Monday, May 19, 2008

Thesis Defense - Spring 2008 - Sarah Johnson

Physical, petrological, and chemical trends associated with the conversion of k-feldspar-absent quartz dioritic and tonalitic conestones to saprolite in a meditteranean (hot summer) climate, Santa Margarita Ecological Reserve (SMER), southern California, U.S.A

Sarah Johnson
M.S. Candidate
Department of Geological Sciences
San Diego State University

Advisor Dr. Gary Girty

Friday, May 9th

ABSTRACT
W. Nesbitt and colleagues proposed that weathered plutonic material will spread linearly from parental fields subparallel to the A-CN join toward the A-K join on A-CN-K diagrams, and followed by a linear trend subparallel to the A-K join towards the A apex. Such linear trends are common because soil solutions are typically supersaturated with respect to K, but not CN. At SMER, our studies reveal a weathering trend that deviates from that proposed by W. Nesbitt and colleagues. SMER lies within a Mediterranean (hot summer) climate with an average precipitation of ~39.4 cm/yr and average temperature of ~16.6˚C. We sampled corestone and adjacent saprolite in an ~123 Ma tonalite, and at two sites lying within an ~107.5 Ma quartz diorite for thin section, physical properties, and chemical analyses. We used the chemical index of alteration (CIA) to determine the degree of weathering and used the transport function (τ) for assessing changes in elemental mass. Each variety of sampled corestone lacks modal K-feldspar but contains 4.50% to 12.0% biotite. Our thin section study of samples of saprolite suggests the following order, from most to least weathered; biotite, amphibole, plagioclase, and quartz. On A-CN-K diagrams saprolitic samples spread linearly from the parental material away from the K apex toward the A-CN join. XRD and microscope analyses indicate that this trend is due to the conversion of biotite to the mixed-layer expandable clays vermiculite-illite and vermiculite-smectite. The transport function, (τ), indicates that during this conversion K, Rb, and to a lesser extent Ba mass was consistently removed at the level of our sampling traverses by migrating paralithic fluids. In contrast, zero to only minor increases or decreases in the masses of most other elements reflect the spatially inconsistent and varied activity of eluviation and illuviation processes within the paralithic zone. Our data consistently suggest that in plutonic rocks lacking K-feldspar, biotite weathers more readily than plagioclase, and, as a result, it controls the direction of weathering trends in A-CN-K space. As noted above, the signature of this process is a trend in saprolitic samples extending from unweathered parental plutonic material away from the K apex and toward the A-CN join. Once biotite has been completely altered, then the weathering of plagioclase should produce a new trend extending subparallel to the A-CN join and toward the A apex. Under the Mediterranean (hot summer) conditions at SMER our data appear to have captured the first step in the initiation of this process.

Thursday, May 8, 2008

Thesis Defense - Spring 2008 - Wallace Sconiers

The feasibility of antipodal volcanism as a result of the K/T impact

Wallace Sconiers
B.S. Candidate
Department of Geological Sciences
San Diego State University

Advisor Dr. Jared Morrow

Friday, May 9th

ABSTRACT
Research regarding the impact event at the Cretaceous-Tertiary (K/T) boundary at Chicxulub, Yucatan Peninsula, and the Deccan flood basalts of Western India has shown both possibility and dismissal of the two as being a series of interrelated events, although most workers agree that both sides were relatively antipodal at the K/T boundary. Subsequent 2D & 3D computer models following the development of Simplified Arbitrary Lagrangian-Eulerian (SALE) and similar code have shown that axial focusing of seismic waves following an impact for a planet analogous to earth is most significant at ~100 km depth below the antipode surface. However, calculations of the initial kinetic energy, total seismic energy produced as a function of the seismic efficiency for a C2 Chondrite bolide impact, and total energy delivered to a basaltic volume near its melting point at a depth of ~100 km generate a thermal pulse, or sudden change in temperature, of 1 millikelvin. This temperature increase is not sufficient to create or enhance pre-existing melts at depth.
Estimates of the total volume of lavas produced at the Deccan traps range from 1 x 10^5 to 1 x 10^6 km^3 over a duration of ~1 m.y., with average intervals between eruptions of sub-groups within the traps of 2-10,000 years. A stratigraphic section composed of main eruptive units within the traps shows one sub-group, the Wai, which is responsible for 50% of the total eruption volume from 66 to 64.5 Ma, peaking with the Ambenali Formation within the sub-group producing 200,000 km^3 of basalt 66 to 65.5 Ma. Activity substantially drops during the last two formations within the sub-group, Panhala and Desur, producing 25,000 and 10,000 km^3, respectively. A ~65 Ma date for the K/T impact would have had no effect on the Deccan trap system whose eruptive volumes were dropping per successive formation at this time.

Thesis Defense - Spring 2008 - Angela Cavallini

Major element variations of Hawaiian parental magmas:
Mantle source or melting control?


Angela Cavallini
B.S. Candidate
Department of Geological Sciences
San Diego State University

Advisor Dr. Aaron Pietruszka

Friday, May 9th

ABSTRACT
The abundances of the major element oxides (SiO2, TiO2, Fe2O3, MnO, MgO, CaO, NaO2, K2O, P2O5) in Hawaiian lavas are subject to change due to variation in (1) the amount of crystal fractionation or accumulation or (2) the pressure (depth) and degree of partial melting of the mantle, and (3) differences in the composition of the mantle source. Since isotope ratios (e.g. 206Pb/204Pb or 87Sr/ 86Sr) are not subject to the effects of crystal fractionation or partial melting, they are thought to be good indicators of the mantle source composition. Literature data shows that there is a correlation between the isotope ratios and major elements abundances of Hawaiian lavas when the latter are corrected for the effects of crystal fractionation. This suggests a relationship between the major element chemistry and the mantle source composition. However, another possibility is that the variations are related to changes in the depth of melting. Hawaiian volcanoes been categorized into two main geographic trends: the northeastern Kea trend (named after Mauna Kea) and the southwestern Loa trend (named after Mauna Loa). In this study, I summarized major element data for both Kea and Loa lavas from the scientific literature. The Kea trend lavas include Mauna Kea and Kilauea and the Loa trend lavas include Mauna Loa, Koolau, and Kahoolawe. Prior to this study, Loihi lavas were grouped with the Loa trend (based on geography), but I found that their chemistry is actually more similar to the Kea trend. To correct for the effect of crystal fractionation and accumulation, sample data were adjusted to a constant MgO value. This was achieved by running the data through a computer program which added or subtracted small increments of equilibrium olivine to each sample composition until 13 wt. % MgO was reached. My results show that there are significant variations in the major elements chemistry between Kilauea, Kahoolawe, Mauna Kea, Mauna Loa and Loihi lavas. The Kea trend lavas are relatively low in SiO2 and abundant in CaO. The Loa trend lavas have higher SiO2 and lower CaO. Some of the most significant variations are a range greater than 3% in both SiO2 and CaO. A 2% range in SiO2 can possibly be explained by variations in the pressure (depth) of melting. However, these same pressure differences cannot explain the 3% variation in CaO. Thus, these major elements variations are better explained by differences in the mantle source composition of these volcanoes. The lower SiO2 and higher CaO lavas are consistent with melting mantle peridotite, whereas the higher SiO2 and lower CaO lavas are not. These lavas are likely formed by melting of pyroxenite derived from ancient, recycled oceanic crust within the Hawaiian mantle plume.