Thirty-First Annual Summer Intern Conference

Total Page:16

File Type:pdf, Size:1020Kb

Thirty-First Annual Summer Intern Conference Papers Presented at the Thirty-First Annual Summer Intern Conference August 6, 2015 Houston, Texas 2015 Summer Intern Program for Undergraduates Lunar and Planetary Institute Sponsored by Lunar and Planetary Institute NASA Johnson Space Center LPI Contribution No. 1859 Compiled in 2015 by Meeting and Publication Services Lunar and Planetary Institute USRA Houston 3600 Bay Area Boulevard, Houston TX 77058-1113 The Lunar and Planetary Institute is operated by the Universities Space Research Association under a cooperative agreement with the Science Mission Directorate of the National Aeronautics and Space Administration. Any opinions, findings, and conclusions or recommendations expressed in this volume are those of the author(s) and do not necessarily reflect the views of the National Aeronautics and Space Administration. Material in this volume may be copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. HIGHLIGHTS Special Activities Date Activity Location June 1 Lunar Curatorial and Stardust Lab Tour NASA JSC June 11 USRA Family BBQ Picnic USRA/LPI July 9 Meteorite Lab Tour NASA JSC July 16 Human Exploration Research Analog (HERA)/Morpheus NASA JSC July 17 LPI Science Staff Research Presentations USRA/LPI July 20 Annual Safety Training USRA/LPI LPI Summer Intern Program 2015 — Brown Bag Seminars Wednesdays, 12:00 noon–1:00 p.m., USRA/LPI Date Speaker Topic Location June 3 Paul Schenk Dwarf Planets Hess Conference Room June 10 Donn Liddle Virtual Extraterrestrial Samples Hess Conference Room June 17 Justin Simon Protoplanetary Disk Hess Conference Room June 24 David Kring Future Lunar Missions Hess Conference Room July 1 LPI Interns Mid-Term Intern Reports Hess Conference Room July 7 Don Pettit Living and Working in Space Lecture Hall July 8 Walter Kiefer Planetary Interiors Hess Conference Room July 15 Buck Sharpton Impact Cratering Hess Conference Room July 22 Steve Clifford Water on Mars Hess Conference Room July 29 Aaron Burton Meteorite Organics Hess Conference Room August 6 Andy Shaner Education and Public Outreach Hess Conference Room LPI Summer Intern Tag Up and Science Fiction Film Series Thursdays, 6:30 p.m., USRA/LPI Date Title Location June 11 Sunshine Hess Conference Room June 16 When Worlds Collide Hess Conference Room June 18 Forbidden Planet Hess Conference Room June 23 Dark City Hess Conference Room June 25 The Core Hess Conference Room July 2 Close Encounters of the Third Kind Hess Conference Room July 9 Fish Story Hess Conference Room AGENDA 8:00 a.m. BREAKFAST 8:25 a.m. Introductory Remarks by Drs. Stephen Mackwell, Paul Spudis, and David Draper 8:30 a.m. TIMOTHY CAO, University of California, Merced (Advisors: Aaron Burton and Keiko Nakamura-Messenger) Nanometer and Milligram Scale Analyses of Organics in CR Chondrites [#4007] 8:50 a.m. CHRISTOPHER DONALDSON, University of Colorado Boulder (Advisor: Paul Niles) Ultra-Low Temperature Acid Alteration of Silicates [#4009] 9:10 a.m. ROBERT TREVOR GOLDMAN, Pomona College (Advisor: Walter Kiefer) Constraining Lunar Thermal Evolution with Gravity Models of Elastic Flexure of Impact Basin Rim Topography [#4008] 9:30 a.m. MYA ANN HABERMANN, University of Georgia (Advisors: Asmaa Boujibar, Kevin Righter, and Lisa Danielson) Partitioning of U, Th, and K Between Silicate and Metal Under Reducing Conditions: Implications for Mercury’s Differentiation [#4003] 9:50 a.m. JESSICA MARIE JOHNSON, Central Connecticut State University (Advisors: Mike Zolensky and David Kring) A Mineralogic and Petrographic Investigation of Unique Foreign Clasts in 3 Ordinary Chondrite Samples [#4004] 10:10 a.m. ELEANOR CARMEN MCINTOSH, University of South Carolina (Advisors: Jennifer Rapp and Dave Draper) Rare Earth Element Partitioning in Lunar Minerals: An Experimental Study [#4012] 10:30 a.m. BREAK 10:40 a.m. ALEXANDRA BOBIAK NAGURNEY, Lafayette College (Advisors: Allan Treiman and Paul Spudis) Petrology, Bulk Composition, and Provenance of Meteorite NWA5000 [#4002] 11:00 a.m. PATRICK RICHARD PHELPS, University of Tulsa (Advisor: David Kring) LL-Chondrite DOM-10092: A Shock-Metamorphosed Sample from an Impact-Modified Asteroid [#4010] 11:20 a.m. MALGORZATA URSZULA SLIZ, The University of