In situ U-Pb and geochemical evidence for ancient Pb-loss during hydrothermal alteration producing apparent young concordant zircon dates in older tuffs

Author(s):  
Jian-Wei Zi ◽  
Birger Rasmussen ◽  
Janet R. Muhling ◽  
Ian R. Fletcher
1992 ◽  
Vol 129 (2) ◽  
pp. 243-246 ◽  
Author(s):  
R. C. Greenwood ◽  
A. E. Fallick ◽  
C. H. Donaldson

AbstractRecent studies indicate that the Rum Tertiary ultrabasic intrusion formed in situ, and was not emplaced as a fault-bounded plug. The suggestion that the Main Ring Fault was the primary pathway for the flow of meteoric-hydrothermal fluids on Rum is therefore seriously flawed. Oxygen isotope evidence is presented indicating that the contact zone of the intrusion was the major pathway for meteoric fluids during cooling of the pluton. δ18O depletions of over 12‰ correlate with hydrothermal alteration assemblages, indicating that the bulk of the interaction with meteoric fluids took place at low temperatures (200–450 °C).


2020 ◽  
Vol 7 (5) ◽  
pp. 1481-1495
Author(s):  
Pieter Bots ◽  
Joanna C. Renshaw ◽  
Timothy E. Payne ◽  
M. Josick Comarmond ◽  
Alexandra E. P. Schellenger ◽  
...  

Colloidal silica is a nanoparticulate material that could have a transformative effect on environmental risk management at nuclear legacy sites by preventing radioactive contamination through the in situ installation of injectable hydraulic barriers.


2020 ◽  
Author(s):  
Mathias Peter ◽  
Wolfgang Bach ◽  
Wolf-Achim Kahl ◽  
Andreas Luttge ◽  
Andreas Turke ◽  
...  

<p><strong>Surface reaction kinetics of volcanic materials at hydrothermal conditions – an in-situ experiment at the Surtsey volcano</strong></p><p>The diversity and functioning of microbial life is a key research topic in the field of marine geochemistry and geobiology. For understanding biological processes at the temperature limit of functional life, it is necessary to gain insights about microbe-rock-fluid interactions under natural hydrothermal conditions within the basaltic ocean crust. Although there has been research in the field of biological interactions on olivine and tephra surface in laboratories and samples from volcanos ([1], [2]), the kinetics of microbe-rock-fluid interactions has not been systematically evaluated by in-situ experiment in a natural reservoir.</p><p>During the ICDP SUSTAIN Expedition 5059 at the Surtsey volcano off the southern coast of Iceland in 2017, a borehole was endowed with a subsurface observatory to analyze the evolution of olivine (Fo<sub>90</sub>) and volcanic glass surfaces embedded in PEEK containers at fixed temperatures ranging from 25°C to 125°C for two years ([3]). This incubation experiment delivers novel data of surface reaction kinetics under defined conditions in a natural setting.</p><p>In-depth analysis of the sample surface with vertical scanning interferometry, atomic force microscopy as well as Raman spectrometry provides insights into solid-fluid reactions of volcanic minerals. On the one hand, this analysis delivers a quantitative and qualitative breakdown of the chemical and physical alteration of natural matter below the oceanic crust. On the other hand, the in situ experiment facilitates a validation of a range of experiments that have been performed in laboratories under similar conditions. The possibility to gain knowledge about dissolution and precipitation on the interface of common seafloor materials within a natural hydrothermal system is critical step towards understanding submarine microbial life.</p><p> </p><p>[1] Konhauser, K. O., Schiffman, P., and Fisher, Q. J., Microbial mediation of authigenic clays during hydrothermal alteration of basaltic tephra, Kilauea Volcano, Geochem. Geophys. Geosyst., 3( 12), 1075, doi:10.1029/2002GC000317, 2002.</p><p>[2] Malvoisin, B., Brunet, F., Carlut, J., Rouméjon, S., and Cannat, M. (2012), Serpentinization of oceanic peridotites: 2. Kinetics and processes of San Carlos olivine hydrothermal alteration, J. Geophys. Res., 117, B04102, doi:10.1029/2011JB008842.</p><p>[3] Türke, A., et al. (2019). "Design of the subsurface observatory at Surtsey volcano, Iceland." Sci. Dril. 25: 57-62.</p>


1984 ◽  
Vol 75 ◽  
pp. 743-759 ◽  
Author(s):  
Kerry T. Nock

ABSTRACTA mission to rendezvous with the rings of Saturn is studied with regard to science rationale and instrumentation and engineering feasibility and design. Future detailedin situexploration of the rings of Saturn will require spacecraft systems with enormous propulsive capability. NASA is currently studying the critical technologies for just such a system, called Nuclear Electric Propulsion (NEP). Electric propulsion is the only technology which can effectively provide the required total impulse for this demanding mission. Furthermore, the power source must be nuclear because the solar energy reaching Saturn is only 1% of that at the Earth. An important aspect of this mission is the ability of the low thrust propulsion system to continuously boost the spacecraft above the ring plane as it spirals in toward Saturn, thus enabling scientific measurements of ring particles from only a few kilometers.


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