Events
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JSG | BEG | UTIG | EPS |
DeFord Lecture: Astrid Holzheid
Start:October 3, 2019 at 3:45 pm
End:
October 3, 2019 at 5:00 pm
Location:
JGB 2.324
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UTIG Seminar Series: Caroline Beghein, UCLA
Start:October 4, 2019 at 10:30 am
End:
October 4, 2019 at 12:00 pm
Location:
PRC ROC Room 1.603
Contact:
Constantino Panagopulos, costa@ig.utexas.edu, 512-574-7376
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Host: Thorsten Becker
Title: Physical Constraints on the Oceanic Plate From Seismic Tomography and Thermodynamics
Abstract: The nature of the interface between the lithosphere and underlying asthenosphere in oceanic settings is still the subject of debate. In particular, questions remain regarding whether it is a temperature-dependent rheological transition, as expected in a thermal convection system, or it is additionally affected by the presence of melts and/or fluids. In this talk, I will present tomographic models of upper mantle seismic wave velocities and anisotropy under the Pacific plate and discuss their interpretation in terms of temperature, melt, and water content.
Our models resulted from the inversion of fundamental ande surface waves using both regularized inverse techniques and a Monte Carlo approach to quantify uncertainties. We found that both shear-wave velocity anomalies and azimuthal anisotropy patterns vary with seafloor crustal age. The thickness of the plate determined from isotropic velocities increases with crustal age, as expected for a thermal control, though uncertainties can be substantial. Similarly, the depth at which the azimuthal anisotropy is well aligned with the plate motion direction increases with age and tends to display a half-space cooling age dependence. In addition, we found that the depth of the Gutenberg discontinuity, which has been mapped in other studies with body wave data and is often associated with the lithosphere-asthenosphere boundary (LAB) and the presence of melts, coincides with high-vertical gradients in azimuthal anisotropy and is located within the age-thickening seismic lithosphere. We hypothesize that the Gutenberg discontinuity results from dehydration of the mantle underlying the mid-ocean ridge, resulting in a chemically depleted, viscous layer that translates away from the spreading center and becomes overprinted by lower temperatures as the plate cools down.
On the contrary, while radial anisotropy models obtained from inversions of Love and Rayleigh wave dispersion do not display any obvious age dependence, we found that they are generally less robust and reliable than azimuthal anisotropy and isotropic velocity models. They tend to differ in pattern depending on which surface wave dataset is employed and their uncertainties are sufficiently large that they cannot be used to constrain the LAB depth reliably.
To better constrain the physical nature of the LAB, we tested our isotropic shear wave velocity models against synthetic models calculated based on thermodynamic considerations for half-space and plate models. We tested the hypothesis that asthenospheric low seismic velocities may have a solid state origin and can be explained purely by thermal effects, including those on seismic attenuation, without any requirement for an additional effect of melt. Our results suggest that, while any direct signature of sub-ridge melt would be too small-scale to be resolved by our data, no significant fractions of melt are needed to explain the shear wave velocities. We note, however, that tomography uncertainties are large and some amount of melt could thus be present but not resolved. In addition, our tomography results are best explained by synthetic models that include a decrease in attenuation due to dehydration by melting at the ridge than by dry models or plate models. This is generally consistent with our azimuthal anisotropy model interpretation, but additional studies to refine the resolution of the anisotropy models are needed.
DeFord Lecture: Liviu Matenco
Start:October 10, 2019 at 3:45 pm
End:
October 10, 2019 at 5:00 pm
Location:
JGB 2.324
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UTIG Seminar Series: Chris Glein, Southwest Research Institute
Start:October 11, 2019 at 10:30 am
End:
October 11, 2019 at 12:00 pm
Location:
PRC ROC Room 1.603
Contact:
Constantino Panagopulos, costa@ig.utexas.edu, 512-574-7376
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Speaker: Chris Glein, Southwest Research Institute San Antonio
Host: Duncan Young
Title: Enceladus: Pathfinder of alien oceans
Abstract: The past decade brought a remarkable transformation in humanity’s understanding of oceans. We used to really know only one ocean – the one that our species has grown up with on Earth. Now, we are starting to learn about other oceans that exist beyond Earth. This talk will focus on Saturn’s moon Enceladus, which is commonly called an “ocean world”. I will present a historical perspective of our exploration of Enceladus, primarily by NASA’s Cassini mission. I will also describe how we came to learn that Enceladus hosts a deep ocean under its icy exterior, and what the ocean is like mainly in terms of its geochemistry and potential habitability. Lastly, I will discuss ongoing efforts to use our experience at Enceladus to guide future exploration of Enceladus and other ocean worlds of great astrobiological interest, such as Jupiter’s moon Europa.