Manchester (Advisor: Paul Spudis) Geology of the Deposits of the Lunar Crisium Basin [#4001] 11:40 a.m. JOANNA SZCZESZEK, Adam Mickiewicz University in Poznań (Advisors: Paul Byrne, Francesca Scipioni, Trudi Hoogenboom, and Paul Schenk) Characterizing Rayed Craters on Mercury and Ganymede [#4005] 12:00 p.m. CHRISTIAN TAI UDOVICIC, University of Toronto (Advisors: Georgiana Kramer and Erika Harnett) Lunar Swirls: Insights from Particle Tracking Simulations at Mare Marginis and NW of Apollo [#4011] 12:20 p.m. ALLISON VANCE, Beloit College (Advisors: Roy Christoffersen and Lindsay Keller) Evolution of Shock Melt Compositions in Lunar Regoliths [#4006] 12:40 p.m. LUNCH CONTENTS Nanometer and Milligram Scale Analyses of Organics in CR Chondrites T. D. Cao , K. Nakamura-Messenger , A. S. Burton , and E. L. Berger ................................. 1 Ultra-Low Temperature Acid Alteration of Silicates C. Donaldson and P. B. Niles ................................................................................................ 4 Constraining Lunar Thermal Evolution with Gravity Models of Elastic Flexure of Impact Basin Rim Topography R. T. Goldman and W. S. Kiefer ............................................................................................ 7 Partitioning of U, Th, and K Between Silicate and Metal Under Reducing Conditions: Implications for Mercury’s Differentiation M. Habermann , A. Boujibar , K. Righter , and L. Danielson ................................................ 10 A Mineralogic and Petrographic Investigation of Unique Foreign Clasts in 3 Ordinary Chondrite Samples J. M. Johnson , M. E. Zolensky , Q. Chan , and D. A. Kring .................................................. 13 Rare Earth Element Partitioning in Lunar Minerals: An Experimental Study E. C. McIntosh , J. F. Rapp , and D. S. Draper ...................................................................... 16 Petrology, Bulk Composition, and Provenance of Meteorite NWA5000 A. B. Nagurney , A. H. Treiman , and P. D. Spudis ................................................................ 19 LL-Chondrite DOM-10092: A Shock-Metamorphosed Sample from an Impact-Modified Asteroid P. R. Phelps and D. A. Kring ................................................................................................ 22 Geology of the Deposits of the Lunar Crisium Basin M. U. Sliz and P. D. Spudis ................................................................................................... 25 Characterizing Rayed Craters on Mercury and Ganymede J. Szczeszek , T. Hoogenboom , F. Scipioni , P. Schenk , K. Johnson , and P. Byrne ............. 28 Lunar Swirls: Insights from Particle Tracking Simulations at Mare Marginis and NW of Apollo C. J. Tai Udovicic , G. Y. Kramer , and E. M. Harnett ........................................................... 31 Evolution of Shock Melt Compositions in Lunar Regoliths A. M. Vance , R. Christoffersen , and L. P. Keller .................................................................. 34 31st Annual Summer Intern Conference (2015) 1 NANOMETER AND MILLIGRAM SCALE ANALYSES OF ORGANICS IN CR CHONDRITES T. D. Cao1, K. Nakamura-Messenger2, A. S. Burton2, E. L. Berger3 1University of California, Merced, CA, tcao6@uc- merced.edu, 2Astromaterials Research and Exploration Science Division, NASA Johnson Space Center, Houston, TX, 3GeoControl Systems Inc – Jacobs JETS contract, NASA Johnson Space Center, Houston, TX, USA Introduction: Primitive carbonaceous chondrites con- minimal aqueous alteration [3]. There have been no or- tain a wide range of organic material, ranging from sol- ganic studies reported in the literature for these speci- uble discrete molecules to insoluble nanoglobules of mens. They have relatively large available masses of macromolecular carbon. The relationship between the ~130 g (MIL 090657, 19) and ~485 g (BUC 10933, 11), soluble organic molecules, macromolecular organic ma- making sufficient masses available for soluble organic terial, and host minerals are poorly understood. Due to extraction. We acquired total mass of 1 g for each me- the differences in extractability of soluble and insoluble teorite sample in our study. organic materials, analysis methods for each differ from Sample Preparation and Analysis Method: each other and are often performed