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Chemical Profile of the Ross Ice Shelf at Little America V, Antarctica

Published online by Cambridge University Press:  30 January 2017

C. C. Langway Jr.,
M. Herron and
J. H. Cragin
C. C. Langway Jr.
Affiliation:
U.S. Army Cold Regions Research and Engineering Laboratory, Hanover, New Hampshire 03755, U.S.A.
M. Herron
Affiliation:
U.S. Army Cold Regions Research and Engineering Laboratory, Hanover, New Hampshire 03755, U.S.A.
J. H. Cragin
Affiliation:
U.S. Army Cold Regions Research and Engineering Laboratory, Hanover, New Hampshire 03755, U.S.A.
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Abstract

Measurements of the concentrations of Na+ K+, Mg2+, and Ca2+ were made on 28 samples from the 255 m deep ice core from Little America V. All concentrations decrease sharply with depth from the firn–ice transition at 52 m to somewhere between 125 m and 150 m. From 150 m to 250 m the cationic concentrations are relatively constant. This is interpreted to indicate that the ice above 125 m fell as snow on the Ross Ice Shelf and that ice below 150 m originated inland on Marie Byrd Land.

On a fait des mesures de concentrations d’ions Na+, K+, Mg2+, et Ca2+ sur 28 échantillons prélevés dans la carotte d’un forage de 255 m dans la glace provenant de Little America V. Toutes les concentrations décroissent rapidement avec la profondeur depuis la transition névé-glace vers 52 m jusqu’a un point entre 125 et 150 m. De 150 à 250 m, les concentrations en cations sont relativement constantes. On interprète ce fait comme une indication que la glace au-dessus de 125 m est tombée sous forme de neige sur la calotte de Ross et que la glace en dessous de 150 m a son origine dans l’intérieur de la Terre Marie Byrd.

Zusammenfassung

Zusammenfassung

An 28 Proben des 255 m langen Bohrkerns von Little America V wurden die Konzentrationen von Na+, K+, Mg2+ und Ca2+ gemessen. Alle Konzentrationen nehmen vom Firn-Eis-Übergang in 52 m Tiefe bis zu einer Tiefe zwischen 125 m–150 m schnell mit zunehmender Tiefe ab. Von 150 m–250 m sind die Konzentrationen der Kationen relativ konstant. Dies wird als Anzeichen dafür gedeutet, dass das Eis über 125 m als Schnee auf das Ross-Schelfeis fiel, während das Eis unter 150 m landeinwärts vom Marie Byrd Land herstammt.

Information

Type
Research Article
Information
Journal of Glaciology , Volume 13 , Issue 69 , 1974, pp. 431 - 435
Copyright
Copyright © International Glaciological Society 1974

Introduction

There is renewed interest in the nature and the origin of Antarctic ice shelves (for example, Ross Ice Shelf: Reference ZumbergeZumberge, 1971; Amery Ice Shelf: Reference BuddBudd, 1966; Reference MorganMorgan 1972). The first ice core ever to be recovered that completely penetrated a floating ice sheet (ice shelf) was obtained near the seaward edge of the Ross Ice Shelf at Little America V (lat. 78° 10’ S., long. 162° 13’ W. in 1957) (Reference Ragle, Ragle, Hansen, Gow and PatenaudeRagle and others, 1960). This core was 255 m long, 10 cm in diameter, and parts of it have been stored since recovery in cold rooms at USA GRRLL at temperatures below –20° C.

Assuming steady-state conditions, Crary and others (1962) estimated that the bottom ice at Little America V may have originated about 340 km from Little America V, about 20 km inland from the grounding line, and that its maximum age was about 4 500 years. They postulated that only the bottom 20 m of ice at Little America V originated inland in West Antarctica. Some studies of physical properties and measurements of electrolytic conductivity were made on the ice core at Little America V (Reference GowGow, 1968[a], Reference Gow[b]). Dansgaard and others (in preparation) recently completed an investigation of the variations in the stable isotopic composition of the core. This report presents results of a study of the Na+, K+, Mg2+, and Ca2+ concentrations found in the Little America V ice core.

