Chapter Vi Report of Divisions, Commissions, and Working
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Observations of Mass Wasting Events in the Cerberus Fossae, Mars
51st Lunar and Planetary Science Conference (2020) 2404.pdf OBSERVATIONS OF MASS WASTING EVENTS IN THE CERBERUS FOSSAE, MARS. C. M. Dundas1, I. J. Daubar, 1U.S. Geological Survey, Astrogeology Science Center, 2255 N. Gemini Dr., Flagstaff, AZ 86001 ([email protected]), 2Brown University. Introduction: The Cerberus Fossae are a set of ge- Rockfall tracks are observed at several locations. ologically-young, steep-sided fissures in the Elysium These include both simPle falls and large events break- region of Mars, which aPPear to have been the source of ing into many individual tracks (Fig. 2). floods of both water and lava [e.g., 1–4]. They have also been proposed as the site of recent seismically-triggered mass wasting [5–6]. The latter Possibility is of Particular interest because the fossae are in the same region as the InSight lander and may be tectonically active [7-8]. This abstract reports on observations of active mass move- ment in and near the Cerberus Fossae using before-and- after comparisons of images acquired by the High Res- olution Imaging Science Experiment (HiRISE) [9]. Observations: Thirty-six locations were analyzed, mostly covering the Cerberus Fossae but also including some nearby craters and massifs. SloPe activity of some form was observed at ten of these locations, although in some cases it is minor. The observed mass wasting near the fossae can be divided into three categories: slope streaks [cf. 10], sloPe lineae, and rockfalls. Slope lineae in the fossae were Previously described [11–12]. Recent observations confirm that some of the lineae in the Cer- berus Fossae grow incrementally (Fig. -
JUICE Red Book
ESA/SRE(2014)1 September 2014 JUICE JUpiter ICy moons Explorer Exploring the emergence of habitable worlds around gas giants Definition Study Report European Space Agency 1 This page left intentionally blank 2 Mission Description Jupiter Icy Moons Explorer Key science goals The emergence of habitable worlds around gas giants Characterise Ganymede, Europa and Callisto as planetary objects and potential habitats Explore the Jupiter system as an archetype for gas giants Payload Ten instruments Laser Altimeter Radio Science Experiment Ice Penetrating Radar Visible-Infrared Hyperspectral Imaging Spectrometer Ultraviolet Imaging Spectrograph Imaging System Magnetometer Particle Package Submillimetre Wave Instrument Radio and Plasma Wave Instrument Overall mission profile 06/2022 - Launch by Ariane-5 ECA + EVEE Cruise 01/2030 - Jupiter orbit insertion Jupiter tour Transfer to Callisto (11 months) Europa phase: 2 Europa and 3 Callisto flybys (1 month) Jupiter High Latitude Phase: 9 Callisto flybys (9 months) Transfer to Ganymede (11 months) 09/2032 – Ganymede orbit insertion Ganymede tour Elliptical and high altitude circular phases (5 months) Low altitude (500 km) circular orbit (4 months) 06/2033 – End of nominal mission Spacecraft 3-axis stabilised Power: solar panels: ~900 W HGA: ~3 m, body fixed X and Ka bands Downlink ≥ 1.4 Gbit/day High Δv capability (2700 m/s) Radiation tolerance: 50 krad at equipment level Dry mass: ~1800 kg Ground TM stations ESTRAC network Key mission drivers Radiation tolerance and technology Power budget and solar arrays challenges Mass budget Responsibilities ESA: manufacturing, launch, operations of the spacecraft and data archiving PI Teams: science payload provision, operations, and data analysis 3 Foreword The JUICE (JUpiter ICy moon Explorer) mission, selected by ESA in May 2012 to be the first large mission within the Cosmic Vision Program 2015–2025, will provide the most comprehensive exploration to date of the Jovian system in all its complexity, with particular emphasis on Ganymede as a planetary body and potential habitat. -
