Abstract:[1] We report analyses of hydrogen abundance in experimentally annealed and natural mantle minerals using FTIR and use these data to establish calibration lines for measurement of H 2 O concentrations in olivine, pyroxenes, garnet, amphibole and mica by secondary ion mass spectrometry (SIMS). We have reduced the detection limit for H 2 O analysis by SIMS to 2-4 ppm H 2 O (by weight) through careful attention to sample preparation and vacuum quality. The accuracy of the SIMS calibrations depends on the choice o… Show more
“…Therefore, this cumulate package represents depleted Martian mantle, a composition comparable in incompatible element composition to terrestrial depleted mantle (i.e., the MORB source [Sun and McDonough 1989] The addition of a reasonable amount of initial water (0.05 wt%) to the Martian magma ocean does not affect the majority of the crystallization sequence perceptibly. The early crystallizing minerals are all nominally anhydrous, meaning that though they can contain petrologically significant amounts of OH (as much as 1000-1500 ppm for olivine and orthopyroxene) (Koga et al 2003;Bell et al 2004;Aubaud et al 2004;Bolfan-Casanova and Keppler 2000), the effect on the overall water content of the melt is small. It is in the late stages of crystallization that the amount of water becomes significant (Fig.…”
Section: Incompatible Element Evolution During Magma Ocean Crystallizmentioning
“…Therefore, this cumulate package represents depleted Martian mantle, a composition comparable in incompatible element composition to terrestrial depleted mantle (i.e., the MORB source [Sun and McDonough 1989] The addition of a reasonable amount of initial water (0.05 wt%) to the Martian magma ocean does not affect the majority of the crystallization sequence perceptibly. The early crystallizing minerals are all nominally anhydrous, meaning that though they can contain petrologically significant amounts of OH (as much as 1000-1500 ppm for olivine and orthopyroxene) (Koga et al 2003;Bell et al 2004;Aubaud et al 2004;Bolfan-Casanova and Keppler 2000), the effect on the overall water content of the melt is small. It is in the late stages of crystallization that the amount of water becomes significant (Fig.…”
Section: Incompatible Element Evolution During Magma Ocean Crystallizmentioning
“…It is worth noting that H + diffusion by the redox mechanism in olivine is on the same order of magnitude as H 2 O diffusion in andesitic melt, which raises the question whether any H 2 O-loss occurred through the olivine instead of exclusively through the melt in the embayment. However, diffusive equilibration through the olivine is also a function of its partition coefficient (Qin et al, 1992), which is very low in olivine (Kd H2O ol/liq = 0.001; Aubaud et al 2004;Koga et al 2003), and so equilibration will be much more efficient through the melt embayment to the bubble. Moreover, significant diffusive equilibration (> 10%) was only observed for relatively small melt inclusions in the Fuego samples (< 30 μm radius; Lloyd et al, 2013); the larger relative volume of the melt embayments (equivalent to a 100-200 μm diameter inclusion) would only experience 1-2% equilibration through the olivine over 10-30 minutes, based on the calculations in Lloyd et al (2013, their Fig.…”
Section: Implications For the 1974 Fuego Eruptionmentioning
The explosivity of volcanic eruptions is governed in part by the rate at which magma ascends and degasses. Because the time scales of eruptive processes can be exceptionally fast relative to standard geochronometers, magma ascent rate remains difficult to quantify.
“…However, a major challenge in making accurate and precise measurements of H 2 O contents at such low abundances with an instrument such as SIMS is the quantification of background hydrogen. Methods used to reduce extraneous contribution of H during measurements include bakingout of the instrument, mounting samples and analytical standards in a hydrogen-free medium, and storing samples in a vacuum oven/desiccator prior to analysis [149,150]. As a result, indium metal is now routinely used as a mounting medium for the standards used to calibrate against unknowns [149,150].…”
Section: Challenges and Future Prospects (A) Analytical Challengesmentioning
A paradigm shift has recently occurred in our knowledge and understanding of water in the lunar interior. This has transpired principally through continued analysis of returned lunar samples using modern analytical instrumentation. While these recent studies have undoubtedly measured indigenous water in lunar samples they have also highlighted our current limitations and some future challenges that need to be overcome in order to fully understand the origin, distribution and evolution of water in the lunar interior. Another exciting recent development in the field of lunar science has been the unambiguous detection of water or water ice on the surface of the Moon through instruments flown on a number of orbiting spacecraft missions. Considered together, sample-based studies and those from orbit strongly suggest that the Moon is not an anhydrous planetary body, as previously believed. New observations and measurements support the possibility of a wet lunar interior and the presence of distinct reservoirs of water on the lunar surface. Furthermore, an approach combining measurements of water abundance in lunar samples and its hydrogen isotopic composition has proved to be of vital importance to fingerprint and elucidate processes and source(s) involved in giving rise to the lunar water inventory. A number of sources are likely to have contributed to the water inventory of the Moon ranging from primordial water to meteorite-derived water ice through to the water formed during the reaction of solar wind hydrogen with the lunar soil. Perhaps two of the most striking findings from these recent studies are the revelation that at least some portions of the lunar interior are as water-rich as some Mid-Ocean Ridge Basalt source regions on Earth and that the water in the Earth and the Moon probably share a common origin.
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