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Planetary Research Center Lowell Observatory Flagstaff, Arizona 86002
N 8 4 - °1* R 7 <• PLANETARY RESEARCH CENTER LOWELL OBSERVATORY FLAGSTAFF, ARIZONA 86002 NASA GRANT NSG-7530 POST-MISSION VIKING DATA ANALYSIS FINAL REPORT ; SUBMITTED: 26 APRIL M-A,- BAUM-- ' KARI_LUMME .__ PRINCIPAL-INVESTIGATOR< -? CO-^INVESTIGATOR J, .WTIN -• LAWRENCE H, WASSERMAN CO-INVESTIGATOR CO-INVESTIGATOR Page 2 PERSONNEL—" Averaged over the time interval (3.7 years) that funds were expended under this grant, the following staff devoted the indicated percentages of their time to it: W. A. Baum, Principal Investigator, 18$ time L. J. Martin, Co-Investigator, 52% K. Lumme, Co-Investigator, 19% L. H. Wasserman, Co-Investigator, S% T. J. Kreidl, Computer Programmer, 5% Others (combined), ResearctuAssistants, 7-$ • ~ -> "Others" include H. S. Horstman, M. L. Kantz, and S. E. Jones. In addition, there are several Observatory employees paid through overhead who provide services such as library, bookkeeping, and maintenance. BACKGROUND Work under this grant was a continuation of our participation in the Viking Mission. That participation commenced in 1970 with Baum's membership on the Viking Orbiter Imaging Team and continued through the end of team operations in 1978. This grant then commenced in 1979 at the start of the Mars Data Analysis Program (MDAP). MDAP was planned by NASA as a 5-year program, and our initial MDAP proposal was scaled to that expectation and to a funding level consistent with the Mars research projects in which we were already engaged. As it turned out, there were subsequent reductions in MDAP funds, and we (like many of our colleagues at other institutions) had to adjust the scope of our Mars research projects accordingly. -
Lowell Observatory Communications Office 1400 W. Mars Hill Rd
Lowell Observatory Communications Office 1400 W. Mars Hill Rd. Flagstaff, AZ 86001 www.lowell.edu PRESS RELEASE FOR IMMEDIATE RELEASE MAY 12, 2015 ***Contact details appear below*** Image attached LOWELL OBSERVATORY TO HOST PLUTO AND BEYOND GALA ON JUNE 13 Flagstaff, Az- Lowell Observatory will host its fourth annual fundraising gala, Pluto and Beyond, on June 13. Sponsored by APS, it will take place on the campus of Northern Arizona University in Flagstaff and feature experts sharing the latest Pluto news, auctions showcasing a variety of travel packages and astronomy-themed collectibles, and live music. Proceeds support Lowell’s mission of astronomical research and outreach. Lisa Actor, Lowell’s Deputy Director for Development, said, “This will be an exciting event in this year when we’re celebrating the 85th anniversary of the discovery of Pluto at Lowell Observatory! I’m anxious to meet and personally thank the many Flagstaff area supporters of the observatory.” Pluto and Beyond kicks off with the Kuiper VIP Reception at 5:30 p.m. Presented by Blue Cross Blue Shield of Arizona, this champagne and cocktail gathering will meet in the 1899 Bar & Grill. The main event happens in the High Country Conference Center, with doors opening at 6 p.m. and a sit-down dinner served at 7:30 p.m. Afterward, experts from Lowell Observatory will discuss the astronomy news story of the year—the New Horizons spacecraft’s July approach to Pluto after an incredible nine-year journey. This program will start with a look at Clyde Tombaugh’s improbable discovery of this icy world at Lowell in 1930 and continue with the latest news from New Horizons as it prepares to capture the first-ever close-up images of Pluto’s surface. -
CNC/IUGG: 2019 Quadrennial Report
