Guide to the Robert W. Jackson Collection, 1964-1999 PP03.02
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Mission to Jupiter
This book attempts to convey the creativity, Project A History of the Galileo Jupiter: To Mission The Galileo mission to Jupiter explored leadership, and vision that were necessary for the an exciting new frontier, had a major impact mission’s success. It is a book about dedicated people on planetary science, and provided invaluable and their scientific and engineering achievements. lessons for the design of spacecraft. This The Galileo mission faced many significant problems. mission amassed so many scientific firsts and Some of the most brilliant accomplishments and key discoveries that it can truly be called one of “work-arounds” of the Galileo staff occurred the most impressive feats of exploration of the precisely when these challenges arose. Throughout 20th century. In the words of John Casani, the the mission, engineers and scientists found ways to original project manager of the mission, “Galileo keep the spacecraft operational from a distance of was a way of demonstrating . just what U.S. nearly half a billion miles, enabling one of the most technology was capable of doing.” An engineer impressive voyages of scientific discovery. on the Galileo team expressed more personal * * * * * sentiments when she said, “I had never been a Michael Meltzer is an environmental part of something with such great scope . To scientist who has been writing about science know that the whole world was watching and and technology for nearly 30 years. His books hoping with us that this would work. We were and articles have investigated topics that include doing something for all mankind.” designing solar houses, preventing pollution in When Galileo lifted off from Kennedy electroplating shops, catching salmon with sonar and Space Center on 18 October 1989, it began an radar, and developing a sensor for examining Space interplanetary voyage that took it to Venus, to Michael Meltzer Michael Shuttle engines. -
Carl Sagan's Groovy Cosmos
CARL SAGAN’S GROOVY COSMOS: PUBLIC SCIENCE AND AMERICAN COUNTERCULTURE IN THE 1970S By SEAN WARREN GILLERAN A thesis submitted in partial fulfillment of the requirements for the degree of MASTER OF ARTS IN HISTORY WASHINGTON STATE UNIVERSITY Department of History MAY 2017 © Copyright by SEAN WARREN GILLERAN, 2017 All Rights Reserved © Copyright by SEAN WARREN GILLERAN, 2017 All Rights Reserved To the Faculty of Washington State University: The members of the Committee appointed to examine the thesis of SEAN WARREN GILLERAN find it satisfactory and recommend that it be accepted. _________________________________ Matthew A. Sutton, Ph.D., Chair _________________________________ Jeffrey C. Sanders, Ph.D. _________________________________ Lawrence B. A. Hatter, Ph.D. ii ACKNOWLEDGEMENT This thesis has been years in the making and is the product of input from many, many different people. I am grateful for the support and suggestions of my committee—Matt Sutton, Jeff Sanders, and Lawrence Hatter—all of whom have been far too patient, kind, and helpful. I am also thankful for input I received from Michael Gordin at Princeton and Helen Anne Curry at Cambridge, both of whom read early drafts and proposals and both of whose suggestions I have been careful to incorporate. Catherine Connors and Carol Thomas at the University of Washington provided much early guidance, especially in terms of how and why such a curious topic could have real significance. Of course, none of this would have happened without the support of Bruce Hevly, who has been extraordinarily generous with his time and whose wonderful seminars and lectures have continued to inspire me, nor without Graham Haslam, who is the best teacher and the kindest man I have ever known. -
ANTIFATT 15RAEL:C'f, 2 SALLYPORT-NOVEMBER
UN:VER:3I Association of Rice Alumni • November 1978 • Volume 35, Number 2 PIECING' _3,800yym 91-II5Ton ATTtLARIEK ANTIFATT 15RAEL:c'f, 2 SALLYPORT-NOVEMBER Dec. 7 North Harris Pc County — 5:30 St] Dec. 9 Angelina College — co; 5:30 — Away coi Jan. 12 St. Mary's — did 7:30 — Away ter Jan. 13 San Antonio fin 1:00 — Away MU SIC Jan. 16 SMU — ART 5:30 The Shepherd School of Music will continue te 18 Jan. Lamar — 7:00 its Fall Concert Season. All concerts take th 20 Nov. 1- "Pattern and Decoration," Jan. TCU — 2:00 place in Hanunan Hall at 8 P.M. unless an of 22 U of Houston — Dec. 13 featuring the works fifteen New Jan. otherwise noted. Concerts are free except his Away York artists. Sewall Gallery. 5:45 — when in conjunction with the Houston Friends by Jan. 8- "The Architecture of Gunnar As- Jan. 24 San Jacinto — 7:00 of Music. For more information call the Jan. 26 St. — Feb. 9 plund," an exhibition of the work of Mary's 7:00 Shepherd School Concert Line at 527-4933. Sweden's leading architect between Jan. 29 SMU — 5:00 — Away Nov. 28 Warren Deck, tuba. the two World Wars. A lecture by Mr. Jan. 31 Prairie View — 5:30 Paul Ellison, double bass. Stuart Wrede, curator of the exhibit Feb. 3 Lamar — 5:15 — Away Nov. 30 SYZYGY. Modern Art, for the Museum of New Swimming Dec. 4 Rice Symphony Orchestra. York, is planned. Sewall Gallery, Nov. 17 Rice Relays(W&M) Dec. -
