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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. -
Craters of the Pluto-Charon System
Icarus 287 (2017) 187–206 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Craters of the Pluto-Charon system ∗ Stuart J. Robbins a, , Kelsi N. Singer a, Veronica J. Bray b, Paul Schenk c, Tod R. Lauer d, Harold A. Weaver e, Kirby Runyon e, William B. McKinnon f, Ross A. Beyer g,h, Simon Porter a, Oliver L. White h, Jason D. Hofgartner i, Amanda M. Zangari a, Jeffrey M. Moore h, Leslie A. Young a, John R. Spencer a, Richard P. Binzel j, Marc W. Buie a, Bonnie J. Buratti i, Andrew F. Cheng e, William M. Grundy k, Ivan R. Linscott l, Harold J. Reitsema m, Dennis C. Reuter n, Mark R. Showalter g,h, G. Len Tyler l, Catherine B. Olkin a, Kimberly S. Ennico h, S. Alan Stern a, the New Horizons LORRI, MVIC Instrument Teams a Southwest Research Institute, 1050 Walnut St., Suite 300, Boulder, CO 80302, United States b Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, United States c Lunar and Planetary Institute, Houston, TX, United States d National Optical Astronomy Observatory, Tucson, AZ 85726, United States e The Johns Hopkins University, Baltimore, MD, United States f Washington University in St. Louis, St. Louis, MO, United States g SETI Institute, 189 Bernardo Avenue, Suite 100, Mountain View CA 94043, United States h NASA Ames Research Center, Moffett Field, CA 84043, United States i NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States j Massachusetts Institute of Technology, Cambridge, MA, United States k Lowell Observatory, Flagstaff, AZ, United States l Stanford University, Stanford, CA, United States m Ball Aerospace, Boulder, CO, United States n NASA Goddard Space Flight Center, Greenbelt, MD, United States a r t i c l e i n f o a b s t r a c t Article history: NASA’s New Horizons flyby mission of the Pluto-Charon binary system and its four moons provided hu- Received 3 March 2016 manity with its first spacecraft-based look at a large Kuiper Belt Object beyond Triton. -
Charon Tectonics
Icarus 287 (2017) 161–174 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Charon tectonics ∗ Ross A. Beyer a,b, , Francis Nimmo c, William B. McKinnon d, Jeffrey M. Moore b, Richard P. Binzel e, Jack W. Conrad c, Andy Cheng f, K. Ennico b, Tod R. Lauer g, C.B. Olkin h, Stuart Robbins h, Paul Schenk i, Kelsi Singer h, John R. Spencer h, S. Alan Stern h, H.A. Weaver f, L.A. Young h, Amanda M. Zangari h a Sagan Center at the SETI Institute, 189 Berndardo Ave, Mountain View, California 94043, USA b NASA Ames Research Center, Moffet Field, CA 94035-0 0 01, USA c University of California, Santa Cruz, CA 95064, USA d Washington University in St. Louis, St Louis, MO 63130-4899, USA e Massachusetts Institute of Technology, Cambridge, MA 02139, USA f Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA g National Optical Astronomy Observatories, Tucson, AZ 85719, USA h Southwest Research Institute, Boulder, CO 80302, USA i Lunar and Planetary Institute, Houston, TX 77058, USA a r t i c l e i n f o a b s t r a c t Article history: New Horizons images of Pluto’s companion Charon show a variety of terrains that display extensional Received 14 April 2016 tectonic features, with relief surprising for this relatively small world. These features suggest a global ex- Revised 8 December 2016 tensional areal strain of order 1% early in Charon’s history. Such extension is consistent with the presence Accepted 12 December 2016 of an ancient global ocean, now frozen. -
Collision Probabilities in the Edgeworth-Kuiper Belt