CNC/IUGG: 2019 Quadrennial Report Geodesy and Geophysics in Canada 2015-2019 Quadrennial Report of the Canadian National Committee for the International Union of Geodesy and Geophysics Prepared on the Occasion of the 27th General Assembly of the IUGG Montreal, Canada July 2019 INTRODUCTION This report summarizes the research carried out in Canada in the fields of geodesy and geophysics during the quadrennial 2015-2019. It was prepared under the direction of the Canadian National Committee for the International Union of Geodesy and Geophysics (CNC/IUGG). The CNC/IUGG is administered by the Canadian Geophysical Union, in consultation with the Canadian Meteorological and Oceanographic Society and other Canadian scientific organizations, including the Canadian Association of Physicists, the Geological Association of Canada, and the Canadian Institute of Geomatics. The IUGG adhering organization for Canada is the National Research Council of Canada. Among other duties, the CNC/IUGG is responsible for: • collecting and reconciling the many views of the constituent Canadian scientific community on relevant issues • identifying, representing, and promoting the capabilities and distinctive competence of the community on the international stage • enhancing the depth and breadth of the participation of the community in the activities and events of the IUGG and related organizations • establishing the mechanisms for communicating to the community the views of the IUGG and information about the activities of the IUGG. The aim of this report is to communicate to both the Canadian and international scientific communities the research areas and research progress that has been achieved in geodesy and geophysics over the last four years. The main body of this report is divided into eight sections: one for each of the eight major scientific disciplines as represented by the eight sister societies of the IUGG. -
Eighteenth-Century English and French Landscape Painting
University of Louisville ThinkIR: The University of Louisville's Institutional Repository Electronic Theses and Dissertations 12-2018 Common ground, diverging paths: eighteenth-century English and French landscape painting. Jessica Robins Schumacher University of Louisville Follow this and additional works at: https://ir.library.louisville.edu/etd Part of the Other History of Art, Architecture, and Archaeology Commons Recommended Citation Schumacher, Jessica Robins, "Common ground, diverging paths: eighteenth-century English and French landscape painting." (2018). Electronic Theses and Dissertations. Paper 3111. https://doi.org/10.18297/etd/3111 This Master's Thesis is brought to you for free and open access by ThinkIR: The University of Louisville's Institutional Repository. It has been accepted for inclusion in Electronic Theses and Dissertations by an authorized administrator of ThinkIR: The University of Louisville's Institutional Repository. This title appears here courtesy of the author, who has retained all other copyrights. For more information, please contact [email protected]. COMMON GROUND, DIVERGING PATHS: EIGHTEENTH-CENTURY ENGLISH AND FRENCH LANDSCAPE PAINTING By Jessica Robins Schumacher B.A. cum laude, Vanderbilt University, 1977 J.D magna cum laude, Brandeis School of Law, University of Louisville, 1986 A Thesis Submitted to the Faculty of the College of Arts and Sciences of the University of Louisville in Partial Fulfillment of the Requirements for the Degree of Master of Arts in Art (C) and Art History Hite Art Department University of Louisville Louisville, Kentucky December 2018 Copyright 2018 by Jessica Robins Schumacher All rights reserved COMMON GROUND, DIVERGENT PATHS: EIGHTEENTH-CENTURY ENGLISH AND FRENCH LANDSCAPE PAINTING By Jessica Robins Schumacher B.A. -
October 2003 SOCIETY
ISSN 0739-4934 NEWSLETTER HISTORY OF SCIENCE VOLUME 32 NUMBER 4 October 2003 SOCIETY those with no interest in botany, the simple beauty of the glass is enough. Natural History Delights in Cambridge From modern-life in glass to long-ago life, it’s only a short walk. The museum houses ant to discuss dinosaurs, explore microfossils of some of the Earth’s earliest life Wancient civilizations, learn wild- forms, as well as fossil fish and dinosaurs – flower gardening, or study endangered such as the second ever described Triceratops, species? If variety is the spice of life, then and the world’s only mounted Kronosaurus, a the twenty-one million specimens at the 42-foot-long prehistoric marine reptile. Harvard Museum of Natural History show a Among its 90,000 zoological specimens the museum bursting with life, much of it unnat- museum also has the pheasants once owned urally natural. by George Washington. And many of the The museum will be the site of the opening mammal collections were put together in the reception for the 2003 HSS annual meeting. 