independently. The Insoluble Organic Material Study: To prepare samples combination of soluble and insoluble analyses can pro- for both SEM and TEM analyses, fine grained dark frag- vide a wider understanding on spatial distribution, and ments (50 – 100 µm) were carefully selected from each elemental, structural and isotopic composition of or- of the two specimen’s matrices under a stereomicro- ganic material in primitive meteorites. Furthermore, scope. Matrix fragments were then embedded in low- they can provide wider perspective on how extraterres- viscosity epoxy resins. Thin sections of 70-100 nm- trial organic materials potentially contributed to the syn- thickness were prepared using ultramicrotomy and de- thesis of life’s essential compounds such as amino acids, posited on TEM grids. Bright and dark-field imaging sugar acids, activated
Recommended publications
  • SOLAR ECLIPSE NEWSLETTER SOLAR ECLIPSE November 2003 NEWSLETTER
    Volume 8, Issue 11 SOLAR ECLIPSE NEWSLETTER SOLAR ECLIPSE November 2003 NEWSLETTER The sole Newsletter dedicated to Solar Eclipses INDEX 2 SECalendar November Dear SENL reader, 6 Artis planetarium 6 CNN tonight 6 Antiquity of 'Dragon's Head and Tail' When we are finishing this newsletter, some of the die 7 New Sony videocamera with 3 Megapixel CCD hards are on its way to observe the total solar eclipse 8 Total irradiance graph 9 Eclipse retrocalculations of 23 November 2003. Indeed, some of the eclipse 10 Saros 139/144 and 129/134 chasers left with the icebreaker from South Africa to- 11 Question about eclipse seasons 11 Virus wards the Antarctic. Hopefully they will have a safe 11 Nasa Eclipse Site CD journey and we hope of course a safe return. 11 Picture Logo NASA WebPages 12 Fast question...... Many others will leave for Australia and will observe the 13 "Our Mr. Sun" 13 An eclipse/transit calculator for your mobile phone! eclipse from the air. We wish them of course all suc- 14 3d pix of eclipse cess with the observations of the eclipse. Hopefully we 15 25 october Mercury occultation by new moon 16 Giant sunspot approaching the Sun's centre will see some nice images of the eclipses, and their ac- 16 Live solar images , and northern lights counts in a few weeks time. 17 Satellites eclipsed 18 New Moon Oct 2003 The total lunar eclipse is another challenge for this 19 NASA Scientist Dives Into Perfect Space Storm 20 On the shortest time lap between tw o totalities in the same month.
    [Show full text]
  • Applications of Solar Wind Particle Impact Simulations at Lunar Magnetic Anomalies to the Study of Lunar Swirls
    47th Lunar and Planetary Science Conference (2016) 2648.pdf APPLICATIONS OF SOLAR WIND PARTICLE IMPACT SIMULATIONS AT LUNAR MAGNETIC ANOMALIES TO THE STUDY OF LUNAR SWIRLS. C. J. Tai Udovicic1, G. Y. Kramer2, and E. M. Harnett3, 1Dept of Earth Sciences, University of Toronto, 22 Russell St, Toronto, ON, Canada, ([email protected]), 2Lunar and Planetary Institute, 3600 Bay Area Bvld, Houston, TX, ([email protected]), 3University of Washington, Earth and Space Sciences, Seattle, WA ([email protected]). Introduction: Lunar swirls are high albedo features highlands often appear to have swirl-like anomalies due that exhibit low spectral maturity. They have been to their complicated topography. To mitigate this, we identified at various sites on the Moon, and all coincide generated a slope map from the WAC GLD100 (SLP), with a lunar magnetic anomaly (magnomaly) [1], which we overlayed with the WAC 643 nm normalized although not all magnomalies have an identifiable swirl. reflectance image to distinguish high albedo swirls from The leading hypothesis for lunar swirl origin is high albedo slopes. Even so, after one pass of the region, presented in [2] as magnetic field standoff of the solar only about half of the swirls could be detected with this wind which causes uneven space weathering at the swirl method alone. The remaining half were found after surface. This hypothesis fails to explain why lunar using particle simulations as a guide. swirls are observed at some but not all of the magnetic Solar wind particle tracking simulations: We anomalies present on the Moon. To investigate the solar used the 2D solar wind particle tracking simulation wind standoff hypothesis further and to improve swirl presented in [2].