Draft version April 30, 2021 Typeset using LATEX default style in AASTeX63 Collision Probabilities in the Edgeworth-Kuiper belt Abedin Y. Abedin,1 JJ Kavelaars,1 Sarah Greenstreet,2, 3 Jean-Marc Petit,4 Brett Gladman,5 Samantha Lawler,6 Michele Bannister,7 Mike Alexandersen,8 Ying-Tung Chen,9 Stephen Gwyn,1 and Kathryn Volk10 1National Research Council of Canada, Herzberg Astronomy and Astrophysics, 5071 West Saanich Road, Victoria, BC V9E 2E7, Canada 2B612 Asteroid Institute, 20 Sunnyside Avenue, Suite 427, Mill Valley, CA 94941, USA 3DIRAC Center, Department of Astronomy, University of Washington, 3910 15th Avenue NE, Seattle, WA 98195, USA 4Institut UTINAM, CNRS-UMR 6213, Universit´eBourgogne Franche Comt´eBP 1615, 25010 Besan¸conCedex, France 5Department of Physics and Astronomy, 6224 Agricultural Road, University of British Columbia, Vancouver, British Columbia, Canada 6Campion College and the Department of Physics, University of Regina, Regina SK, S4S 0A2, Canada 7University of Canterbury, Christchurch, New Zealand 8Minor Planet Center, Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138, US 9Academia Sinica Institute of Astronomy and Astrophysics, Taiwan 10Lunar and Planetary Laboratory, University of Arizona: Tucson, AZ, USA Submitted to AJ ABSTRACT Here, we present results on the intrinsic collision probabilities, PI , and range of collision speeds, VI , as a function of the heliocentric distance, r, in the trans-Neptunian region. The collision speed is one of the parameters, that serves as a proxy to a collisional outcome e.g., complete disruption and scattering of fragments, or formation of crater, where both processes are directly related to the impact energy. We utilize an improved and de-biased model of the trans-Neptunian object (TNO) region from the \Outer Solar System Origins Survey" (OSSOS). -
Properties Available for Claim by County
05/17/2019 Properties Available For Claim By County ADAMS Property ID Owner Name Street 1 Street 2 City ST ZIP Amount Shares 3192640 A Y MINI MART 100 LOWER WOODVILLE RD NATCHEZ MS 39120 $93.10 0.00 1036910 ABERDEFN INC 25 SEARGANT PRENTISS DR NATCHEZ MS 39120 $71.31 0.00 2324787 ACCESS TRAVEL P O BOX 17787 NATCHEZ MS 39122-7787 $815.51 0.00 3162705 ACKERMAN ANNET PO BOX P NATCHEZ MS 39121 $85.00 0.00 3392306 ACKERMAN ANNET ROSE P O BOX P NATCHEZ MS 39121-3015 $1,421.35 0.00 2584242 ACKERMAN ELODIE 518 GREENFIELD RD NATCHEZ MS 39120-8760 $84.04 0.00 1427482 ACUMEN CLAIM SERVICE PO BOX 17915 NATCHEZ MS 39122 $248.00 0.00 1314305 ACUMEN CLAIM SERVICES PO BOX 17975 NATCHEZ MS 39122 $337.00 0.00 4220401 ADAM T GWIN 102 SOUTH MARTIN LUTHER KING NATCHEZ MS 39121 $235.22 0.00 2981594 ADAMS BERNARD RR 6 BOX 125 NATCHEZ MS 39120 $1,000.00 0.00 1243566 ADAMS CHARLES E P O BOX 2237 NATCHEZ MS 39121 $0.00 2.00 2748567 ADAMS CNTY JUSTICE COURT 37 GREENWOOD SUBD RD NATCHEZ MS 39120 $212.52 0.00 2047419 ADAMS CO DEMOCRATIC EXEC COMMI 107 GAILE AVE NATCHEZ MS 39120-2608 $244.99 0.00 2813325 ADAMS COUNTY DEPUTY FUND PO DRAWER F NATCHEZ MS 39121 $100.00 0.00 2891312 ADAMS COUNTY F C/O RUBY M GAYLOR NATCHEZ MS 39120 $346.92 0.00 3208263 ADAMS COUNTY TAX COLLECTOR 1 FREDERICK ROAD NATCHEZ MS 39120 $2,176.66 0.00 3872896 ADAMS COUNTY TAX COLLECTOR P O BOX 1128 NATCHEZ MS 39121 $2,137.23 0.00 3470845 ADAMS EARNESTINE 11 OLD SMITHS LN NATCHEZ MS 39120 $672.27 0.00 1390575 ADAMS EMERG 54 SGT S PRENTISS DR NATCHEZ MS 39120- $170.00 0.00 2167569 ADAMS EMERGENCY -
Summary of Sexual Abuse Claims in Chapter 11 Cases of Boy Scouts of America