19th century by “lions” in the history of sci- The reception begins at 7 p.m. Thursday, 20 ence, like Louis Agassiz. November, and tickets will be available at the Much of the museum’s collection of rocks and meeting registration desk. Buses will run from ores is the result of field work, but the museum the host hotel to the museum. houses not only that which has been dug up, but The Harvard MNH is an ideal spot for his- also that which has fallen out of the sky. -
+ New Horizons
Media Contacts NASA Headquarters Policy/Program Management Dwayne Brown New Horizons Nuclear Safety (202) 358-1726 [email protected] The Johns Hopkins University Mission Management Applied Physics Laboratory Spacecraft Operations Michael Buckley (240) 228-7536 or (443) 778-7536 [email protected] Southwest Research Institute Principal Investigator Institution Maria Martinez (210) 522-3305 [email protected] NASA Kennedy Space Center Launch Operations George Diller (321) 867-2468 [email protected] Lockheed Martin Space Systems Launch Vehicle Julie Andrews (321) 853-1567 [email protected] International Launch Services Launch Vehicle Fran Slimmer (571) 633-7462 [email protected] NEW HORIZONS Table of Contents Media Services Information ................................................................................................ 2 Quick Facts .............................................................................................................................. 3 Pluto at a Glance ...................................................................................................................... 5 Why Pluto and the Kuiper Belt? The Science of New Horizons ............................... 7 NASA’s New Frontiers Program ........................................................................................14 The Spacecraft ........................................................................................................................15 Science Payload ...............................................................................................................16 -
2018: Aiaa-Space-Report
AIAA TEAM SPACE TRANSPORTATION DESIGN COMPETITION TEAM PERSEPHONE Submitted By: Chelsea Dalton Ashley Miller Ryan Decker Sahil Pathan Layne Droppers Joshua Prentice Zach Harmon Andrew Townsend Nicholas Malone Nicholas Wijaya Iowa State University Department of Aerospace Engineering May 10, 2018 TEAM PERSEPHONE Page I Iowa State University: Persephone Design Team Chelsea Dalton Ryan Decker Layne Droppers Zachary Harmon Trajectory & Propulsion Communications & Power Team Lead Thermal Systems AIAA ID #908154 AIAA ID #906791 AIAA ID #532184 AIAA ID #921129 Nicholas Malone Ashley Miller Sahil Pathan Joshua Prentice Orbit Design Science Science Science AIAA ID #921128 AIAA ID #922108 AIAA ID #761247 AIAA ID #922104 Andrew Townsend Nicholas Wijaya Structures & CAD Trajectory & Propulsion AIAA ID #820259 AIAA ID #644893 TEAM PERSEPHONE Page II Contents 1 Introduction & Problem Background2 1.1 Motivation & Background......................................2 1.2 Mission Definition..........................................3 2 Mission Overview 5 2.1 Trade Study Tools..........................................5 2.2 Mission Architecture.........................................6 2.3 Planetary Protection.........................................6 3 Science 8 3.1 Observations of Interest.......................................8 3.2 Goals.................................................9 3.3 Instrumentation............................................ 10 3.3.1 Visible and Infrared Imaging|Ralph............................ 11 3.3.2 Radio Science Subsystem................................. -
100M Dash (5A Girls) All Times Are FAT, Except
