Jhc. Bain et al., TOWARDS AN UNDERSTANDING OF THE AGE AND ORIGIN OF MESOTHERMAL GOLD MINERALIZATION IN THE ETHERIDGE GOLDFIELD, GEORGETOWN REGION, NORTH QUEENSLAND, Australian journal of earth sciences, 45(2), 1998, pp. 247-263
Small mesothermal vein quam-gold-base-metal sulfide deposits from whic
h some 20 t of Au-Ag bullion have been extracted, are the most common
gold deposits in the Georgetown region of north Queensland-several hun
dred were mined or prospected between 1870 and 1950. These deposits ar
e mostly hosted by Proterozoic granitic and metamorphic rocks and are
similar to the much larger Charters Towers deposits such as Day Dawn a
nd Brilliant, and in some respects to the Motherlode deposits of Calif
ornia. The largest deposit in the region-Kidston (> 138 t of Au and Ag
since 1985)- is substantially different. It is hosted by sheeted quar
tz veins and cavities in brecciated Silurian granite and Proterozoic m
etamorphics above nested high-level Carboniferous intrusives associate
d with a nearby cauldron subsidence structure. This paper provides new
information (K-Ar and Rb-Sr isotopic ages, preliminary oxygen isotope
and fluid-inclusion data) from some of the mesothermal deposits and c
ompares it with the Kidston deposit. All six dated mesothermal deposit
s have Siluro-Devonian (about 425 to 400 Ma) ages. All nine of such de
posits analysed have delta(18)O quartz values in the range 8.4 to 15.7
parts per thousand, Fluid-inclusion data indicate homogenisation temp
eratures in the range 230-350 degrees C. This information, and a re-in
terpretation of the spatial relationships of the deposits with various
elements of the updated regional geology, is used to develop a prelim
inary metallogenic model of the mesothermal Etheridge Goldfield. The m
odel indicates how the majority of deposits may have formed from hydro
thermal systems initiated during the emplacement of granitic batholith
s that were possibly, but not clearly, associated with Early Palaeozoi
c subduction, and that these fluid systems were dominated by substanti
ally modified meteoric and/or magmatic fluids. The large Kidston depos
it and a few small relatives are of Carboniferous age and formed more
directly from magmatic systems much closer to the surface.