A Handbook of Citation Form for Law Clerks at the Appellate Courts of the State of Hawai#I
A HANDBOOK OF CITATION FORM FOR LAW CLERKS AT THE APPELLATE COURTS OF THE STATE OF HAWAI ###I 2008 Edition Hawai #i State Judiciary 417 South King Street Honolulu, HI 96813 TABLE OF CONTENTS I. CASES............................................ .................... 2 A. Basic Citation Forms ............................................... 2 1. Hawai ###i Courts ............................................. 2 a. HAWAI #I SUPREME COURT ............................... 2 i. Pre-statehood cases .............................. 2 ii. Official Hawai #i Reports (volumes 1-75) ............. 3 iii. West Publishing Company Volumes (after 75 Haw.) . 3 b. INTERMEDIATE COURT OF APPEALS ........................ 3 i. Official Hawai #i Appellate Reports (volumes 1-10) . 3 ii. West Publishing Company Volumes (after 10 Haw. App.) .............................................. 3 2. Federal Courts ............................................. 4 a. UNITED STATES SUPREME COURT ......................... 4 b. UNITED STATES COURTS OF APPEALS ...................... 4 c. DISTRICT COURTS ...................................... 4 3. Other State Courts .......................................... 4 B. Case Names ................................................... 4 1. Case Names in Textual Sentences .............................. 5 a. ACTIONS AND PARTIES CITED ............................ 5 b. PROCEDURAL PHRASES ................................. 5 c. ABBREVIATIONS ....................................... 5 i. in textual sentences .............................. 5 ii. business -
Naming the Extrasolar Planets
Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named. -
A Systematic Concept Exploration Methodology Applied to Venus in Situ Explorer
Session III: Probe Missions to the Giant Planets, Titan and Venus A Systematic Concept Exploration Methodology Applied to Venus In Situ Explorer Jarret M. Lafleur *, Gregory Lantoine *, Andrew L. Hensley *, Ghislain J. Retaureau *, Kara M. Kranzusch *, Joseph W. Hickman *, Marc N. Wilson *, and Daniel P. Schrage † Georgia Institute of Technology Atlanta, Georgia 30332 ABSTRACT One of the most critical tasks in the design of a complex system is the initial conversion of mission or program objectives into a baseline system architecture. Presented in this paper is a methodology to aid in this process that is frequently used for aerospace problems at the Georgia Institute of Technology. In this paper, the methodology is applied to initial concept formulation for the Venus In Situ Explorer (VISE) mission. Five primary steps are outlined which encompass program objective definition through evaluation of candidate designs. Tools covered include the Analytic Hierarchy Process (AHP), Technique for Order Preference by Similarity to Ideal Solution (TOPSIS), and morphological matrices. Direction is given for the application of modeling and simulation as well as for subsequent iterations of the process. The paper covers both theoretical and practical aspects of the tools and process in the context of the VISE example, and it is hoped that this methodology may find future use in interplanetary probe design. 1. INTRODUCTION One of the most critical tasks in the design of a complex engineering system is the initial conversion of mission or program objectives and requirements into a baseline system architecture. In completing this task, the challenge exists to comprehensively but efficiently explore the global trade space of potential designs. -
SFSC Search Down to 4