100m Dash (5A Girls) All times are FAT, except 2 0 2 1 R A N K I N G S A L L - T I M E T O P - 1 0 P E R F O R M A N C E S 1 12 Nerissa Thompson 12.35 North Salem 1 Margaret Johnson-Bailes 11.30a Churchill 1968 2 12 Emily Stefan 12.37 West Albany 2 Kellie Schueler 11.74a Summit 2009 3 9 Kensey Gault 12.45 Ridgeview 3 Jestena Mattson 11.86a Hood River Valley 2015 4 12 Cyan Kelso-Reynolds 12.45 Springfield 4 LeReina Woods 11.90a Corvallis 1989 5 10 Madelynn Fuentes 12.78 Crook County 5 Nyema Sims 11.95a Jefferson 2006 6 10 Jordan Koskondy 12.82 North Salem 6 Freda Walker 12.04c Jefferson 1978 7 11 Sydney Soskis 12.85 Corvallis 7 Maya Hopwood 12.05a Bend 2018 8 12 Savannah Moore 12.89 St Helens 8 Lanette Byrd 12.14c Jefferson 1984 9 11 Makenna Maldonado 13.03 Eagle Point Julie Hardin 12.14c Churchill 1983 10 10 Breanna Raven 13.04 Thurston Denise Carter 12.14c Corvallis 1979 11 9 Alice Davidson 13.05 Scappoose Nancy Sim 12.14c Corvallis 1979 12 12 Jada Foster 13.05 Crescent Valley Lorin Barnes 12.14c Marshall 1978 13 11 Tori Houg 13.06 Willamette Wind-Aided 14 9 Jasmine McIntosh 13.08 La Salle Prep Kellie Schueler 11.68aw Summit 2009 15 12 Emily Adams 13.09 The Dalles Maya Hopwood 12.03aw Bend 2016 16 9 Alyse Fountain 13.12 Lebanon 17 11 Monica Kloess 13.14 West Albany C L A S S R E C O R D S 18 12 Molly Jenne 13.14 La Salle Prep 9th Kellie Schueler 12.12a Summit 2007 19 9 Ava Marshall 13.16 South Albany 10th Kellie Schueler 12.01a Summit 2008 20 11 Mariana Lomonaco 13.19 Crescent Valley 11th Margaret Johnson-Bailes 11.30a Churchill 1968 -
TENURE-TRACK Or TENURED ASTRONOMER Lowell Observatory
TENURE-TRACK or TENURED ASTRONOMER Lowell Observatory invites applications for one or more tenure-track or tenured research positions in astronomy or planetary science. We invite applicants at any career level who can build on current strengths or open new areas for Lowell. A Ph.D. in astronomy, planetary science, or a related field is required, as is an outstanding record of research and demonstrated ability or potential to obtain external research funding. Candidates are invited to describe how they would make use of our observational facilities, but we will give equal consideration to all research areas. The start date for this position is flexible but desired by Fall 2016. Lowell Observatory is an independent, non-profit research institution. Our astronomers have access to our new 4.3-meter Discovery Channel Telescope, operated in partnership with Boston University, the University of Toledo, the University of Maryland/GSFC, Northern Arizona University, Yale University, and Discovery Communications. Lowell also maintains 1.8-m, 1.1-m, and 0.9-m telescopes equipped with optical and IR imagers and spectrographs. We partner with the US Naval Observatory and the Naval Research Laboratory in the Navy Precision Optical Interferometer. Lowell offers numerous opportunities for involvement in education and outreach as well. To apply: Send applications electronically to [email protected]. Applications should include (1) a cover letter and CV, (2) a research plan of 3 pages or less, and (3) names and mail/email addresses of three individuals who have agreed to serve as references. Do not ask for reference letters to be sent in advance. -
Planetary Patrol - an International Effort
136 COMMISSIONS 16, 17 AND 40 ments devoted to the passage through the asteroid belt which precedes the Jupiter rendezvous. Emphasis was placed on the anticipated contributions of these three programs to our understanding of the solar system. In discussion Carl Sagan stressed that mission B of the Mariner Mars 1971 program is designed to have an orbital period four-thirds the Martian rotational period so that every four days the space craft observes the same area under the same lighting conditions. In this way intrinsic Martian albedo changes can be distinguished from effects due to the scattering phase function of surface material. He also mentioned the possibility that photographic mapping of Phobos and Deimos by the Mariner Mars 1971 mission would provide cartography of these moons superior to the best groundbased cartography of Mars. PLANETARY PATROL - AN INTERNATIONAL EFFORT W. A. Baum Lowell Observatory Abstract. An international photographic planetary patrol network, consisting of the Mauna Kea Observatory in Hawaii, the