Sample Preparation and Analytical Methods

All laboratory work was performed in a laminar-flow clean-air station; workers wore powder-free polyethylene gloves. Core samples 10 to 23 cm long were selected, spaced over the entire depth profile below the firn–ice transition at 52 m. Surface contaminants resulting from drilling and handling were removed from core samples by one of two procedures depending upon whether or not drilling fluid was used during the coring operation. The core above 250 m was obtained in a “dry-hole” (i.e. without the use of drilling fluids), and samples were prepared for chemical analysis by holding them with stainless steel tongs and rinsing with doubly-distilled de-ionized water (DDW). Approximately 1 200 ml of DDW was used per 500 g of sample. Samples below 250 m were exposed to drilling fluid (88% diesel fuel and 12% trichloroethylene) and were cleaned by alternate rinsings with electronic grade acetone and distilled de-ionized water until the odor of drilling fluid could no longer be detected. The core was then rinsed with DDW as described above. The effectiveness of both cleaning procedures was verified (Herron and others, in preparation) by the constancy of ionic concentrations observed in melt water collected sequentially as progressive outer layers of core are removed by melting. For example, the sodium concentration of the outer 20% of a “dry-hole” sample was 185 μg/l, while the remaining five aliquots had an average sodium concentration of 24.4± 1.8 μg/1. Similarly, the outer 30% of a core sample exposed to drilling fluid contained an order of magnitude higher sodium concentration than the 29.0±0.7 μg/l average of the inner aliquots.

Both groups of solid cleaned samples were then melted in pre-cleaned polyethylene containers in a microwave oven and aliquots were taken for analysis. Measurements were made directly on the melt water using atomic absorption. Samples and standards were analyzed in triplicate with average standard deviations in μg/l of: Na+ 1.2; K+, 0.6; Mg2+,0.3; and Ca2+, 0.7.

Results and Discussion

The results of the measurements are presented in Figure 1. Table I lists averages of these data and the Na/K, Na/Mg and Na/Ca ratios. All cationic concentrations decrease sharply from a depth of 52 m to somewhere between 125 m and 150 m. From approximately 150 m to 250 m, the cationic concentrations appear relatively constant. A slight increase in all of the measured constituents appears below 250 m.

Fig. 1.

Concentration profile of Na+, Mg2+, K+ and Caz+ in the Little America V ice core.

Table I.

Average Cationic Concentrations in Ice Core Samples From Little America V and “Byrd” Station, Antarctica.

* Number in parentheses is the number of samples analyzed for Na+, K+ and Mg2+ over the stated depth interval. For Ca2+ one less sample was analyzed in each of the depth intervals 52-84, 90-123, and 250-255 m, resulting in a total of 25 samples.

† Average of five samples deposited between 11 800 and 2 500 B.P. from the Byrd station deep ice core (Cragin and others, in press).

‡ Deviations represent a measure of dispersion of the concentrations for the number of samples measured and are not an indication of precision.

Since deposited snow follows the “law of superposition” (i.e. younger layers overlie older layers), it is evident that the deeper shelf ice is older than the upper shelf ice and originated further up-stream along a flow-line. The differences in cationic concentrations between the ice above 125 m and that below 150 m indicate that the upper ice originated on the shelf itself and that the lower ice originated inland from the grounding line in a different environmental regime. The reported flow-line of ice from West Antarctica to Little America V runs parallel to the West Antarctic coast until it passes the grounding line and then moves toward the seaward edge of the shelf (Reference HughesHughes, 1973). Thus, the lower ice could have been deposited at a rather constant distance from the coast; this explains the uniform composition of the core from 150 m to 250 m.

