Italian Antarctic Data Center
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During the XX and XXI Italian Antarctic expeditions (2004/05, 2005/06), 668 rocks have been sampled within the aim of the project "Chronologic-dynamic zoning of the Ross Orogen" in northern and southern Victoria Land. They include intrusive, subvolcanic, volcanic, metamorphic and sedimentary rocks. The investigated regions are within Cape Hallett SS 58-60/2, Coulman Island SS 58-60/6, Daniels Range SR 57-58/14, Freyberg Mountains SS 58-60/1, Mount Melbourne SS 58-60/9, Mount Murchison SS 58-60/5, Mount Soza SR 57-58/15, Ob' Bay SR 57-58/11, Pomerantz Tableland SR 57-58/10, Relief Inlet SS 58-60/13, Sequence Hills SS 55-57/8 and Welcome Mountain SS 55-57/4 USGS sheets.
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During the XXVI and XXVII Italian Antarctic expeditions (2010/11, 2011/12), 668 rocks have been sampled within the aim of the project "Geological continental markers of Cenozoic climate changes in Victoria Land, Antarctica" in northern Victoria Land. They include intrusive, subvolcanic, volcanic, metamorphic and sedimentary rocks. The investigated regions are within Cape Hallett SS 58-60/2, Coulman Island SS 58-60/6, Mount Joyce SS 55-57/16, Mount Melbourne SS 58-60/9, Mount Murchison SS 58-60/5 and Relief Inlet SS 58-60/13 USGS sheets.
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The project aims to carry out a climatological analysis of the dynamics and structure of the Antarctic polar stratospheric vortex over the last decade 1993-2003 and its relationship with the 'Ozone (O3) hole' phenomenon. In particular will be evaluated all the data from the ground by LIDAR, gained by balloon and by satellite, a high resolution transport model and a GCM model will be used for the climatic characterization of the dynamics of the vortex and its interactions with the polar troposphere and mid-latitudes, and finally a climatology of aerosols and PSCs will be analyzed during the polar winter.
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The Observatory main purpose is to contribute to the monitoring of global climate change monitoring standard meteorological parameters. The automatic weather station AWS Paola is located at Talos Dome (72° 49′ 45″ S - 159° 11′ 36″ E) at 2370 m a.s.l., and has been installed on the 26 january 2003. It acquired, every hour, all year round, the meteorological vaiables of wind velocity, wind direction, temperature, pressure and relative humidity, plus snow height acquired as daily averages.
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The Concordia Research Station provides a unique location for preparatory activities for future human journey to Mars, to explore microbial diversity at subzero temperatures and monitor the dissemination of human-associated microorganisms within the pristine surrounding environment. The present study was performed in the frame of the BacFinder project (European Space Agency, ESA AO-13-Concordia) with the aim to unravel the environmental- and human-associated microbial diversity in the surrounding of the Concordia Station. This is the first intensive and extensive surface snow sampling performed monthly over a two-year period at three distances (10, 500, and 1000 m) from the Concordia Station, and investigated by a high-throughput sequencing approach. Emphasis was laid on the relation between microbial presence and both seasonality and distance from the Base. Data suggested that if present the anthropogenic impact was below the detection limit of the employed DNA sequencing-based techniques. On the other hand, our study corroborated the use of DNA sequencing for revealing microbial presence in remote and hostile environments, with implications for Planetary Protections and for life-detection in astrobiology relevant targets.
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This dataset includes all the lunar meteorites (achondrites) collected during the Italian Antarctic Expeditions since 2013 in Victoria Land and now preserved at the repository of the Museo Nazionale dell’Antartide.
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