DI024
Interiors of Planets and Moons: Learning from Spacecraft Observations, Simulations, and in Situ Data II Posters

Tuesday, 15 December 2020: 04:00-20:59
Poster
Primary Convener:  Renee C Weber, NASA Marshall Space Flight Center, Huntsville, AL, United States
Conveners:  Jessica C E Irving, University of Bristol, School of Earth Sciences, Bristol, BS8, United Kingdom and Ceri Nunn, Jet Propulsion Laboratory, Pasadena, United States
Primary Liaison:  Renee C Weber, NASA Marshall Space Flight Center, Huntsville, AL, United States
Chairs:  Jessica C E Irving, Princeton University, Department of Geosciences, Princeton, NJ, United States, Renee C Weber, NASA/NSSTC, Huntsville, AL, United States and Ceri Nunn, University of Cambridge, Cambridge, United Kingdom
OSPA Liaison:  Jessica C E Irving, Princeton University, Department of Geosciences, Princeton, NJ, United States
 
Lithospheric Thickness and Heat Flow on Venus: Results from a Global Survey of Flexure at Steep-Sided Domes (742176)
Madison Borrelli1, Joseph G O'Rourke1 and Suzanne E Smrekar2, (1)Arizona State University, Tempe, AZ, United States, (2)NASA Jet Propulsion Laboratory, Pasadena, CA, United States
 
Using Impacts to Initiate a Mobile-Lid Regime on Venus (740450)
Grant Euen and Scott D King, Virginia Polytechnic Institute and State University, Blacksburg, VA, United States
 
The Moon as a cornerstone of understanding for terrestrial planetary interiors (663882)
Renee C Weber, NASA Marshall Space Flight Center, Huntsville, AL, United States, Clive Robert Neal, University of Notre Dame, Notre Dame, IN, United States, Nicholas C Schmerr, University of Maryland College Park, College Park, MD, United States, Heidi Haviland, NASA Marshall Space Flight Center, Heliophysics and Planetary Science Branch, Huntsville, AL, United States and Barbara A Cohen, NASA Goddard Space Flight Center, Greenbelt, MD, United States
 
Expanding the Shallow Surface Velocity at the Apollo 17 Landing Site to Determine Thermal Moonquake Locations (709565)
Deanna Phillips, University of Alabama in Huntsville, Huntsville, AL, United States and Renee C Weber, NASA/NSSTC, Huntsville, AL, United States
 
A parameterization model to analyze lunar thermal history and thermal stress for inducing moonquakes (729787)
Sha Tao, UCAS University of Chinese Academy of Sciences, Beijing, China, Yaolin Shi, University of Chinese Academy of Sciences, Beijing, China and Bojing Zhu, Yunnan Astronomical Observatories, Kunming, Yunnan, China
 
The Role of the Nucleation Barrier on Lunar Geodynamo Evolution (740895)
Sara Gutierrez, Case Western Reserve University, Cleveland, OH, United States and Steven A. Hauck, II, Case Western Reserve University, Cleveland, United States
 
New Constraints on the Interior Properties of Mars (701266)
Robert L Huguenin, RLH Scientific, LLC, Groton, MA, United States
 
Insight Low Frequency Seismological Measurements: Environmental Noise Decorrelation And Applicability To Mars Internal Structure Refinement (721253)
Baptiste Pinot1, Raphael F. Garcia2, David Mimoun2, Laurent Pou3, Francis Nimmo4, Aymeric Spiga5, Philippe Henri Lognonné6, Donald J Banfield7, Leo Martire2, Naomi Murdoch8, Nicolas Compaire1 and W Bruce Banerdt9, (1)Institut Supérieur de l'Aéronautique et de l'Espace, Toulouse Cedex 04, France, (2)Institut Supérieur de l'Aéronautique et de l'Espace, DEOS/SSPA, Toulouse Cedex 04, France, (3)University of California Santa Cruz, Earth and Planetary Sciences, Santa Cruz, CA, United States, (4)University of California-Santa Cruz, Earth and Planetary Sciences, Santa Cruz, CA, United States, (5)Laboratoire de Météorologie Dynamique UPMC, Paris, France, (6)Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France, (7)Cornell University, Center for Radiophysics and Space Research, Ithaca, NY, United States, (8)Institut Supérieur de l’Aéronautique et de l’Espace, DEOS/SSPA, Toulouse, France, (9)NASA Jet Propulsion Laboratory, Pasadena, CA, United States
 