C M Y K www.newssun.com EWS UN NHighlands County’s Hometown-S Newspaper Since 1927 Rivalry rout Deadly wreck in Polk Harris leads Lake 20-year-old woman from Lake Placid to shutout of AP Placid killed in Polk crash SPORTS, B1 PAGE A2 PAGE B14 Friday-Saturday, March 22-23, 2013 www.newssun.com Volume 94/Number 35 | 50 cents Forecast Fire destroys Partly sunny and portable at Fred pleasant High Low Wild Elementary Fire alarms “Myself, Mr. (Wally) 81 62 Cox and other administra- Complete Forecast went off at 2:40 tors were all called about PAGE A14 a.m. Wednesday 3 a.m.,” Waldron said Wednesday morning. Online By SAMANTHA GHOLAR Upon Waldron’s arrival, [email protected] the Sebring Fire SEBRING — Department along with Investigations into a fire DeSoto City Fire early Wednesday morning Department, West Sebring on the Fred Wild Volunteer Fire Department Question: Do you Elementary School cam- and Sebring Police pus are under way. Department were all on think the U.S. govern- The school’s fire alarms the scene. ment would ever News-Sun photo by KATARA SIMMONS Rhoda Ross reads to youngsters Linda Saraniti (from left), Chyanne Carroll and Camdon began going off at approx- State Fire Marshal seize money from pri- Carroll on Wednesday afternoon at the Lake Placid Public Library. Ross was reading from imately 2:40 a.m. and con- investigator Raymond vate bank accounts a children’s book she wrote and illustrated called ‘A Wildflower for all Seasons.’ tinued until about 3 a.m., Miles Davis was on the like is being consid- according to FWE scene for a large part of ered in Cyprus? Principal Laura Waldron. -
Nds of Marriage: the Implications of Hawaiian Culture & Values For
Configuring the Bo(u)nds of Marriage: The Implications of Hawaiian Culture & Values for the Debate About Homogamy Robert J. Morris, J.D.* (Kaplihiahilina)** Eia 'o Hawai'i ua ao,pa'alia i ka pono i ka lima. Here is Hawai'i, having become enlightened, confirmed by justice in her hands.1 * J.D. University of Utah College of Law, 1980; degree candidate in Hawaiian Language, University of Hawai'i at Manoa. Mahalo nui to Daniel R. Foley; Evan Wolfson; Matthew R. Yee; Walter L. Williams; H. Arlo Nimmo; Hon. Michael A. Town; Len Klekner; Andrew Koppelman; Albert J. Schtltz; the editors of this Journal; and the anonymous readers for their assistance in the preparation of this Article. As always, I acknowledge my debt to feminist scholarship and theory. All of this notwithstanding, the errors herein are mine alone. This Article is dedicated to three couples: Russ and Cathy, Ricky and Mokihana, and Damian and his aikAne. Correspondence may be sent to 1164 Bishop Street #124, Honolulu, HI 96813. ** Kapd'ihiahilina, my Hawaiian name, is the name of the commoner of the island of Kaua'i who became the aikane (same-sex lover) of the Big Island ruling chief Lonoikamakahiki. These two figures will appear in the discussion that follows. 1. MARY KAWENA P0KU'I & SAMUEL H. ELBERT, HAWAIIAN DICTIONARY 297 (1986). This is my translation of a name song (mele inoa) for Lili'uokalani, the last monarch of Hawai'i. Her government was overthrown with the assistance of resident American officials and citizens January 14-17, 1893. The literature on this event is voluminous, but the legal issues are conveniently summarized in Patrick W. -
Volcanism on Mars
