Exploring Antarctica
Exploring Antarctica
Exploring Antarctica
Exploring Antarctica
Exploring Antarctica
Exploring Antarctica
Exploring Antarctica
Exploring Antarctica
Exploring Antarctica
Exploring Antarctica
 
Exploring Antarctica

Science Notes - 12/14/03

Graphite Peak, Central Transantarctic Mountains

Palaeosols across the Permian-Triassic boundary at Graphite Peak are strikingly similar to those across the boundary in the Sydney Basin (Retallack 1999b). The suite of tuffaceous and coaly paleosols in the Late Permian upper Buckley Formation are very similar to those in the Newcastle Coal Measures of New South Wales. Green and red paleosols of the Early Triassic Fremouw Formation are similar to those of the Narrabeen Group of New South Wales (Retallack 1976, 1977a, 1977b). At Graphite Peak there is also claystone breccia, pale green in color, but otherwise similar to claystone breccias at the Permian-Triassic boundary in Victoria Land and southeastern Australia (Retallack et al. 1998a). At Graphite Peak, the breccia includes claystone clasts with birefingence fabrics and weathering like those of associated paleosols, as well as numerous altered volcanic rock fragments and much quartz. These boundary beds have yielded rare (0.8 grains.cm-2), small (152 mm) grains of shocked quartz (Retallack et al. 1998b). Becker and Poreda have also recently found fullerenes in the boundary breccia (Becker and Poreda, 2001). A statistically significant but faint iridium anomaly (up to 59 pg.g-1 over background of 20 pg.g-1) also has been detected, but it is from the base of the coal underlying the claystone breccia (Kyte for Retallack et al. 1998a).

Stable isotope analyses of organic carbon in our samples from Graphite Peak (Fig. 3) show that the global Permian-Triassic boundary d13C excursion (Holser et al. 1989, 1991; Morante 1996) is at the contact of the Buckley and Fremouw Formations (Krull & Retallack, 2000). This contact is 1 m above the last Vertebraria root and directly above the last coal in the section. The region around Graphite Peak has been shown to have both Late Permian (stage 5) palynofloras (Farabee et al. 1991) and glossopterid fructifications (Retallack et al. 1998b, Retallack & Krull 1999) and earliest Triassic (Lystrosaurus zone) vertebrates (Elliot et al. 1970; Cosgriff et al. 1982; Hammer 1990a, 1990b; Lucas 1998). Graphite Peak was the initial discovery site for earliest Triassic vertebrates in Antarctica (Barrett et al. 1968), and has yielded bones of Lystrosaurus murrayi, Thrinaxodon liorhinus, Austrobrachyops jenseni and Prolacerta broomi (Colbert 1974; Colbert & Kitching 1977; Hammer 1989, 1990a; Retallack & Hammer 1998) 24-83 m above the base of the Fremouw Formation (280-339). This assemblage is also found about 40 m above the Permian-Triassic boundary in South Africa (Smith & Ward, 2002). The Fremouw Formation also yielded fossil plants including Voltziopsis africana (55 m above base of Fremouw Formation or 301 m ) and Dicroidium zuberi (110 m above base or 366 m), which are Early Triassic species (Retallack 1977a, 1977b, 1995). Permian-Triassic boundary at the Buckley-Fremouw contact is the same as mapped by Collinson & Elliot (1984a), Barrett et al. (1986) and Collinson et al. (1994).

We have preliminary analyses at Graphite Peak sediment samples provided by Retallack from a previous field season at Antarctica for fullerenes and bulk noble gases. A fullerene component was successfully isolated from the acid resistant residue (100 mg) of the Graphite Peak boundary breccia. The helium isotopic ratio of this fullerene component is (30-80x106) and the sub-atmospheric 40Ar/36Ar ratio are consistent with other Permian-Triassic sites (Becker et al., 2001). Interestingly, this ET fullerene signal occurs only at the “upper” boundary layer (see Fig. photo gallery) (~65cm.), coincident with the shocked quartz and not with the Ir that occurs below the coal (~145 cm.) (Retallack et al., 1998). Thus our data support the notion that the boundary is present at Graphite Peak and is coincident with the biostratgraphy, chemostratigraphy and shocked

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Exploring Antarctica
Institute of Crustal Studies National Aeronautics and Space Administration National Science Foundation University of California Santa Barbara