NASA and Planetary Exploration
**EU5 Chap 2(263-300) 2/20/03 1:16 PM Page 263 Chapter Two NASA and Planetary Exploration by Amy Paige Snyder Prelude to NASA’s Planetary Exploration Program Four and a half billion years ago, a rotating cloud of gaseous and dusty material on the fringes of the Milky Way galaxy flattened into a disk, forming a star from the inner- most matter. Collisions among dust particles orbiting the newly-formed star, which humans call the Sun, formed kilometer-sized bodies called planetesimals which in turn aggregated to form the present-day planets.1 On the third planet from the Sun, several billions of years of evolution gave rise to a species of living beings equipped with the intel- lectual capacity to speculate about the nature of the heavens above them. Long before the era of interplanetary travel using robotic spacecraft, Greeks observing the night skies with their eyes alone noticed that five objects above failed to move with the other pinpoints of light, and thus named them planets, for “wan- derers.”2 For the next six thousand years, humans living in regions of the Mediterranean and Europe strove to make sense of the physical characteristics of the enigmatic planets.3 Building on the work of the Babylonians, Chaldeans, and Hellenistic Greeks who had developed mathematical methods to predict planetary motion, Claudius Ptolemy of Alexandria put forth a theory in the second century A.D. that the planets moved in small circles, or epicycles, around a larger circle centered on Earth.4 Only partially explaining the planets’ motions, this theory dominated until Nicolaus Copernicus of present-day Poland became dissatisfied with the inadequacies of epicycle theory in the mid-sixteenth century; a more logical explanation of the observed motions, he found, was to consider the Sun the pivot of planetary orbits.5 1. -
Publication Named Lunar Formations by Blagg and Müller (Published in 1935)
Lunar and Planetary Information Bulletin January 2018 • Issue 151 Contents Feature Story From the Desk of Jim Green News from Space Meeting Highlights Opportunities for Students Spotlight on Education In Memoriam Milestones New and Noteworthy Calendar Copyright 2018 The Lunar and Planetary Institute Issue 151 Page 2 of 76 January 2018 Feature Story Planetary Nomenclature: A Brief History and Overview Note from the Editors: This issue’s lead article is the ninth in a series of reports describing the history and current activities of the planetary research facilities partially funded by NASA and located nationwide. This issue provides a brief history and overview of planetary nomenclature, an important activity that provides structure and coordination to NASA’s planetary exploration program and the scientific analysis of planetary data. — Paul Schenk and Renée Dotson Humans have been naming the stars and planets for thousands of years, and many of these ancient names are still in use. For example, the Romans named the planet Mars for their god of war, and the satellites Phobos and Deimos, discovered in 1877, were named for the twin sons of Ares, the Greek god of war. In this age of orbiters, rovers, and high-resolution imagery, modern planetary nomenclature is used to uniquely identify a topographical, morphological, or albedo feature on the surface of a planet or satellite so that the feature can be easily located, described, and discussed by scientists and laypeople alike. History of Planetary Nomenclature With the invention of the telescope in 1608, astronomers from many countries began studying the Moon and other planetary bodies. -
NASA News National Aeronautics and Space Administration Washington, D.C
NASA News National Aeronautics and Space Administration Washington, D.C. 20546 AC 202 755-8370 For Release THURSDAY July 27, 1978 Pr6SS Kit Project Pioneer Venus 2 RELEASE NO: 78-101 CNASA-Ne»s-Eelease-78-101) SECOND VENOS N78-28105 SPACECBAFT SET FOB LAUNCH {National Aeronautics and Space Administration) 120 p CSCL 22A CJnclas 00/1_2 27327 Contents V* i GENERAL RELEASE ^At^S^T. 1-6 MISSION PROFILE 7-24 Pioneer Venus Multiprobe Mission 13-24 THE PLANET VENUS 25-40 MAJOR QUESTIONS ABOUT VENUS 41-42 HISTORICAL DISCOVERIES ABOUT VENUS 43-45 EXPLORATION OF VENUS BY SPACECRAFT 46-47 THE PIONEER VENUS SPACECRAFT 48-62 The Orbiter Spacecraft 53-58 The Multiprobe Spacecraft 58-62 VENUS ATMOSPHERIC PROBES 63-76 The Large Probe 63-70 The Small Probe 70-76 11 SCIENTIFIC INVESTIGATIONS 77-97 Orbiter 77-85 Orbiter Radio Science 85-88 Large Probe Experiments 88-92 Large and Small Probe Instruments 92-93 Small Probe Experiments 94 Multiprobe Bus Experiment 94-95 Multiprobe Radio Science Experiments 95-96 PRINCIPAL INVESTIGATORS AND SCIENTIFIC INSTRUMENTS 97-100 LAUNCH VEHICLE 101-102 LAUNCH FLIGHT SEQUENCE 102 LAUNCH VEHICLE CHARACTERISTICS , . 103 ATLAS CENTAUR FLIGHT SEQUENCE (AC-50) 104 LAUNCH OPERATIONS 105 MISSION OPERATIONS 105-107 DATA RETURN, COMMAND AND TRACKING 108-111 PIONEER VENUS TEAM 112-114 CONTRACTORS 114-117 VENUS STATISTICS 118 NOTE TO EDITORS; This press kit covers the launch phase of the Pioneer Venus Multiprobe spacecraft and cruise phases of both the Pioneer Venus Orbiter and the Multiprobe spacecraft. Much of the material is also pertinent to the Venus encounter, but an updated press kit will be issued shortly before arrival at the planet in December 1978. -