Summary of Sexual Abuse Claims in Chapter 11 Cases of Boy Scouts of America There are approximately 101,135sexual abuse claims filed. Of those claims, the Tort Claimants’ Committee estimates that there are approximately 83,807 unique claims if the amended and superseded and multiple claims filed on account of the same survivor are removed. The summary of sexual abuse claims below uses the set of 83,807 of claim for purposes of claims summary below.1 The Tort Claimants’ Committee has broken down the sexual abuse claims in various categories for the purpose of disclosing where and when the sexual abuse claims arose and the identity of certain of the parties that are implicated in the alleged sexual abuse. Attached hereto as Exhibit 1 is a chart that shows the sexual abuse claims broken down by the year in which they first arose. Please note that there approximately 10,500 claims did not provide a date for when the sexual abuse occurred. As a result, those claims have not been assigned a year in which the abuse first arose. Attached hereto as Exhibit 2 is a chart that shows the claims broken down by the state or jurisdiction in which they arose. Please note there are approximately 7,186 claims that did not provide a location of abuse. Those claims are reflected by YY or ZZ in the codes used to identify the applicable state or jurisdiction. Those claims have not been assigned a state or other jurisdiction. Attached hereto as Exhibit 3 is a chart that shows the claims broken down by the Local Council implicated in the sexual abuse. -
“Vulcan Planum” Map Dark-Colored Ejecta Scale Maps
Charon: Geologic Map of New Horizons’ Encounter Hemisphere, III S.J. Robbins0,1, J.R. Spencer1, R.A. Beyer2,3, P. Schenk4, J.M. Moore3, W.B. McKinnon5, R.P. Binzel6, M.W. Buie1, B.J. Buratti7, A.F. Cheng8, W.M. Grundy9, I.R. Linscott10, H.J. Reitsema11, D.C. Reuter12, M.R. Showalter2, G.L. Tyler1, L.A. Young1, C.B. Olkin1, K. Ennico3, H.A. Weaver8, S.A. Stern1, the New Horizons Geology & Geophysics Investigation Team, LORRI Instrument Team, MVIC Instrument Team, and the New Horizons Encounter Team Tectonics Map Geologic Contacts Mapping Details map boundary boundary, certain Global boundary, approximate Approximate Map Area: 60% of disk* Linear Features Full Map Scale: 1:3M printed map 50” crest of buried crater crest of crater rim Mapping Scale (6×): 1:500,000 depression margin map colors used only in tectonics Vertex Spacing: 2.5 km (⅘ mm) graben trace Min. Crater: 30 km (1 cm) groove ridge crest Min. Feature Length: 15 km (½ cm) catena Min. Unit: 250 km2 scarp base *Map area covers images taken within a few scarp crest hours of closest approach and closely corre- broad warp sponds with the areas imaged at ≲1 km/px. Southern margin of “map boundary” corre- example of offset due to different versions sponds to terminator topography and is not fully of the basemap being used; all lines must Surface Features reflected in incidence / emission angle and pixel be redrafted to the same, most recent solution “Vulcan Planum” Map dark-colored ejecta scale maps. Area is ≈2,800,000 km2. -
Asteroids, Comets, Meteors -‐‑ ACM2017 -‐‑ Montevid
Asteroids, Comets, Meteors - ACM2017 - Montevideo THE GEOLOGY OF CHARON AS REVEALED BY NEW HORIZONS J. M. Moore1, J. R. Spencer2, W. B. McKinnon3, R. A. Beyer1,4, S.A. Stern2, K. Ennico1, C.B. Olkin2, H.A. Weaver5, L.A. Young2, and the New Horizons Science Team 1National Aeronautics and Space Administration (NASA) Ames Research Center, MS-245-3 Space 2 Sci. Division, Moffett Field, CA 94035, USA, Southwest Research Institute, Boulder, CO 80302, USA, 3Washington University, St. Louis, MO 63130, USA, 4SETI Institute, Mt. View, CA 94043, USA, 5Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA. Introduction: Pluto’s large moon Charon (ra- Clarke Montes appears to expose a more rugged dius 606 km; r = 1.70 g cm-3) exhibits a striking terrain, with smooth plains embaying the mar- variety of landscapes. Charon can be divided gins, two of which are lobate. In addition to the into two broad provinces separated by a roughly moats surrounding these mountains, there are aligned assemblage of ridges and canyons, two additional depressions surrounded by which span from east to west. North of this tec- rounded or lobate margins. We speculate that tonic belt is rugged, cratered terrain (Oz Terra); both the moats and depressions may be the ex- south of it are smoother but geologically com- pressions of the flow of, and incomplete enclo- plex plains (Vulcan Planum). (All place names sure by, viscous, cryovolcanic materials, such as here are informal.) Relief exceeding 20 km is proposed at Ariel and Miranda [5, 6]. The seen in limb profiles and stereo topography. -