    [Show full text]
  • Apollo 17 Index: 70 Mm, 35 Mm, and 16 Mm Photographs
    General Disclaimer One or more of the Following Statements may affect this Document This document has been reproduced from the best copy furnished by the organizational source. It is being released in the interest of making available as much information as possible. This document may contain data, which exceeds the sheet parameters. It was furnished in this condition by the organizational source and is the best copy available. This document may contain tone-on-tone or color graphs, charts and/or pictures, which have been reproduced in black and white. This document is paginated as submitted by the original source. Portions of this document are not fully legible due to the historical nature of some of the material. However, it is the best reproduction available from the original submission. Produced by the NASA Center for Aerospace Information (CASI) Preparation, Scanning, Editing, and Conversion to Adobe Portable Document Format (PDF) by: Ronald A. Wells University of California Berkeley, CA 94720 May 2000 A P O L L O 1 7 I N D E X 7 0 m m, 3 5 m m, A N D 1 6 m m P H O T O G R A P H S M a p p i n g S c i e n c e s B r a n c h N a t i o n a l A e r o n a u t i c s a n d S p a c e A d m i n i s t r a t i o n J o h n s o n S p a c e C e n t e r H o u s t o n, T e x a s APPROVED: Michael C .
    [Show full text]
  • Simulations of Particle Impact at Lunar Magnetic Anomalies and Comparison with Spectral Observations
    Simulations of Particle Impact at Lunar Magnetic Anomalies and Comparison with Spectral Observations Erika Harnett∗ Department of Earth and Space Science, University of Washington,Seattle, WA 98195-1310, USA Georgiana Kramer Lunar and Planetary Institute, 3600 Bay Area Blvd, Houston, TX 77058, USA Christian Udovicic Department of Physics, University of Toronto, 60 St George St,Toronto, ON M5S 1A7, Canada Ruth Bamford RAL Space, STFC, Rutherford Appleton Laboratory,Chilton, Didcot Ox11 0Qx, UK (Dated: November 5, 2018) Ever since the Apollo era, a question has remained as to the origin of the lunar swirls (high albedo regions coincident with the regions of surface magnetization). Different processes have been proposed for their origin. In this work we test the idea that the lunar swirls have a higher albedo relative to surrounding regions because they deflect incoming solar wind particles that would otherwise darken the surface. 3D particle tracking is used to estimate the influence of five lunar magnetic anomalies on incoming solar wind. The regions investigated include Mare Ingenii, Gerasimovich, Renier Gamma, Northwest of Apollo and Marginis. Both protons and electrons are tracked as they interact with the anomalous magnetic field and impact maps are calculated. The impact maps are then compared to optical observations and comparisons are made between the maxima and minima in surface fluxes and the albedo and optical maturity of the regions. Results show deflection of slow to typical solar wind particles on a larger scale than the fine scale optical, swirl, features. It is found that efficiency of a particular anomaly for deflection of incoming particles does not only scale directly with surface magnetic field strength, but also is a function of the coherence of the magnetic field.
    [Show full text]
  • Astronomy an Overview
    Astronomy An overview PDF generated using the open source mwlib toolkit. See http://code.pediapress.com/ for more information. PDF generated at: Sun, 13 Mar 2011 01:29:56 UTC Contents Articles Main article 1 Astronomy 1 History 18 History of astronomy 18 Archaeoastronomy 30 Observational astronomy 56 Observational astronomy 56 Radio astronomy 61 Infrared astronomy 66 Visible-light astronomy 69 Ultraviolet astronomy 69 X-ray astronomy 70 Gamma-ray astronomy 86 Astrometry 90 Celestial mechanics 93 Specific subfields of astronomy 99 Sun 99 Planetary science 123 Planetary geology 129 Star 130 Galactic astronomy 155 Extragalactic astronomy 156 Physical cosmology 157 Amateur astronomy 164 Amateur astronomy 164 The International Year of Astronomy 2009 170 International Year of Astronomy 170 References Article Sources and Contributors 177 Image Sources, Licenses and Contributors 181 Article Licenses License 184 1 Main article Astronomy Astronomy is a natural science that deals with the study of celestial objects (such as stars, planets, comets, nebulae, star clusters and galaxies) and phenomena that originate outside the Earth's atmosphere (such as the cosmic background radiation). It is concerned with the evolution, physics, chemistry, meteorology, and motion of celestial objects, as well as the formation and development of the universe. Astronomy is one of the oldest sciences. Prehistoric cultures left behind astronomical artifacts such as the Egyptian monuments and Stonehenge, and early civilizations such as the Babylonians, Greeks, Chinese, Indians, and Maya performed methodical observations of the night sky. However, the invention of the telescope was required before astronomy was able to develop into a modern science. Historically, astronomy A giant Hubble mosaic of the Crab Nebula, a supernova remnant has included disciplines as diverse as astrometry, celestial navigation, observational astronomy, the making of calendars, and even astrology, but professional astronomy is nowadays often considered to be synonymous with astrophysics.