S-coda wave analysis of InSight seismic data to determine the scattering and intrinsic attenuation in the crust of Mars (677348)
Foivos Georgios Karakostas1, Nicholas C Schmerr1, Ross Maguire2, Doyeon Kim3, Quancheng Huang4, Taichi Kawamura5, Keisuke Onodera6, Philippe Henri Lognonné7, Domenico Giardini8 and William Bruce Banerdt9, (1)University of Maryland College Park, College Park, MD, United States, (2)University of New Mexico Main Campus, Albuquerque, NM, United States, (3)Cornell University, Ithaca, NY, United States, (4)University of Maryland, Department of Geology, College Park, MD, United States, (5)Université de Paris, Institut de physique du globe de Paris, Paris, France, (6)Université de Paris, Institut de Physique du Globe de Paris, Paris, France, (7)Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France, (8)Swiss Federal Institute of Technology (ETH), Zurich, Switzerland, (9)JPL/NASA/Caltech, Pasadena, CA, United States
 
Detecting the Mantle Transition Zone of Mars From Seismic Triplicated and Reflected Waves (680965)
Quancheng Huang1, Nicholas C. Schmerr2, Ross Maguire1, Daniele Antonangeli3, Benjamin Fernando4, Kuangdai Leng4, Tarje Nissen-Meyer5, Scott D King6, Attilio Rivoldini7, Ana-Catalina Plesa8, Carolina R Lithgow-Bertelloni9, Tamara Gudkova10, Henri Samuel11, Domenico Giardini12, Philippe Henri Lognonné11 and William Bruce Banerdt13, (1)University of Maryland, Department of Geology, College Park, MD, United States, (2)University of Maryland College Park, Department of Geology, College Park, MD, United States, (3)Sorbonne Université - MNHN - CNRS - IMPMC, Paris, France, (4)University of Oxford, Oxford, United Kingdom, (5)University of Oxford, Department of Earth Sciences, Oxford, United Kingdom, (6)Virginia Polytechnic Institute and State University, Blacksburg, VA, United States, (7)Royal Observatory of Belgium, Brussels, Belgium, (8)German Aerospace Center (DLR), Berlin, Germany, (9)University of California Los Angeles, Los Angeles, CA, United States, (10)Schmidt Institute of Physics of the Earth RAS, Moscow, Russia, (11)Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France, (12)Swiss Federal Institute of Technology (ETH), Zurich, Switzerland, (13)JPL/NASA/Caltech, Pasadena, CA, United States
 
Statistical and energetic characteristic of High Frequency (HF) and Very High Frequency (VHF) Martian events (692075)
Sabrina Menina1, Ludovic Margerin2, Taichi Kawamura3, Philippe Henri Lognonné1, Jules Marti2, Melanie Drilleau4, Marie Calvet2, Nicholas C Schmerr5 and Martin van Driel6, (1)Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France, (2)IRAP - Universite de Toulouse, Toulouse, France, (3)Université de Paris, Institut de physique du globe de Paris, Paris, France, (4)Institut Supérieur de l'Aéronautique et de l'Espace, Toulouse Cedex 04, France, (5)University of Maryland College Park, College Park, MD, United States, (6)ETH Zurich, Department of Earth Sciences, Institute of Geophysics, Zurich, Switzerland
 
The seismic moment and seismic efficiency of small impacts on Mars (692446)
Natalia Wojcicka, Imperial College London, London, SW7, United Kingdom, Gareth S Collins, Imperial College London, London, United Kingdom, Ian D Bastow, Imperial College London, Department of Earth Science and Engineering, London, SW7, United Kingdom, Nicholas A Teanby, University of Bristol, Bristol, United Kingdom, Katarina Miljkovic, Curtin University, Perth, Australia, Andrea Rajsic, Curtin University, School of Earth and Planetary Sciences, Perth, Australia, Ingrid Daubar, Brown University, Department of Earth, Environmental and Planetary Sciences, Providence, United States and Philippe Henri Lognonné, Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France
 
