continent, and younger ice that formed from
snowfall onto the ice shelf was identified by the radar. Along the
Mulock Glacier flowline the continental ice layer thins by more than 75
m over a distance of 40 km over a period of ~82 years, to reach 0
thickness about 50 km south of the ice front. Based on these
observations, the steady thinning rate for this layer over the last ~80
years is 0.9 m/year. Change in thickness is a combination of basal mass
balance and ice divergence. It is suggested by strain rates calculated
from a satellite-derived ice velocity field (Moholdt, Padman & Fricker,
2014) that in this region compressive flow causes thickening of this
layer of 0.33 m/yr. A basal melt rate of 1.23 m/yr is found by applying
this strain correction to the observed thinning rate, which matches the
1.2 ± 0.2 m/yr basal melt rate that was derived from satellite altimetry
(Moholdt, Padman & Fricker, 2014). It is suggested by the close match
between the method of Tinto et al.
and the satellite altimetry result that the processes that are currently
melting the EAIS ice near Ross Island have persisted throughout the last
century.
Future vulnerability and past ice sheet processes
It is indicated by the results of the study by Tinto et
al. that the asymmetry in the
bathymetry that is controlled by tectonics will prevent melt rates at
the grounding line from changing substantially for future moderate
change in climate, which agrees with Dinniman et
al. (Dinniman et
al., 2018). In this case melt
rates will remain high, though stable, at the deep grounding lines of
EAIS glaciers, as they are controlled by HSSW for which temperature
remains constant (about -1.9oC) and whose circulation is
controlled strongly by bathymetry. Near grounding lines of the WAIS melt
rates will remain low because the large-scale circulation accumulates
very cold meltwater in this region, and the thinness of the cavity on
the West Antarctic side of the tectonic boundary provides a strong
dynamic barrier to incursions of the global ocean heat from the mCDW
inflows.
The primary sensitivity of the mass balance of the Ross Ice Shelf will
be, in the near term, to variations in local climate that change melt
rates near the ice front (Stewart et
al., 2019; Assmann, Hellmer &
Beckmann, 2003; Stern et al.,
2013). Tinto et al. suggest
that changes in frontal melt may be driven by changes in the amount of
mCDW flowing south across the continental shelf along Hayes Bank, and by
variable production of AASW in summer. The mCDW heat flux depends on
large-scale climate processes that determine the rate at which CDW (with
temperature greater than 0OC) is forced onto the continental
shelf and subsequent loss of heat from the mCDW by mixing and convection
of the upper ocean in winter. The production rate and properties of AASW
are influenced strongly by conditions of the local sea ice, influx of
freshwater from the Amundsen Sea (Jacobs & Giulivi, 2010) which
influences heat content and stability of the upper ocean, and the net
atmospheric heat flux (Schneider & Reusch, 2016).
The effect on the stability of ice sheets of changing ice shelf melt
rates depends on the local contribution of the ice to net buttressing of
the grounded ice flow. ‘Passive shelf ice’ comprises most of the ice
front. Any loss of ice from this region will have only a small effect on
the acceleration of grounded ice flow. Contrasting with this, ice shelf
thinning or retreat near Ross Island will reduce the buttressing of
nearby glaciers in EAIS as well as the ice streams of WAIS that are more
distant (Reese et al., 2018).
Tinto et al. proposed that
the grounded ice catchments around Ross Embayment are most vulnerable to
ice shelf loss near the ice shelf front around Ross Island and Minna
Bluff, due specifically to increased duration and intensity of the
production in summer of warm AASW and its subsequent flow beneath the
ice shelf (Stewart et al.,
2019; Dinniman et al., 2018;
Assmann, Hellmer & Beckmann, 2003; Stern et
al., 2013).
The role of climate variations on longer timescales in the
destabilisation of the Ross Ice Shelf of will depended on the position
of the ice front. The grounding line of the ice sheet during the Last
Glacial Maximum (LGM) was near the edge of the continental shelf
(Anderson et al., 2014).
Water masses that were formed locally in this configuration are likely
to have played a lesser role as the globally controlled, CDW that was
relatively warm, could flow into the cavity beneath the ice, thereby
generating high melt rates at the grounding line similar to those that
are observed at present in the Amundsen Sea (Dutrieux et
al., 2014). The ability of
the wind-forced ice-front polynyas, during the subsequent retreat of the
ice sheet, to produce colder HSSW would have been established. The Ross
Ice Shelf system would have shifted to a locally controlled, cold,
sub-ice cavity as the HSSW filled the ice cavity (MacAyeal, 1984). This
switch from global to local controls should have been preserved in the
geological record of former ice shelf extent, including existing
sediment cores (Naish et al.,
2009).
According to Tinto et al. following the Last Glacial Maximum, as the
grounded ice retreated, the ice sheets in East and West Antarctica would
have responded differently to the bathymetry on either side of the
tectonic boundary. To the north of the modern ice shelf, in the Ross
Sea, extensive sediments from the Cainozoic buried the bathymetric
expression of the boundary and so would not have had direct influence on
the retreat of the grounding line across this region. Instead, the
bathymetry of this region has been sculpted by glacial deposition and
erosion (Anderson et al.,
2014). The bathymetry beneath the Ross Ice Shelf of the present reflects
clearly the tectonic boundary. The rapid retreat of the grounding line,
which is inferred on the Eastern Side (Spector et
al., 2017), would have been
aided by the deep bathymetric troughs connected to the Nimrod and Byrd
glaciers. Slower ice sheet retreat will have been experienced by the
shallow West Antarctic side, as it has pinning points such as Roosevelt
Island, Steershead Ice Rise and Crary Ice Rise.
Different boundary conditions are also introduced by the contrasting
properties of the crust across the tectonic boundary, modulating the
flow of grounded ice from East and West Antarctica during prior glacial
epochs. The production and localisation of geothermal heat flux are
controlled by crustal properties as well as influencing the isostatic
response of the lithosphere to ice loading and unloading. A key role is
played by the response to changing ice load in the WAIS grounding line
history around Crary Ice Rise (Kingslake et
al., 2018), which lies on the
boundary between East and West Antarctic crust. As the ice sheets
retreated across different material on either side of the tectonic
boundary they will have produced different isostatic responses.
It has been shown by the results of the survey by Tinto et
al. that the bathymetry and
basal boundary conditions beneath the Ross Ice Shelf have a tectonic
origin which indicates that the contrasting conditions under the WAIS
and EAIS sectors have endured through the entire glacial history of the
Ross embayment. Beneath the Ross Ice Shelf of the present, the shape of
the sub-ice-shelf cavity is controlled by the newly identified tectonic
boundary, which enables circulation that insulates the groundling line
from the influence of global ocean heat. Tinto et
al. have identified that for
the East and West ice sheets in the Ross Sea sector that the greatest
vulnerability is to local, seasonal, upper ocean warming and deepening
of the surface layer at a key region of the ice front, near Ross Island.
The need to incorporate the ice shelf response to local climate
processes in large-scale predictions of ice sheet behaviour in the
broader tectonic framework.
Tinto, K. J., et al. (2019). "Ross Ice Shelf response to climate driven
by the tectonic imprint on seafloor bathymetry." Nature Geoscience
12(6): 441-449. |
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Author: M.H.Monroe Email: admin@austhrutime.com Sources & Further reading |