A White Paper on Pluto Follow on Missions: Background, Rationale
A White Paper on Pluto Follow On Missions: Background, Rationale, and New Mission Recommendations 2018 March 12 1 Signatories In Alphabetical Order: Caitlin Ahrens, Michelle T. Bannister, Tanguy Bertrand, Ross Beyer, Richard Binzel, Maitrayee Bose, Paul Byrne, Robert Chancia, Dale Cruikshank, Rajani Dhingra, Cynthia Dinwiddie, David Dunham, Alissa Earle, Christopher Glein, Cesare Grava, Will Grundy, Aurelie Guilbert, Doug Hamilton, Jason Hofgartner, Brian Holler, Mihaly Horanyi, Sona Hosseini, James Tuttle Keane, Akos Kereszturi, Eduard Kuznetsov, Rosaly Lopes, Renu Malhotra, Kathleen Mandt Jeff Moore, Cathy Olkin, Maurizio Pajola, Lynnae Quick, Stuart Robbins, 2 Gustavo Benedetti Rossi, Kirby Runyon, Pablo Santos Sanz, Paul Schenk Jennifer Scully, Kelsi Singer, Alan Stern, Timothy Stubbs, Mark Sykes, Laurence Trafton, Anne Verbiscer, Larry Wasserman, and Amanda Zangari 3 Executive Summary The exploration of the binary Pluto-Charon and its small satellites during the New Horizons flyby in 2015 revealed not only widespread geologic and compositional diversity across Pluto, but surprising complexity, a wide range of surface unit ages, evidence for widespread activity stretching across billion of years to the near-present, as well as numerous atmospheric puzzles, and strong atmospheric coupling with its surface. New Horizons also found an unexpected diversity of landforms on its binary companion, Charon. Pluto’s four small satellites yielded surprises as well, including their unexpected rapid and high obliquity rotation states, high albedos, and diverse densities. Here we briefly review the findings made by New Horizons and the case for a follow up mission to investigate the Pluto system in more detail. As the next step in the exploration of this spectacular planet-satellite system, we recommend an orbiter to study it in considerably more detail, with new types of instrumentation, and to observe its changes with time. -
Spaceflight a British Interplanetary Society Publication
SpaceFlight A British Interplanetary Society publication Volume 60 No.8 August 2018 £5.00 The perils of walking on the Moon 08> Charon Tim Peake 634072 Russia-Sino 770038 9 Space watches CONTENTS Features 14 To Russia with Love Philip Corneille describes how Russia fell in love with an iconic Omega timepiece first worn by NASA astronauts. 18 A glimpse of the Cosmos 14 Nicholas Da Costa shows us around the Letter from the Editor refurbished Cosmos Pavilion – the Moscow museum for Russian space achievements. In addition to the usual mix of reports, analyses and commentary 20 Deadly Dust on all space-related matters, I am The Editor looks back at results from the Apollo particularly pleased to re- Moon landings and asks whether we are turning introduce in this month’s issue our a blind eye to perils on the lunar surface. review of books. And to expand that coverage to all forms of 22 Mapping the outer limits media, study and entertainment be SpaceFlight examines the latest findings it in print, on video or in a concerning Charon, Pluto’s major satellite, using 18 computer game – so long as it’s data sent back by NASA's New Horizons. related to space – and to have this as a regular monthly contribution 27 Peake Viewing to the magazine. Rick Mulheirn comes face to face with Tim Specifically, it is gratifying to see a young generation stepping Peake’s Soyuz spacecraft and explains where up and contributing. In which this travelling display can be seen. regard, a warm welcome to the young Henry Philp for having 28 38th BIS Russia-Sino forum provided for us a serious analysis Brian Harvey and Ken MacTaggart sum up the of a space-related computer game latest Society meeting dedicated to Russian and which is (surprisingly, to this Chinese space activities. -
