PSI Scienst Shows Evidence of Supervolcano on Mars
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Planetary Geologic Mappers Annual Meeting
Program Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 Planetary Geologic Mappers Annual Meeting June 12–14, 2018 • Knoxville, Tennessee Institutional Support Lunar and Planetary Institute Universities Space Research Association Convener Devon Burr Earth and Planetary Sciences Department, University of Tennessee Knoxville Science Organizing Committee David Williams, Chair Arizona State University Devon Burr Earth and Planetary Sciences Department, University of Tennessee Knoxville Robert Jacobsen Earth and Planetary Sciences Department, University of Tennessee Knoxville Bradley Thomson Earth and Planetary Sciences Department, University of Tennessee Knoxville Abstracts for this meeting are available via the meeting website at https://www.hou.usra.edu/meetings/pgm2018/ Abstracts can be cited as Author A. B. and Author C. D. (2018) Title of abstract. In Planetary Geologic Mappers Annual Meeting, Abstract #XXXX. LPI Contribution No. 2066, Lunar and Planetary Institute, Houston. Guide to Sessions Tuesday, June 12, 2018 9:00 a.m. Strong Hall Meeting Room Introduction and Mercury and Venus Maps 1:00 p.m. Strong Hall Meeting Room Mars Maps 5:30 p.m. Strong Hall Poster Area Poster Session: 2018 Planetary Geologic Mappers Meeting Wednesday, June 13, 2018 8:30 a.m. Strong Hall Meeting Room GIS and Planetary Mapping Techniques and Lunar Maps 1:15 p.m. Strong Hall Meeting Room Asteroid, Dwarf Planet, and Outer Planet Satellite Maps Thursday, June 14, 2018 8:30 a.m. Strong Hall Optional Field Trip to Appalachian Mountains Program Tuesday, June 12, 2018 INTRODUCTION AND MERCURY AND VENUS MAPS 9:00 a.m. Strong Hall Meeting Room Chairs: David Williams Devon Burr 9:00 a.m. -
Supervolcanoes Within an Ancient Volcanic Province in Arabia Terra, Mars 2 3 4 Joseph
EMBARGOED BY NATURE 1 1 Supervolcanoes within an ancient volcanic province in Arabia Terra, Mars 2 3 4 Joseph. R. Michalski 1,2 5 1Planetary Science Institute, Tucson, Arizona 85719, [email protected] 6 2Dept. of Earth Sciences, Natural History Museum, London, United Kingdom 7 8 Jacob E. Bleacher3 9 3NASA Goddard Space Flight Center, Greenbelt, MD, USA. 10 11 12 Summary: 13 14 Several irregularly shaped craters located within Arabia Terra, Mars represent a 15 new type of highland volcanic construct and together constitute a previously 16 unrecognized martian igneous province. Similar to terrestrial supervolcanoes, these 17 low-relief paterae display a range of geomorphic features related to structural 18 collapse, effusive volcanism, and explosive eruptions. Extruded lavas contributed to 19 the formation of enigmatic highland ridged plains in Arabia Terra. Outgassed sulfur 20 and erupted fine-grained pyroclastics from these calderas likely fed the formation of 21 altered, layered sedimentary rocks and fretted terrain found throughout the 22 equatorial region. Discovery of a new type of volcanic construct in the Arabia 23 volcanic province fundamentally changes the picture of ancient volcanism and 24 climate evolution on Mars. Other eroded topographic basins in the ancient Martian 25 highlands that have been dismissed as degraded impact craters should be 26 reconsidered as possible volcanic constructs formed in an early phase of 27 widespread, disseminated magmatism on Mars. 28 29 30 EMBARGOED BY NATURE 2 31 The source of fine-grained, layered deposits1,2 detected throughout the equatorial 32 region of Mars3 remains unresolved, though the deposits are clearly linked to global 33 sedimentary processes, climate change, and habitability of the surface4. -
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Understanding the History of Arabia Terra, Mars Through Crater-Based Tests Karalee Brugman University of Colorado Boulder