    [Show full text]
  • Abd Al-Rahman Al-Sufi and His Book of the Fixed Stars: a Journey of Re-Discovery
    ResearchOnline@JCU This file is part of the following reference: Hafez, Ihsan (2010) Abd al-Rahman al-Sufi and his book of the fixed stars: a journey of re-discovery. PhD thesis, James Cook University. Access to this file is available from: http://eprints.jcu.edu.au/28854/ The author has certified to JCU that they have made a reasonable effort to gain permission and acknowledge the owner of any third party copyright material included in this document. If you believe that this is not the case, please contact [email protected] and quote http://eprints.jcu.edu.au/28854/ ′Abd al-Raḥmān al-Ṣūfī and His Book of the Fixed Stars: A Journey of Re-discovery Thesis submitted by Ihsan Hafez In October 2010 For the degree of Doctor of Philosophy In the School of Engineering and Physical Sciences James Cook University STATEMENT OF ACCESS I, the undersigned, author of this work, understand that James Cook University will make this thesis available for use within the University Library and, via the Australian Digital Theses network, for use elsewhere. I understand that, as an unpublished work, a thesis has significant protection under the Copyright Act and; I do not wish to place any further restriction on access to this work. Signature: Date: I STATEMENT OF SOURCES DECLARATION I declare that this thesis is my own work and has not been submitted in any form for another degree or diploma at any university or other institution of tertiary education. Information derived from the published or unpublished work of others has been acknowledged in the text and a list of references is given.
    [Show full text]
  • Mission Requirements J-1 Type Mission
    MSC-02575 NASA National Aeronautics and Space Administration MISSION REQUIREMENTS J-1 TYPE MISSION January 4, 1971 Contract NAS 9-8166 i MSC-02575 MISSION REQUIREMENTS J-1 TYPE MISSION Contract NAS 9-8166 Prepared by TRW Systems for Systems Engineering Division Apollo Spacecraft Program Office Manned Spacecraft Center Houston, Texas Submitted byb741~ IJames M. Peacock Mission Staff Engineer Approved by Ronald L. Kubicki, Acting Chief Systems Engineering Division Approved by Concurrence ~8Xi!Ile~~~-~ ~Faget, Director p- . Engineering and Development Concurrence Concurrence Science Concurrenc~~ /?J,}>.. Charles A. Berry, rector Medical Research and Operations iii CCBD ECP DATE NUMI:IERS NUMBERS MANNED SPACECRAFT CENTER PCN PROGRAM OFFICE 22 July 197 CONFIGURATION MSC 1C0302 CONTROL BOARD DIRECTIVE CHANGE PRIORITY PAGE 1 1 IMPACT ON 0 CSM 0 LM 0 GFE 0 LV 0 LF 0 EXP OF 0 GSE 0 OTHER MSFC CHANGE TITLE KSC Change C to MSC-02575 NOMENCLATURE AND PART NO. OF AFFECTED END ITEM CHANGE IMPACT SUt+IARY Mission Requirements, J-1 Type Mission, Lunar Landing GSE 0 PRODUCTION EFFECTIVITY MODIFICATION EFFECTIVITY SPARES 0 TRAINERS 0 ESTIMATED COST SOFTWARE 0 FY71 J FY72 FY73 ITOTAL FLIGHT PROGRAMS 0 None None None RTCC PROGRAMS 0 SCHEDULE IMPACT AOH 0 None 'STOWAGE LIST 0 DISPOSITION AND DIRECTED ACTION: COMAT 0 CHANGE TO BE IMPLEMlNTED ONLY WHEN All INTERFACE ACTIONS HAVE BEEN AUTHORIZED TCRD 0 •The Test Conditions for objectives EVA Communications ERD 0 With the LCRU/GCTA, CM Photographic Tasks and Visual RETEST 0 Light Flash Phenomenon are modified. OTHER 0 •The Composite Casting in-flight demonstration is deleted. WEIGHT •The LM ascent stage lunar impact coordinates are LM changed.
    [Show full text]