De Ford Lecture Series: Chris Bell
Start:October 17, 2019 at 3:45 pm
End:
October 17, 2019 at 5:00 pm
Location:
JGB 2.324
UTIG Seminar Series: Bob Kopp, Rutgers University
Start:October 18, 2019 at 10:30 am
End:
October 18, 2019 at 12:00 pm
Location:
PRC ROC Room 1.900
Contact:
Constantino Panagopulos, costa@ig.utexas.edu, 512-574-7376
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PLEASE NOTE: THIS WILL BE A REMOTE PRESENTATION
THE PRESENTATION WILL BE SCREENED LIVE AT ROC 1.900
Speaker: Bob Kopp, Rutgers University
Host: Pedro DiNezio
Title: Coasts in times of sea-level rise
Abstract: Around the world, sea levels are rising in response to warming oceans, melting glaciers, and shrinking ice sheets – and even faster rise is projected in the coming century. In this talk, I will explore the different physical processes driving sea-level rise, the geological record of past sea-level changes, methods for assessing the probability of different levels of future changes, and the implications for future coastal flood risks.
Hot Science - Cool Talk: Sustainability of Outer Space
Start:October 18, 2019 at 7:00 pm
End:
October 18, 2019 at 8:15 pm
Location:
William C. Powers Student Activity Center (WCP)
Contact:
Didey Montoya, didey@austin.utexas.edu, 5124714211
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Is it really true that there are over 20,000 junked satellites in outer space? What is their fate? Dr. Moriba Jah examines what we can do to make space safe, secure and sustainable in the long term.
Save the Date - Annual Tailgate Party
Start:October 19, 2019
End:
October 19, 2019
Location:
University of Texas at Austin campus
Contact:
Kristen Tucek, ktucek@jsg.utexas.edu, 512-471-2223
DeFord Lecture: Sharon Mosher
Start:October 22, 2019 at 3:30 pm
End:
October 22, 2019 at 5:00 pm
Location:
JGB 2.324
DeFord Lecture: Melissa Sims
Start:October 24, 2019 at 3:30 pm
End:
October 24, 2019 at 5:00 pm
Location:
JGB 2.324
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UTIG Seminar Series: Kelly Hereid, Chubb Corp.
Start:October 25, 2019 at 10:30 am
End:
October 25, 2019 at 12:00 pm
Location:
PRC ROC Room 1.603
Contact:
Constantino Panagopulos, costa@ig.utexas.edu, 512-574-7376
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Speaker: Kelly Hereid, Chubb Corp.
Host: Pedro DiNezio
Title: Woolly problems in catastrophe modeling
Abstract: Insurance companies rely on catastrophe models, which simulate thousands of years of natural disasters, to quantify their exposure to extreme events. However, many of these extremes are highly susceptible to impacts from climate change. Here I highlight key emerging research areas in the science of catastrophe modeling that may be influenced by climate change, and how catastrophe modeling can be used to quantify economic impacts on the built environment. The effect of sea level rise on hurricane storm surge, expanding boundaries of hurricane impacts, compound disasters that incorporate extreme rainfall events, and high-resolution hazards with a complex relationship to climate change are all opportunities for climate research to inform risk management practices in the public and private sectors.
