The large late-glacial Ho eruption of the Hudson volcano, southern Chile
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Weller, D.
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The large late-glacial Ho eruption of the Hudson volcano, southern Chile
Abstract
Lakes formed in the Aysén region of southern Chile
after the retreat of mountain glaciers, established by ~17,900
calendar years before present (cal years BP) or earlier, contain
numerous late-glacial and Holocene tephra layers derived
from >70 eruptions of the volcanoes in the region, including
Hudson, the southernmost in the Andean Southern Volcanic
Zone (SVZ). Sediment cores fromseven of these lakes contain
an unusually thick late-glacial age tephra layer, which based
on its distribution and bulk trace-element composition was
derived from a large explosive eruption of Hudson volcano
between 17,300 and 17,440 cal years BP and is termed Ho. In
13 cores from six of these lakes, each located ~100 km generally
northeast of Hudson, the Ho tephra layer ranges between
50 and 88 cm in thickness, and contains pumice grains
up to 2 cm in maximum diameter. Comparison with three
previously documented large explosive Holocene Hudson
eruptions (H1 at 7,750 cal years BP, H2 at 3,920 cal years
BP, and H3 in 1991 AD) suggests that Ho was larger, with an
estimated tephra volume of >20 km3, the largest post-glacial
eruption documented for any volcano in the southern Andes
and most likely responsible for the formation of the Hudson
caldera. In total, Hudson has erupted ≥45 km3 of pyroclastic
material in the last ~17,500 years, making it the most productive volcano in the southern Andes in terms of the total
volume erupted since the beginning of deglaciation in the
region. Chemical stratification is not seen in the waterlain
Ho tephra, but these deposits are bi-modal, consisting of a
much greater proportion of dark glassy basaltic-trachyandesite
dense fragments and pumice, with glasses which range between
55 and 59 wt.% SiO2, along with volumetrically lesssignificant
lighter-colored trachydacite pumice, with glass of
66 wt.% SiO2. In contrast, H1 products are trachyandesitic in
composition, H2 ones are more felsic than H1, being composed
essentially of trachydacite, and although H3 1991 AD
again produced tephra of bi-modal compositions, it erupted a
much smaller proportion of mafic compared to felsic material
than did Ho. Thus, the repetitive large explosive eruptions of
Hudson volcano have evolved to progressively less-mafic
overall compositions from late-glacial to historic times, and
their volumes have decreased. Sr-isotopic composition of bulk
samples of the most mafic dense glass and most felsic pumice
components of the Ho tephra, as well as samples from other
Hudson eruptions, which overall range from 51 to 66 wt.%
SiO2, with 525 to 227 ppm Sr, are all similar (0.70444±
0.00007), indicating that crystal-liquid fractionation rather
than crustal assimilation was the main process responsible
for these chemical variations.
General note
Artículo de publicación ISI
Patrocinador
This research
was supported by Fondecyt (Chile) grant #1121141, the Institute of
Ecology and Biodiversity grants ICM P05–002 and PFB-23, and the
Department of Geological Sciences, CU-Boulder. We also would like to
thank A. Vichick, T. Nightingale,M., D.T., D.R, and D.T.Weller for their
continued support.
Quote Item
Bull Volcanol (2014) 76:831
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