Could Some Mars Seismic Events be Generated by Fluid Flow? (699179)
Scott D King1, Sharon Kedar2, Mark P Panning3, Suzanne E Smrekar4, Matthew P Golombek2, Michael Manga5, Bruce R Julian6, Brian Shiro7, Clement Perrin8, John A Power9, Chloe Michaut10, Domenico Giardini11, Simon C Staehler12, Philippe Henri Lognonné13 and William Bruce Banerdt14, (1)Virginia Polytechnic Institute and State University, Blacksburg, VA, United States, (2)JPL, Pasadena, CA, United States, (3)Univ of FL-Geological Sciences, Gainesville, FL, United States, (4)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (5)Univ of California Berkeley, Berkeley, CA, United States, (6)USGS California Water Science Center Menlo Park, Menlo Park, CA, United States, (7)USGS Hawaii Volcano Observatory, Hawaii Natl Park, HI, United States, (8)Université de Paris, Institut de Physique du Globe de Paris, CNRS, Paris, France, (9)USGS, Alaska Volcano Observatory, Anchorage, AK, United States, (10)Institut de Physique du Globe, Paris cedex 13, France, (11)Swiss Federal Institute of Technology (ETH), Zurich, Switzerland, (12)ETH Zurich, Department of Earth Sciences, Institute of Geophysics, Zurich, Switzerland, (13)Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France, (14)JPL/NASA/Caltech, Pasadena, CA, United States
 
Sensitivity of the ancient martian dynamo to hemispheric CMB heat flux patterns (699848)
Chi Yan1, Ankit Barik2, Ana-Catalina Plesa3, Attilio Rivoldini4 and Sabine Stanley2, (1)Johns Hopkins University, Earth and Planetary Science, Baltimore, MD, United States, (2)Johns Hopkins University, Department of Earth and Planetary Sciences, Baltimore, MD, United States, (3)German Aerospace Center (DLR), Berlin, Germany, (4)Royal Observatory of Belgium, Brussels, Belgium
 
Seismic Velocities Distribution in a 3D Mantle: Implications for InSight Measurements (726609)
Ana-Catalina Plesa1, Ebru Bozdag2, Attilio Rivoldini3, Martin Knapmeyer1, Scott M McLennan4, Sebastiano Padovan1, Nicola Tosi1, Doris Breuer1, Daniel B Peter5, Simon C Staehler6, Mark A Wieczorek7, Martin van Driel6, Amir Khan6, Tilman Spohn1,8, Caio Ciardelli2 and Scott D King9, (1)German Aerospace Center DLR Berlin, Berlin, Germany, (2)Colorado School of Mines, Golden, CO, United States, (3)Royal Observatory of Belgium, Brussels, Belgium, (4)Stony Brook University, Stony Brook, NY, United States, (5)King Abdullah University of Science and Technology, Physical Sciences and Engineering, Thuwal, Saudi Arabia, (6)ETH Zurich, Department of Earth Sciences, Institute of Geophysics, Zurich, Switzerland, (7)Observatoire de la Côte d'Azur, Nice, France, (8)International Space Science Institute, Bern, Switzerland, (9)Virginia Polytechnic Institute and State University, Blacksburg, VA, United States
 
Preliminary Analysis of Horizontal to Vertical Spectral Ratio of InSight Seismic Data on Mars (728803)
Wanbo Xiao and Yanbin WANG, Department of Geophysics, Peking University, Beijing, China
 
Constraining marsquake focal mechanisms and martian crustal structure using InSight's seismic data (752199)
Nienke Brinkman1, Simon C Staehler1, Cedric Schmelzbach1, Martin van Driel1, Amir Khan1, John F Clinton2, Brigitte Knapmeyer-Endrun3, Domenico Giardini4, Johan O A Robertsson1, Philippe Henri Lognonné5 and W Bruce Banerdt6, (1)ETH Zurich, Department of Earth Sciences, Institute of Geophysics, Zurich, Switzerland, (2)ETH Swiss Federal Institute of Technology Zurich, Swiss Seismological Service (SED), Zurich, Switzerland, (3)University of Cologne, Bensberg Observatory, Cologne, Germany, (4)Swiss Federal Institute of Technology (ETH), Zurich, Switzerland, (5)Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France, (6)NASA Jet Propulsion Laboratory, Pasadena, CA, United States
 
Evaluating the Thermal and Geochemical Evolution of Mars (771081)
Fiona Clare McGroarty, Virginia Tech, Department of Geosciences, Blacksburg, VA, United States, Megan S Duncan, Virginia Polytechnic Institute and State University, Blacksburg, VA, United States and Matt B Weller, Brown University, Department of Earth, Environmental and Planetary Sciences, Providence, RI, United States