Distributor Settlement Agreement
DISTRIBUTOR SETTLEMENT AGREEMENT Table of Contents Page I. Definitions............................................................................................................................1 II. Participation by States and Condition to Preliminary Agreement .....................................13 III. Injunctive Relief .................................................................................................................13 IV. Settlement Payments ..........................................................................................................13 V. Allocation and Use of Settlement Payments ......................................................................28 VI. Enforcement .......................................................................................................................34 VII. Participation by Subdivisions ............................................................................................40 VIII. Condition to Effectiveness of Agreement and Filing of Consent Judgment .....................42 IX. Additional Restitution ........................................................................................................44 X. Plaintiffs’ Attorneys’ Fees and Costs ................................................................................44 XI. Release ...............................................................................................................................44 XII. Later Litigating Subdivisions .............................................................................................49 -
Report 2017 Research, Education and Public Outreach Activity Report 2017 Research, Education and Public Outreach
Activity Report 2017 Research, Education and Public Outreach Activity Report 2017 Research, Education and Public Outreach Nathalie A. Cabrol Director, Carl Sagan Center, Pamela Harman, Acting Director, Center for Education Rebecca McDonald Director, Center for Outreach Bill Diamond President & CEO The SETI Institute: 189 N Bernardo Avenue Suite 200, Mountain View, CA 94043. Phone: (650) 961-6633 Activity Report 2017 Research, Education and Public Outreach TABLE OF CONTENTS Peer-reviewed publications 10 Conferences: Abstracts & Proceedings 18 Technical Reports & Data Releases 29 Outreach, Media Coverage, Web Stories & Interviews 31 Invited Talks (Professional & Public) 39 Highlights, Significant Events & Activities 46 Fieldwork 52 Honors & Awards 54 Missions, Observations & Strategic Planning 56 Acknowledgements 60 The SETI Institute: 189 N Bernardo Avenue Suite 200, Mountain View, CA 94043. Phone: (650) 961-6633 Activity Report 2017 Research, Education and Public Outreach FROM THE SETI INSTITUTE President and CEO Dear friends, The scientists, educators and outreach professionals of the SETI Institute had yet another banner year of productivity in 2017. We are delighted to present our 2nd annual report, cataloging the research and education programs of the Institute, as well as the myriad of mainstream media stories about our people and our work. Among the highlights from this year’s report are 147 peer-reviewed articles in scientific journals, 225 conference proceedings and abstracts, 172 media stories and interviews, and 177 invited talks.