University of Colorado, Boulder CU Scholar Undergraduate Honors Theses Honors Program Spring 2014 Understanding the History of Arabia Terra, Mars Through Crater-Based Tests Karalee Brugman University of Colorado Boulder Follow this and additional works at: http://scholar.colorado.edu/honr_theses Recommended Citation Brugman, Karalee, "Understanding the History of Arabia Terra, Mars Through Crater-Based Tests" (2014). Undergraduate Honors Theses. Paper 55. This Thesis is brought to you for free and open access by Honors Program at CU Scholar. It has been accepted for inclusion in Undergraduate Honors Theses by an authorized administrator of CU Scholar. For more information, please contact [email protected]. ! UNDERSTANDING+THE+HISTORY+OF+ARABIA+TERRA,+MARS++ THROUGH+CRATER4BASED+TESTS+ Karalee K. Brugman Geological Sciences Departmental Honors Thesis University of Colorado Boulder April 4, 2014 Thesis Advisor Brian M. Hynek | Geological Sciences Committee Members Charles R. Stern | Geological Sciences Fran Bagenal | Astrophysical and Planetary Sciences Stephen J. Mojzsis | Geological Sciences ABSTRACT' Arabia Terra, a region in the northern hemisphere of Mars, has puzzled planetary scientists because of its odd assemblage of characteristics. This makes the region difficult to categorize, much less explain. Over the past few decades, several hypotheses for the geological history of Arabia Terra have been posited, but so far none are conclusive. For this study, a subset of the Mars crater database [Robbins and Hynek, 2012a] was reprocessed using a new algorithm [Robbins and Hynek, 2013]. Each hypothesis’s effect on the crater population was predicted, then tested via several crater population characteristics including cumulative size-frequency distribution, depth-to-diameter ratio, and rim height. -
Overview of SPRITE: Saturn Probe Interior and Atmosphere Explorer Concept
Overview of SPRITE: Saturn PRobe Interior and aTmosphere Explorer Concept Marcus Lobbia1 Co-Authors: Amy Simon2, Rolf Danner1, Dave Atkinson1, Cavan Cuddy3 1 Jet Propulsion Laboratory, California Institute of Technology 2 NASA Goddard Space Flight Center 3 Lockheed Martin Space Systems © 2017 California Institute of Technology. Government sponsorship acknowledged. Predecisional information for planning and discussion only Saturn Probe Mission Concept – Decadal Survey • Planetary Sciences Decadal Survey – Saturn Probe mission one of several recommended Medium-class missions for New Frontiers program • Objectives – 1: Determine Saturn’s Role in Solar System Formation and Evolution • Measure noble gas abundances and isotopic ratios in Saturn’s atmosphere – 2: Characterize Saturn’s atmosphere structure and composition • Measure atmospheric structure and cloud properties at Probe descent location SPRITE is proposed as a New Frontiers candidate mission to address these high-priority Decadal Survey objectives Predecisional information for planning and discussion only 2 jpl.nasa.gov Saturn’s Role in Solar System Formation • Did Saturn arrest Jupiter migration to inner solar system? – In situ measurements will help identify Saturn’s age and formation location – Sample elemental abundances and isotopic ratios from 0.2 to 10 bars pressure Predecisional information for planning and discussion only 3 jpl.nasa.gov Truth Beneath Saturn’s Clouds • What are the properties and locations of Saturn’s various cloud layers? What are vertical profiles of pressure, -
Harvesting Electromagnetic Energy from Hypervelocity Impacts for Solar System Exploration