As shown in Table I, concentration levels and ratios in the lower portion of the core are quite close to those found in recent deposits from the “Byrd” station, West Antarctica area (Cragin and others, in preparation) which is more than 700 km from Little America V. This suggests that the lower ice in the Little America V core originated in an environmental regime similar to that in West Antarctica. The ratios of Na/K, Na/Mg and Na/Ca for the upper portion of the Little America V core approach those of sea-water, reflecting the proximity of the open Ross Sea. The Na/K and Na/Ca ratios decrease with depth; this may indicate a geochemical enrichment of K+ and Ca2+ relative to Na+ that becomes more pronounced in deposits greater distances from the coast (Reference Chesselet, Chesselet, Morelli and Buat-MenardChesselet and others, 1972; Reference Boutron, Boutron, Echevin and LoriusBoutron and others, 1972). The low silicon concentration (0.8 μg/l) found in West Antarctica (Reference Murozumi, Murozumi and PattersonMurozumi and others, 1969) suggests that the contribution of terrestrial dust to Marie Byrd Land is negligible.

The above interpretation is in accord with a possible interpretation of the profile of the stable isotopic composition of the core (Dansgaard and others, in preparation). Also, Reference GowGow (1970) found an abrupt change in ice texture and fabric in the core at about 150 m which he suggested may be due to a transition from shelf- to inland-derived ice. The slight apparent increase below 250 m in all constituents measured cannot be entirely due to diffusion of ions from the sea-water below. In addition, the concentration levels in the bottom 5 m of the core are too low to indicate sea-water accretion and, in fact, physical and temperature gradient considerations indicate that appreciable melting of the bottom of the ice occurs at Little America V (Reference Crary, Crary, Robinson, Bennett and BoydCrary and others, 1962). Furthermore, stable oxygen isotopic measurements confirm that the core is composed entirely of glacial ice (Dansgaard and others, in preparation).

In the absence of supporting chemical data along the proposed flow-line, another interpretation of the data must be considered. Concentrations of sea-salt constituents in precipitation generally decrease with increasing distance from the coast until a stable concentration plateau is reached (Reference JungeJunge, 1963). In general, the greater the distance of this plateau from the coast the lower the plateau concentration. Such a plateau was found to exist at distances of 600 km to 900 km from the coast in East Antarctica, with average plateau sodium concentrations of 23 μg/1 (Reference Boutron, Boutron, Echevin and LoriusBoutron and others, 1972). This compares favourably with the average sodium concentration of 27 ug/l in the section of the Little America V core approximately from 150 m to 250 m. No corresponding traverse data exist for West Antarctica; but, if a similar phenomenon exists there, the relative constancy of the concentrations in the portion of the core from 150 m to 250 m suggests that this mass of ice may have originated more than 600 km inland from Little America V.

Conclusions

Our results suggest that more than the lower 20 m of the Ross Ice Shelf at Little America V must have originated inland from the grounding line. We are led to believe that flow conditions in West Antarctica have not existed in a steady state for the last several thousand years. If the lower ice originated 600 km from Little America V instead of the calculated 340 km (Crary and others, 1962), flow rates may have been much higher in the recent past than at present and the age of the bottom ice may be much less than the calculated 4 500 years. Reference Johnsen, Johnsen, Dansgaard, Clausen and LangwayJohnsen and others (1972) reported an apparent decrease in surface altitude at Byrd Station with a greatly negative mass budget lasting from 4000 B.P. to 2500 B.P. The accompanying increased ice flow rates would probably bring ice from further inland to little America V. A more definitive analysis of the recent history of the Ross Ice Shelf depends upon additional cores and surface samples from various geographical areas of West Antarctica.

Acknowledgements

Financial support was provided by the National Science Foundation under grants AG-212 and AG-394. We thank G. Klouda of USA CRREL who performed some of the chemical analyses and S. J. Johnsen of the University of Copenhagen who kindly reviewed the manuscript.

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Figure 0

Fig. 1.Concentration profile of Na+, Mg2+, K+ and Caz+ in the Little America V ice core.

Figure 1

Table I.Average Cationic Concentrations in Ice Core Samples From Little America V and “Byrd” Station, Antarctica.