Age determination of hornblende in ODP Site 188-1165 and DSDP Hole 28-268

Sediments from Ocean Drilling Program Site 1165 in the Indian Ocean sector of the Southern Ocean (off Prydz Bay) contain a series of layers that are rich in ice-rafted debris (IRD). Here we present evidence that IRD-rich layers at Site 1165 at 7, 4.8, and 3.5 Ma record short-lived, massive discharges of icebergs from Wilkes Land and Adélie Land, more than 1500 kilometers to the east of the depositional site. This distant source of icebergs is clearly defined by the presence of IRD hornblende grains with 40Ar/39Ar ages of 1200-1100 Ma and 1550-1500 Ma, ages that are not found on the East Antarctic continent in locations closer to Site 1165. This observation requires enormous amounts of detritus-carrying drifting icebergs, most likely in the form of large icebergs. These events probably reflect destabilization, surge, and break-up of ice streams on the Wilkes Land and Adélie Land margins of the East Antarctic Ice Sheet, in the vicinity of the low-lying Aurora and Wilkes Basins. They occurred under warming conditions, but each coast seems to have produced ice-rafting events independently, at different times. The data presented here constitute the first evidence of far-traveled icebergs from specific source areas around the East Antarctic perimeter. Launch of these icebergs may have happened during quite dramatic events, perhaps analogous to "Heinrich Events" in the North Atlantic.

Mercury content and isotopic composition of teeth, and sex and age of skulls of polar bears collected in Svalbard

We examined the use of mercury (Hg) and nitrogen and carbon stable isotopes in teeth of polar bear (Ursus maritimus) from Svalbard as biotracers of temporal changes in Hg pollution exposure between 1964 and 2003. Teeth were regarded as a good matrix of the Hg exposure, and in total 87 teeth of polar bears were analysed. Dental Hg levels ranged from 0.6 to 72.3 ng/g dry weight and increased with age during the first 10 years of life. A decreasing time trend in Hg concentrations was observed over the recent four decades while no temporal changes were found in the stable isotope ratios of nitrogen (d15N) and carbon (d13C). This suggests that the decrease of Hg concentrations over time was more likely due to a lower environmental Hg exposure in this region rather than a shift in the feeding habits of Svalbard polar bears.

(Table 1) Distribution of ostracods in Jurassic sediments of DSDP Hole 79-547

Eighteen samples from the Early Jurassic (Hettangian to Pliensbachian) and nine from the Bajocian to Berriasian interval have been examined. The ostracode fauna has been left largely in open nomenclature pending a more detailed study. At least four new genera, listed simply as Gen. nov. A-D sp. nov. have been recognized. Although many new species are present, there is a similarity between this ostracode fauna and that of northwest Europe of comparable age. This is particularly true for the Early Jurassic from which Bairdia guttulae Herrig, 1979, Ptychobairdia cf. aselfingenensis (Lord and Moorley, 1974), Monoceratina scrobiculata Triebel and Bartenstein, 1938, Bairdia sp. 4134 Michelsen, 1975, Ogmoconcha cf. contractula Triebel, 1941, and Paracypris cf. redcarensis Blake, 1876 have been obtained. Monoceratina vulsa (Jones and Sherborn, 1888), present in the Toarcian to Callovian of Britain, is recorded here from a sample provisionally dated as Bajocian to Callovian on foraminiferal evidence. The more important species are illustrated and their distribution recorded in Table 1.