Mount Stromlo Observatory in eastern Australia, the Republic Observa tory in South Africa, the Cerro Tololo Inter-American Observatory in northern Chile, and the Lowell Observatory, has been in operation since April 1969. The Magdalena Peak Station of the Mexico State University also participated temporarily. New stations are now being added at the Perth Observatory in western Australia and at the Kavalur Station of the Kodaikanal Observatory in southern India. During 1969 Mars and Jupiter were photographed through blue, green, and red filters; and the network produced more than 11000 fourteen-exposure filmstrips with images of a quality suitable for analysis. -
9–22–00 Vol. 65 No. 185 Friday Sept. 22, 2000 Pages 57277–57536
9±22±00 Friday Vol. 65 No. 185 Sept. 22, 2000 Pages 57277±57536 VerDate 11-MAY-2000 19:36 Sep 21, 2000 Jkt 190000 PO 00000 Frm 00001 Fmt 4710 Sfmt 4710 E:\FR\FM\22SEWS.LOC pfrm11 PsN: 22SEWS 1 II Federal Register / Vol. 65, No. 185 / Friday, September 22, 2000 The FEDERAL REGISTER is published daily, Monday through SUBSCRIPTIONS AND COPIES Friday, except official holidays, by the Office of the Federal Register, National Archives and Records Administration, PUBLIC Washington, DC 20408, under the Federal Register Act (44 U.S.C. Subscriptions: Ch. 15) and the regulations of the Administrative Committee of Paper or fiche 202±512±1800 the Federal Register (1 CFR Ch. I). The Superintendent of Assistance with public subscriptions 512±1806 Documents, U.S. Government Printing Office, Washington, DC 20402 is the exclusive distributor of the official edition. General online information 202±512±1530; 1±888±293±6498 Single copies/back copies: The Federal Register provides a uniform system for making available to the public regulations and legal notices issued by Paper or fiche 512±1800 Federal agencies. These include Presidential proclamations and Assistance with public single copies 512±1803 Executive Orders, Federal agency documents having general FEDERAL AGENCIES applicability and legal effect, documents required to be published Subscriptions: by act of Congress, and other Federal agency documents of public interest. Paper or fiche 523±5243 Assistance with Federal agency subscriptions 523±5243 Documents are on file for public inspection in the Office of the Federal Register the day before they are published, unless the issuing agency requests earlier filing. -
1 the New Horizons Spacecraft Glen H. Fountain, David Y
The New Horizons Spacecraft Glen H. Fountain, David Y. Kusnierkiewicz, Christopher B. Hersman, Timothy S. Herder, Thomas B Coughlin, William T. Gibson, Deborah A. Clancy, Christopher C. DeBoy, T. Adrian Hill, James D. Kinnison, Douglas S. Mehoke, Geffrey K. Ottman, Gabe D. Rogers, S. Alan Stern, James M. Stratton, Steven R. Vernon, Stephen P. Williams Abstract The New Horizons spacecraft was launched on January 19, 2006. The spacecraft was designed to provide a platform for the seven instruments designated by the science team to collect and return data from Pluto in 2015 that would meet the requirements established by the National Aeronautics and Space Administration (NASA) Announcement of Opportunity AO-OSS-01. The design drew on heritage from previous missions developed at The Johns Hopkins University Applied Physics Laboratory (APL) and other NASA missions such as Ulysses. The trajectory design imposed constraints on mass and structural strength to meet the high launch acceleration consistent with meeting the AO requirement of returning data prior to the year 2020. The spacecraft subsystems were designed to meet tight resource allocations (mass and power) yet provide the necessary control and data handling finesse to support data collection and return when the one way light time during the Pluto fly-by is 4.5 hours. Missions to the outer regions of the solar system (where the solar irradiance is 1/1000 of the level near the Earth) require a Radioisotope Thermoelectric Generator (RTG) to supply electrical power. One RTG was available for use by New Horizons. To accommodate this constraint, the spacecraft electronics were designed to operate on less than 200 W.