URSI GASS 2020, Rome, Italy, 29 August - 5 September 2020 Harvesting Electromagnetic Energy from Hypervelocity Impacts for Solar System Exploration Sean A. Q. Young*(1), Nicolas Lee(1), and Sigrid Close(1) (1) Department of Aeronautics & Astronautics, Stanford University, Stanford, California, USA, 94305 Abstract CubeSats have opened new opportunities for solar system exploration by decreasing mission development and launch costs. While they have proven successful in the inner so- lar system, providing sustained power to these spacecraft Figure 1. Graphical representation of the HVI energy har- at large distances from the sun requires novel power gener- vesting concept. ation methods. Solar power is dramatically diminished at these distances and radioisotope thermoelectric generators do not scale well to spacecraft with small dimensions. The CubeSats as free-flying sensors can produce plasma mea- space environment could provide a solution; by harnessing surements spread over hundreds of kilometers — a signif- energetic hazards in the environments under investigation, icant improvement over the tens of meters that a boom- the spacecraft could forgo traditional power sources. Radio mounted sensor would provide. This concept has heritage frequency emissions are abundant in the space environment in the Cluster [1] mission for example. with sources originating from planetary aurora, particle dy- namics in the magnetosphere, and electromagnetic pulses Power presents a challenge to small spacecraft in the outer (EMPs) associated with hypervelocity impacts between mi- solar system. The extreme distance from the sun precludes crometeoroids and spacecraft. A case study of a mission the use of solar panels for Cubesats, and radioisotope ther- to the rings of Saturn is presented and analyzed for feasi- moelectric generators are expensive, difficult to handle, and bility. -
Krista Marie Soderlund the University of Texas at Austin Institute for Geophysics, John A
Krista Marie Soderlund The University of Texas at Austin Institute for Geophysics, John A. & Katherine G. Jackson School of Geosciences J.J. Pickle Research Campus, Bldg. 196 (ROC), 10100 Burnet Rd. (R2200), Austin, TX 78758-4445 [email protected], Office: 512-471-0449, Cell: 218-349-3006, FAX: 512-471-8844 Research Interests Geophysical Fluid Dynamics, Magnetohydrodynamics, Planetary Science, Cryosphere Education University of California, Los Angeles Ph.D., Geophysics and Space Physics, 2011 M.S., Geophysics and Space Physics, 2009 Florida Institute of Technology B.S., Double major in Physics & Space Science, 2005, Summa Cum Laude Employment University of Texas at Austin, Institute for Geophysics Research Associate, September 2014-Present UTIG Postdoctoral Fellow, October 2011-September 2014 University of California, Los Angeles, Department of Earth and Space Sciences Graduate Student Researcher, Advisor: Dr. Jonathan M. Aurnou, 2006-2011 California Institute of Technology, Division of Geological and Planetary Sciences Summer Undergraduate Research Fellow, Dr. Joann M. Stock, 2005 NASA Jet Propulsion Laboratory, CA Consultant, Dr. Bonnie J. Buratti, 2006 Planetary Geology & Geophysics Undergrad Research Program, Dr. B.J. Buratti, 2004 Florida Institute of Technology, Department of Physics and Space Science Undergraduate Researcher, Dr. Niescja E. Turner, 2004-2005 Naval Oceanographic Office, Hydrology Code, Stennis Space Center, MS Physical science aid, 2003 Mission Experience Saturn Probe Interior and aTmosphere Explorer (SPRITE) -
Intellectual Culture of the Hudson Bay Eskimos
THE LIBRARY OF YORK UNIVERSITY - _ Date Due »Cim, Aug i ~ RENEWED C AUGbJ 1 1992 (ap Æ 21W FA'tf sc 1 ICS JAN 6 1993 4 s — Mrrt * 06 1995 - ^ tim sCft: sc FA y APR 16 1993 J(Æ s~ — '9Wj scc —RENEWED / «x < " ?99f - _ * : tt! 2sc Gift JUL 1 2 19Vi : > d — OCT 1995 see * l» - APR 27m i)L 1 York Form — Cooper Graphics — v., ffte FOAM 109 Digitized by the Internet Archive in 2014 https://archive.org/details/intellectualcultOOrasm REPORT OF THE FIFTH THULE EXPEDITION 1921—24 THE DANISH EXPEDITION TO ARCTIC NORTH AMERICA IN CHARGE of KNUD RASMUSSEN, ph. d. VOL. VII. NO. 1 INTELLECTUAL CULTURE OF THE IGLULIK ESKIMOS BY KNUD RASMUSSEN GYLDENDALSKE BOGHANDEL, NORDISK FORLAG COPENHAGEN 1929 Edited with the Support of the Ministry of Education. Translation Expenses defrayed by the Rask-Ørsted