Author's personal copy Chapter 41 Volcanism on Mars James R. Zimbelman Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, DC, USA William Brent Garry and Jacob Elvin Bleacher Sciences and Exploration Directorate, Code 600, NASA Goddard Space Flight Center, Greenbelt, MD, USA David A. Crown Planetary Science Institute, Tucson, AZ, USA Chapter Outline 1. Introduction 717 7. Volcanic Plains 724 2. Background 718 8. Medusae Fossae Formation 725 3. Large Central Volcanoes 720 9. Compositional Constraints 726 4. Paterae and Tholi 721 10. Volcanic History of Mars 727 5. Hellas Highland Volcanoes 722 11. Future Studies 728 6. Small Constructs 723 Further Reading 728 GLOSSARY shield volcano A broad volcanic construct consisting of a multitude of individual lava flows. Flank slopes are typically w5, or less AMAZONIAN The youngest geologic time period on Mars identi- than half as steep as the flanks on a typical composite volcano. fied through geologic mapping of superposition relations and the SNC meteorites A group of igneous meteorites that originated on areal density of impact craters. Mars, as indicated by a relatively young age for most of these caldera An irregular collapse feature formed over the evacuated meteorites, but most importantly because gases trapped within magma chamber within a volcano, which includes the potential glassy parts of the meteorite are identical to the atmosphere of for a significant role for explosive volcanism. Mars. The abbreviation is derived from the names of the three central volcano Edifice created by the emplacement of volcanic meteorites that define major subdivisions identified within the materials from a centralized source vent rather than from along a group: S, Shergotty; N, Nakhla; C, Chassigny. -
Dikes of Distinct Composition Intruded Into Noachian-Aged Crust Exposed in the Walls of Valles Marineris Jessica Flahaut, John F
Dikes of distinct composition intruded into Noachian-aged crust exposed in the walls of Valles Marineris Jessica Flahaut, John F. Mustard, Cathy Quantin, Harold Clenet, Pascal Allemand, Pierre Thomas To cite this version: Jessica Flahaut, John F. Mustard, Cathy Quantin, Harold Clenet, Pascal Allemand, et al.. Dikes of dis- tinct composition intruded into Noachian-aged crust exposed in the walls of Valles Marineris. Geophys- ical Research Letters, American Geophysical Union, 2011, 38, pp.L15202. 10.1029/2011GL048109. hal-00659784 HAL Id: hal-00659784 https://hal.archives-ouvertes.fr/hal-00659784 Submitted on 19 Jan 2012 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. GEOPHYSICAL RESEARCH LETTERS, VOL. 38, L15202, doi:10.1029/2011GL048109, 2011 Dikes of distinct composition intruded into Noachian‐aged crust exposed in the walls of Valles Marineris Jessica Flahaut,1 John F. Mustard,2 Cathy Quantin,1 Harold Clenet,1 Pascal Allemand,1 and Pierre Thomas1 Received 12 May 2011; revised 27 June 2011; accepted 30 June 2011; published 5 August 2011. [1] Valles Marineris represents the deepest natural incision and HiRISE (High Resolution Imaging Science Experiment) in the Martian upper crust. -
PREFERRED LIST of BOOKS for DISTRICT SCHOOL LIBRARIES in the STATE of MICHIGAN
z UC-NRLF , ^H 1037 ImsJ PREFERRED LIST OF BOOKS for DISTRICT SCHOOL LIBRARIES in the STATE OF MICHIGAN LANSING 1914 PREFERRED LIST OF BOOKS FOR DISTRICT SCHOOL LIBRARIES IN THE STATE OF MICHIGAN THIS BOOK LIST IS THE PROPERTY OF THE SCHOOL. DISTRICT AND IS TO BE AS STRICTLY ACCOUNTED FOR AS ANY OTHER SCHOOL PROPERTY LANSING 1914 <A IS ^ #P & €*'P*» EXTRACT FROM SCHOOL LIBRARY LAWS Act 323, Chapter 1, Section 3, laws of 1913: The Superintendent of Public Instruction * * * * with the cooperation of the State Librarian, shall prepare, at least once in every two years, lists of books suitable for township and district libraries, and furnish copies of such lists to each township and school officer entrusted with the care and custody of their respective libraries, from which lists the said school officers shall select and purchase books for their respective libraries. Approved May 13, 1913. 324611 Digitized by the Internet Archive in 2007 with funding from Microsoft Corporation http://www.archive.org/details/booklistOOmichrich CONTENTS Page INTRODUCTION 7 GENERAL LIST OF BOOKS 9-140 Picture books and primers 9-17 Religion 18-19 Mythology 19-24 Fairy tales 24-33 Folklore and legend 34-41 Government and citizenship 41-43 Nature and science 44r-60 General 44-46 Astronomy 46 Electricity—Physics 46-48 Chemistry 48 Physical geography—Geology 48-49 Botany—Gardening 49-51 Animals 51-54 Animal stories 54-58 Birds 58-59 Prehistoric man 60 Useful arts 61-67 Amusements 67-70 Art and music .\ 70-72 Literature 72-82 Collections 72-77 Poetry 77-82 Fiction -
