There is intense scientific interest in the history, dynamics and future
of the West Antarctic Ice Sheet because it is the world's only remaining
marine ice sheet and is considered by many to be inherently unstable and
prone to catastrophic collapse and melting (e.g. Hollin, 1962; Hughes,
1973; Mercer, 1978; MacAyeal, 1992; Binschadler, 1995). If the WAIS
were to collapse, global sea level would rise by 6 meters. The stability
of the WAIS is a function of some balance between external sea level and
climate and internal controls of marine ice-sheet and ice-stream dynamics
(Alley and Whillans, 1991; MacAyeal, 1992; Bentley, 1997). Ultimately,
accurate predictions of future ice-sheet stability and behavior will require
numerical models, based on an understanding of the physical dynamics of
the present ice sheet and tested by geological constraints on past ice-sheet
configurations.
One approach to providing geological constraints on the age of the West
Antarctic Ice Sheet is through direct dating and geochemical correlation
of englacial tephra layers within the ice sheet. The stratigraphy
and morphology of many West Antarctic englacial tephra layers suggests
that the layers were deposited on snow at the time of the volcanic eruption,
and were incorporated into the ice with little reworking or mixing,
indicating that the age of the tephra layer is truly representative of
the age of the surrounding ice.
Several West Antarctic englacial tephra site exist. Mt.
Waesche is located at between 1900-2000 meters elevation in a blue
ice field on the south side of the volcano, and displays a complex, deformed
stratigraphy. A second important site, Mt.
Moulton, is located at 2800 meters elevation of the summit ridge of
the extinct chain or The tephra layers at Mt. Waesche are dominantly either
coarse and basanitic, probably of local derivation,
or fine and trachytic, mainly derived from West Antarctic volcanoes Mt.
Berlin or Mt. Takahe. Several
new, locally-derived englacial tephra layers were found at Mt. Takahe
during the 1998/99 field season. Although displaying boudin-shaped
features, the thicker tephra layers at Mt. Waesche appear relatively undeformed,
whereas some of the thinner, intercalated layers are strongly isoclinally
folded. Three tephra layers at Mt. Waesche have been geochemically
correlated with layers found at Mt. Moulton. The correlative layers
have ages of between 15 and 27 ka, 27±2 ka, and between 106 and
119 ka, consistent with apparent stratigraphic order. A single
tephra layer at Mt. Waesche has been directly dated using 40Ar/39Ar, and
yields an apparent age of 117±7 ka. Although there are tephra
layers that seem stratigraphically below the 117±7 ka layer, they
appear to represent an overturned repetition of some part of the upper
section. Hence, there is no evidence for ice significantly older
Dunbar, N. W., R. P. Esser, W. C. McIntosh, G. A. Zielinski, and P.
R. Kyle, 1998. Englacial tephra layers in West Antarctica: Implications
for the history of the West Antarctic Ice Sheet. 4th Annual
West Antarctic Ice Sheet Workshop. ABSTRACT
Dunbar, N. W., R. P. Esser, and W. C. McIntosh, 1998, Englacial tephra
layers in West Antarctica: Implications for the history of the West
Antarctic Ice Sheet: Antarctic Journal of the U.S., v. XXXIII- Review
1998.
Dunbar, N. W., R. P. Esser, W. C. McIntosh, P. R. Kyle, and G. A. Zielinski,
1997, Englacial tephra layers in the East and West Antarctic ice sheets: Indicators
of glacial flow patterns on ice sheet margins: EOS, Transactions of the
American Geophysical Union, v. 78, p. F250 ABSTRACT.
Dunbar, N.W., Kurbatov, A., Zielinski, G., McIntosh, W.C., Price, P.B.,
and Bay, R.C., 2003, Volcanic ash records
in the Siple Dome Ice Core: West Antarctic Ice Shelf 2003 Research
Meeting.
Dunbar, N.W.,
Kurbatov, A., Zielinski, G., McIntosh, W.C., Price, P.B., and Bay, R.C.,
2004, Volcanic ash records in the Siple Dome Ice Core: Siple Dome Principal
Investigator Meeting, Reno, NV, Feb. 24, 2003. Download
Powerpoint
Dunbar, N. W., W. McIntosh, R. Esser, T. Wilch, and G. Zielinski, 1998,
Direct dating and geochemical correlations of englacial tephra layers
at two sites in West Antarctica: Proceedings of the West Antarctic Ice
Sheet Meeting Chapman Conference, Sept. 13-18, 1998, p. 18-19. ABSTRACT
Dunbar, N.W., McIntosh, W.C., and Esser, R.P., 2008, Physical setting and tephrochronology of the summit caldera ice record at Mount Moulton, West Antarctica: Geological Society of America Bulletin, v. 120, p. 796-812. See abstact
Dunbar, N.W., McIntosh, W.C., V., K.A., and Wilch, T.I., 2007, Integrated tephrochronology of the West Antarctic region; implications for a potential tephra record in the West Antarctic ice sheet (WAIS) Divide ice core, in Cooper, A., and Raymond, C., eds., Tenth international symposium on Antarctic earth sciences; Antarctica; a keystone in a changing world, U. S. Geological Survey. Extended abstract
DUNBAR, N., G. ZIELINSKI, and D. VOISINS, 2003, Tephra
layers in the Siple and Taylor Dome Ice Cores, Antarctica: Correlations
and Sources. Journal of Geophysical Research,108, 2374-2385. See abstract
Kurbatov, A.V., Zielinski, G.A., Dunbar, N.W., Mayewski, P.A., Meyerson, E.A., Sneed, S.B., and Taylor, K.C., 2006, A 12,000 year record of explosive volcanism in the Siple Dome Ice Core, West Antarctica: Journal of Geophysical Research-Atmospheres, v. 111, p. D12307. See abstract
McIntosh, W.C. and Wilch, T.I., 1995b. Late Pleistocene (223-125 ka)
Plinian eruptions in Marie Byrd Land: Potential time horizons in West
Antarctic ice cores. VII International Symposium of Antarctic Earth Sciences,
Siena, Italy. P. 261.
Wilch, T.I., McIntosh W.C., and Dunbar, N.W., (1999) Late Quaternary
volcanic activity in Marie Byrd Land: potential 40Ar/39Ar
-dated time horizons in future West Antarctic ice and marine cores, Geol.
Soc. Am. Bull., 111, 1563-1580. ABSTRACT
Zielinksi, G., and N. Dunbar, 1998, Volcanic Record from the Siple and
Taylor Domes, Antarctica: WAISCORES Meeting, Sept. 10, 1998.
Any opinions, findings and conclusions or recomendations expressed in
this material are those of the author(s) and do not necessarily reflect
the views of the National Science Foundation (NSF)