Fund. Translated by W. WORSTER from the Danish original. PRINTED IN DENMARK GYLDENDALS FORLAOSTRYKKERI KØBENHAVN TO MY FRIEND WILLIAM THALBITZER PROFESSOR OF ESKIMO LANGUAGE AND CULTURE IN THE UNIVERSITY OF COPENHAGEN General Plan and Methods of Work. The work of the Fifth Thule Expedition was divided up between us so that Kaj Birket-Smith and Therkel Mathiassen dealt with the material aspects of the Eskimo culture, while I took the intellectual side. My principal objects of study under this head comprised: 1) The natives in the vicinity of our headquarters at Danish Is- land, or in other words, the Aivilingmiut, Iglulingmiut and the immi- grant Netsilingmiut. The Aivilingmiut and Iglulingmiut constitute, together with the Tununermiut at Ponds Inlet, the Iglulik group. -
Identifying Evidence for Explosive Volcanism on Mars Through Geomorphologic and Thermophysical Observations
IDENTIFYING EVIDENCE FOR EXPLOSIVE VOLCANISM ON MARS THROUGH GEOMORPHOLOGIC AND THERMOPHYSICAL OBSERVATIONS by Gabriel Cecilio Garcia A thesis submitted in partial fulfillment of the requirements for the degree of Master of Science in Geosciences Boise State University May 2018 © 2018 Gabriel Cecilio Garcia ALL RIGHTS RESERVED BOISE STATE UNIVERSITY GRADUATE COLLEGE DEFENSE COMMITTEE AND FINAL READING APPROVALS of the thesis submitted by Gabriel Cecilio Garcia Thesis Title: Identifying Evidence for Explosive Volcanism on Mars through Geomorphologic and Thermophysical Observations Date of Final Oral Examination: 24 January 2018 The following individuals read and discussed the thesis submitted by student Gabriel Cecilio Garcia, and they evaluated his presentation and response to questions during the final oral examination. They found that the student passed the final oral examination. Brittany D. Brand, Ph.D. Chair, Supervisory Committee Joshua L. Bandfield, Ph.D. Member, Supervisory Committee Jennifer L. Pierce, Ph.D. Member, Supervisory Committee The final reading approval of the thesis was granted by Brittany D. Brand, Ph.D., Chair of the Supervisory Committee. The thesis was approved by the Graduate College. DEDICATION I dedicate this thesis to my parents. Their love and support has provided me the opportunity to strive for greatness and live a life that I can truly be proud of. No matter where I go, I will always live by your example. iv ACKNOWLEDGEMENTS I would like to thank my advisors, Brittany Brand and Joshua Bandfield, for all they have helped me with. I would not be the scientist I am now without their guidance and teachings. I would also like to thank the Idaho Space Grant Consortium for funding this research. -
Scientific Rationale for Uranus and Neptune in Situ Explorations
Planetary and Space Science 00 (2017) 1–?? Scientific rationale for Uranus and Neptune in situ explorations O. Mousisa, D. H. Atkinsonb, T. Cavalie´c, L. N. Fletcherd, M. J. Amatoe, S. Aslame, F. Ferrif, J.-B. Renardg, T. Spilkerh, E. Venkatapathyi, P. Wurzj, K. Aplink, A. Coustenisc, M. Deleuila, M. Dobrijevicl, T. Fouchetc, T. Guillotm, P. Hartoghn, T. Hewagamao, M. D. Hofstadterb, V. Huep, R. Huesoq, J.-P. Lebretong, E. Lellouchc, J. Mosesr, G. S. Ortonb, J. C. Pearle, A. Sanchez-Lavega´ q, A. Simone, O. Venots, J. H. Waitep, R. K. Achterbergo, S. Atreyat, F. Billebaudl, M. Blancv, F. Borgetu, B. Bruggera, S. Charnozw, T. Chiavassau, V. Cottinio, L. d’Hendecourtu, G. Dangeru, T. Encrenazc, N. J. P. Goriusx, L. Jordaa, B. Martyy, R. Morenoc, A. Morsez, C. Nixone, K. Rehb, T. Ronneta, F.-X. Schmiderm, S. Sheridanz, C. Sotinb, P. Vernazzaa, G. L. Villanuevae aAix Marseille Universit´e,CNRS, LAM (Laboratoire d’Astrophysique de Marseille) UMR 7326, 13388, Marseille, France bJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Dr., Pasadena, CA 91109, USA c LESIA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universit´es,UPMC Univ. Paris 06, Univ. Paris Diderot, Sorbonne Paris Cit´e,5 place Jules Janssen, 92195 Meudon, France dDepartment of Physics & Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UK eNASA Goddard Space flight Center, Greenbelt, MD 20771, USA fUniversit`adegli Studi di Padova, Centro di Ateneo di Studi e Attivit`aSpaziali “Giuseppe Colombo” (CISAS), via Venezia -