Jason A. Dittmann 51 Pegasi B Postdoctoral Fellow
Jason A. Dittmann 51 Pegasi b Postdoctoral Fellow Contact Massachusetts Institute of Technology MIT Kavli Institute: 37-438f 617-258-5928 (office) 70 Vassar St. 520-820-0928 (cell) Cambridge, MA 02139 [email protected] Education Harvard University, Cambridge, MA PhD, Astronomy and Astrophysics, May 2016 Advisor: David Charbonneau, PhD • University of Arizona, Tucson, AZ BS, Astronomy, Physics, May 2010 Advisor: Laird Close, PhD • Recent 51 Pegasi b Postdoctoral Fellow July 2017 – Present Research Earth and Planetary Science Department, MIT Positions Faculty Contact: Sara Seager Postdoctoral Researcher Feb 2017 – June 2017 Kavli Institute, MIT Supervisor: Sarah Ballard Postdoctoral Researcher July 2016 – Jan 2017 Center for Astrophysics, Harvard University Supervisor: David Charbonneau Research Assistant Sep 2010 – May 2016 Center for Astrophysics, Harvard University Advisors: David Charbonneau Publication 16 first and second authored publications Summary 22 additional co-authored publications 1 first-authored publication in Nature 1 co-authored publication in Nature Selected 51 Pegasi b Postdoctoral Fellowship 2017 – Present Awards and Pierce Fellowship 2010 – 2013 Honors Certificate of Distinction in Teaching 2012 Best Project Award, Physics Ugrd. Research Symp. 2009 Best Undergraduate Research (Steward Observatory) 2009 – 2010 Grants Principal Investigator, Hubble Space Telescope 2017, 10 orbits Awarded “Initial Reconaissance of a Transiting Rocky (maximum award) Planet in a Nearby M-Dwarf’s Habitable Zone” Principal Investigator, -
Geologic Mapping of the Chaac-Camaxtli Region of Io from Galileo Imaging Data David A
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 107, NO. E9, 5068, doi:10.1029/2001JE001821, 2002 Geologic mapping of the Chaac-Camaxtli region of Io from Galileo imaging data David A. Williams,1 Jani Radebaugh,2 Laszlo P. Keszthelyi,2 Alfred S. McEwen,2 Rosaly M. C. Lopes,3 Sylvain Doute´,3 and Ronald Greeley1 Received 13 November 2001; revised 22 April 2002; accepted 5 June 2002; published 26 September 2002. [1] We produced a geologic/geomorphologic map of the Chaac-Camaxtli region of Io’s leading anti-Jovian hemisphere using regional resolution (186 m/pixel) Galileo imaging data collected during orbit I27 (February 2000) integrated with lower resolution (1.4 km/ pixel) color data, along with other Galileo imaging and spectral data. This is the first regional map of Io made from Galileo data. Nine color and geomorphologic units have been mapped, and the close proximity of dark and various colored bright materials suggests that there is an intimate interaction between (presumably) silicate magmas and sulfur-bearing volatile materials that produced a variety of explosive and effusive deposits in the recent geologic past. This region of Io is dominated by 11 volcanic centers, most of which are paterae that are analogous in morphology to terrestrial calderas but larger in size. Mapping of structural features indicates that most of the active regions occur in topographic lows, and less active or inactive paterae are associated with topographic highs. This indicates that crustal thickness variations influence magma access to the surface. Surface changes in this region since the Voyager flybys (1979) are relatively minor (additional bright and dark flows, color changes), although several active vents have migrated within paterae.