De Ford Lecture Series: Zoltan Sylvester
Start:October 31, 2019 at 3:30 pm
End:
October 31, 2019 at 5:00 pm
Location:
JGB 2.324
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UTIG Seminar Series: Tanner Mills, UTIGApril, 19 2024Time: 10:30 AM - 11:30 AMLocation: PRC 196/ROC 1.603 Speaker: Tanner Mills, Postdoctoral Fellow, University of Texas Institute for Geophysics Host: Peter Flemings Title: Predicting greenhouse gas fluxes to the atmosphere from thawing permafrost Abstract: Arctic permafrost is thawing at rapid rates, which threatens to expose large stores of soil organic carbon to microbial degradation. As microbes utilize this carbon source, they produce greenhouse gasses (GHGs; CO2 and CH4) that can be emitted to the atmosphere and act as a positive feedback during future global temperature increases. While the permafrost carbon feedback has received much attention in the literature, little is known about the multiphase flow properties and the temperature dependence of microbial GHG production rates in thawing permafrost, both of which are essential for predicting GHG emissions from permafrost in the future. Flow experiments of synthetic and natural permafrost specimens under frozen conditions and incubations of permafrost samples are being performed to better understand the effective and relative permeabilities and GHG production rates of thawing permafrost soils. These data will be integral in providing new source terms for permafrost and global carbon models. |
Master\'s Thesis PresentationsApril, 19 2024Time: 2:00 PM - 5:00 PMLocation: JGB The Master of Science (MS) degree at the Jackson School of Geosciences is considered to be the professional degree for a career in the Geosciences. This degree is the foundation for students pursuing employment in the petroleum industry, environmental and hydrogeological fields, state and federal government agencies, and other related geoscience fields. Some students also use the MS degree as preparation for pursuing a Ph.D. The Energy & Earth Resources Interdisciplinary program provides the opportunity for students to prepare themselves in management, finance, economics, law and policy leading to analytical and leadership positions in resource-related fields. The private sector and government organizations face a growing need for professionals that can plan, evaluate, and manage complex resource projects, commonly international in scope, which often include partners with a variety of professional backgrounds. As requirements for these degrees, students must present a professional talk on Master\'s Thesis Presentations. |
Hot Science - Cool Talks: \"Humans vs AI\"April, 19 2024Time: 5:30 PM - 8:15 PMLocation: Burdine 106 Advancements in AI have unleashed astonishing capabilities, but it is not magic. Peter Stone reveals his insights into cutting-edge AI and robotics and explores how they may reshape our world. Someday these technologies could win the World Cup, and they are already outperforming the best humans at complex tasks like high-speed racing. |
Planetary Habitability Seminar SeriesApril, 22 2024Time: 1:00 PM - 2:00 PMLocation: PMA 15.216B UT Center for Planetary Systems Habitability Seminar Series. See website for speaker schedule and more details: View Events Join remotely: https://utexas.zoom.us/j/94052130734 In person: Classroom 15.216B, Physics, Math and Astronomy Bldg. UT Austin, Department of Astronomy 2515 Speedway, Stop C1400 Austin, Texas 78712-1205 |
UTIG Discussion Hour: Nicholas Montiel - PhD Talk (UTIG)April, 23 2024Time: 2:00 PM - 3:00 PMLocation: ROC 2.201 |
UTIG Seminar Series: Cornelia Rasmussen, UTIGApril, 26 2024Time: 10:30 AM - 11:30 AMLocation: PRC 196/ROC 1.603 Speaker: Cornelia Rasmussen, Research Associate, University of Texas Institute for Geophysics Host: Krista Soderlund Title: The Emerging Field Of Position-Specific Isotope Analysis: Applications in chemical forensics, exobiology, geo- and environmental sciences Abstract: Complex organics can be found all over our solar system and within each living thing on our planet, be it as part of its physiology or as a contaminant. However, different processes can lead to the formation of chemical identical molecules. This makes answering a number of scientific questions challenging. One example is distinguishing between biotic and abiotic molecules, hence hindering life detection on early Earth but especially on other planetary bodies, such as on Mars, Titan, Enceladus and on meteorites where organics have been detected. Moreover, tracing molecules as they move through the environment can be demanding, yet is essential in studying the flow of organic molecules as well as correlating pollutants with their source. Novel tools to address these challenges are currently being developed. Especially, the emerging field of position-specific isotope analysis is beginning to grant access to the unique intramolecular carbon (13C/12C) isotope fingerprint preserved in complex molecules. This fingerprint can be applied in various scientific disciplines, ranging from forensics to exobiology, geo- and environmental sciences, including geo health. Nuclear magnetic resonance spectroscopy (NMR) has the potential to become a key player in this research area, as it allows the analysis of organics within complex mixtures, all without the need to fragment the molecule into single carbon units or the combustion of the molecule of interest. We have been developing several NMR tools that allow us to investigate the intramolecular carbon isotope distribution within various molecule classes and to test the central hypothesis that the position-specific carbon isotope distribution within complex organics depends on a molecule’s source and formation history. |
Planetary Habitability Seminar SeriesApril, 29 2024Time: 1:00 PM - 2:00 PMLocation: PMA 15.216B UT Center for Planetary Systems Habitability Seminar Series. See website for speaker schedule and more details: View Events Join remotely: https://utexas.zoom.us/j/94052130734 In person: Classroom 15.216B, Physics, Math and Astronomy Bldg. UT Austin, Department of Astronomy 2515 Speedway, Stop C1400 Austin, Texas 78712-1205 |
UTIG Discussion Hour: Kristian Chan - PhD Talk (UTIG)April, 30 2024Time: 2:00 PM - 3:00 PMLocation: ROC 2.201 |