Modern Traveller
THE MODERN TRAVELLER. A POPULAR DESCRIPTION, GEOGRAPHICAL, HISTORICAL, AND TOPOGRAPHICAL, OF THE VARIOUS COUNTRIES OF THE GLOBE. SPAIN AND PORTUGAL. VOL. II. LONDON: PRINTED FOR JAMES DUNCAN; OLIVER AND BOYD, EDINBURGH; M.OGLE, GLASGOW; AND R. M. TIMS, DUBLIN. 1826. m 3. MOYSS, TEMPLE PRINTING OFFICE, EOÜVEEIE STREET. - •••• CONTENTS OP THE SECOND VOLUME. .... SPAIN. PAGE SEVILLE •••• I CORDOVA 35 FROM CORDOVA TO TOLEDO 44 TOLEDO •••••• 50 FROM CORDOVA TO MADRID 59 LA MANCHA 61 ARANJUEZ 71 MADRID 76 THE ESCÜRIAL • Ill FROM MADRID TO SEGOVIA AND BURGOS 126 SAN ILDEFONSO 127 VALLADOLID 134 BURGOS 144 FROM MADRID TO OVIEDO 153 LEON 156 OVIEDO 165 FROM MADRID TO CORUNA 178 SALAMANCA 180 CORUNA 203 FROM MADRID TO LISBON 214 MERIDA 224 / CONTENTS. PAGE BADAJOZ 228 PLASENCIA 238 FROM MADRID TO BAYONNE 248 ZARAGOZA 256 SIEGES OF 1808 AND 1809 261 FROM BURGOS TO BAYONNE 271 PORTUGAL. BOUNDARIES, ANCIENT AND MODERN 287 HISTORY" OF PORTUGAL 288 LISBON • 295 CINTRA ••. 310 SETUBAL •' - • 315 BRAGA • • 324 OPORTO 325 COIMBRA 330 8ATALHA 333 EVORA 340 .. ! DIRECTIONS FOR. PLACING THE PLATES. Vol.. I. MAP of SPAIN to face the Title. PORT of BARCELONA MALL at BARCELONA 92 MONTSERRAT 101 COURT of the LIONS in the ALBAMRA... 241 Vol. II. COSTUME of TOLEDO 50 The ESCURIAL ........................ 124 VIEW of LISBON 295 THE MODERN TRAVELLER, ETC. ETC. SPAIN. SEVILLE. HISPALIS,* the capital of Hispania Baetica, of which Seville is the representative, is mentioned by Strabo, Pomponius Mela, Pliny, and Ptolemy, as being an cient even in their time. It, is supposed to have been founded by the Phenieians,—according to the popular tradition, by Hercules. -
The New Frontiers Saturn Probe Interior and Atmosphere Explorer (SPRITE) Mission Proposal
EPSC Abstracts Vol. 11, EPSC2017-356, 2017 European Planetary Science Congress 2017 EEuropeaPn PlanetarSy Science CCongress c Author(s) 2017 The New Frontiers Saturn PRobe Interior and aTmosphere Explorer (SPRITE) Mission Proposal D. Atkinson (1), A. A. Simon (2), D. Banfield (3), S. Atreya (4), J. Blacksberg (1), W. Brinckerhoff (2), A. Colaprete (5), A. Coustenis (6), L. Fletcher (7), T. Guillot (8), M. Hofstadter (9), J. Lunine (3), P.Mahaffy (2), M. Marley (5), O. Mousis (9), T. Spilker (10), M. Trainer (2), C. Webster (1) (1) Jet Propulsion Laboratory, California Institute of Technology ([email protected]), (2) NASA Goddard Space Flight Center, (3) Cornell University, (4) Univ. Michigan, (5) NASA Ames Research Center, (6) LESIA, Observ. Paris-Meudon, CNRS, Paris Univ., France, (7) Univ. Leicester, (8) Observatoire de la Cote d'Azur CNRS / Laboratoire Cassiopée, (9) Laboratoire d'Astrophysique de Marseille, (10) Independent Consultant Abstract SPRITE is proposed to launch in late November The 2013-2022 Planetary Decadal Survey Vision and 2024 launch and follows an Earth-Venus-Earth-Earth Voyages [1] identified Saturn as a target of high gravity assist trajectory to reach Saturn in November, priority for a New Frontiers probe mission concept. 2034. The SPRITE probe enters Saturn’s atmosphere To better constrain models of Solar System formation, at a relative velocity of ~27 km/s, experiencing a 2 giant planet formation and evolution, and to provide peak heat flux near 3000 W/cm and a peak an improved context for understanding exoplanetary deceleration up to 45 g’s. The aeroshell is released systems, fundamental measurements of Saturn above the tropopause and the descent science including noble gas abundances, isotope ratios of sequence is initiated, permitting up to 2 hours for the hydrogen, carbon, oxygen, and nitrogen, and probe to pass through 10 bars.