Planets Solar System Paper Contents
Planets Solar system paper Contents 1 Jupiter 1 1.1 Structure ............................................... 1 1.1.1 Composition ......................................... 1 1.1.2 Mass and size ......................................... 2 1.1.3 Internal structure ....................................... 2 1.2 Atmosphere .............................................. 3 1.2.1 Cloud layers ......................................... 3 1.2.2 Great Red Spot and other vortices .............................. 4 1.3 Planetary rings ............................................ 4 1.4 Magnetosphere ............................................ 5 1.5 Orbit and rotation ........................................... 5 1.6 Observation .............................................. 6 1.7 Research and exploration ....................................... 6 1.7.1 Pre-telescopic research .................................... 6 1.7.2 Ground-based telescope research ............................... 7 1.7.3 Radiotelescope research ................................... 8 1.7.4 Exploration with space probes ................................ 8 1.8 Moons ................................................. 9 1.8.1 Galilean moons ........................................ 10 1.8.2 Classification of moons .................................... 10 1.9 Interaction with the Solar System ................................... 10 1.9.1 Impacts ............................................ 11 1.10 Possibility of life ........................................... 12 1.11 Mythology ............................................. -
LUNAR and PLANETARY INFORMATION BULLETIN The
The Scar on Jupiter: Discovery of Comet Shoemaker Feature Story · From the Desk of Jim Green · News from Space · LPI 50th Anniversary Science Symposium Meeting Highlights · Spotlight on Education · In Memoriam · Milestones · New and Noteworthy · Calendar LUNAR AND PLANETARY INFORMATION BULLETIN April 2018 Issue 152 Issue 152 2 of 87 April 2018 Feature Story The Scar on Jupiter: Discovery of Comet Shoemaker-Levy 9 and Its Impact Into Jupiter 25 Years Later On March 24, 1993, in the midst of a photographic search for near-Earth objects at the fabled Palomar Observatory, Drs. Carolyn and Eugene Shoemaker and Dr. David Levy acquired an image in the vicinity of planet Jupiter using surplus film. This image surprised the observers when they first examined it. Expecting to find yet another small asteroid trail, they instead found an elongate object comprising several large clumps all strung out in a chain thousands of kilometers long in the night sky, each with its own cometary tail. Its orbital position proved to be quite close to Jupiter, and it did not take long to determine that it was in fact orbiting that giant planet and would come very close to the cloud tops the following year. The discovery of this strange comet was both serendipitous and completely unexpected, and the rest of the world was startled when the image was released three days later. No object like it had ever been seen before. It would be named P/Shoemaker-Levy 9 after its discoverers (SL- 9 for short). We had observed comets break apart during close encounters with the Sun into irregular clumps, but the linear geometry of this object indicated that it had passed very close to Jupiter in July 1992 and been ripped apart by tidal forces, something we had not observed or even predicted before. -
Fall 2019 Faculty News Around the Department
FALL 2019 GREETINGS FROM THE (OUTGOING) DEPARTMENT HEAD JULIE BRIGHAM-GRETTE Department Head Passing of the Torch! FACULTY NEWS New Faculty As we start another academic year, the Department of Justin Richardson Geosciences has much to celebrate! We have created Seda Şalap – Ayça opportunities to broaden our research and teaching Stephen Turner mission with the addition of new faculty, renovated old Matthew Winnick spaces, and new instrumentation needed to drive discovery. In this newsletter you will meet our new faculty and learn about some of the research that feeds our curiosity while also training students with relevant and IN MEMORIAM rigorous tools to tackle local to global challenges in building a sustainable world. As a department that is Pete Robinson home to the academic disciplines of geology and John Hubert geography, we bring diverse perspectives and methods to Sheila Seaman examining the inter-relationships between the environment and societies, economies, George McGill and cultures. We do this traveling the globe! The Earth and its people are our office and classroom. The growth in our Geographic Information Systems program includes a new faculty member teaching at the new UMass-Amherst Mt. Ida campus! AROUND THE We also enter the Fall in mourning as we cope with the untimely passing of Dr. Sheila Seaman in late July. We will miss this outstanding, award-winning professor for her DEPARTMENT bravery to never give up, and for her heart to always find the best in everyone. Sheila’s kindness was without end. We also mourn the passing of several of our dear Geology News emeritus faculty – John Hubert, George McGill, and Peter Robinson – on who’s Geography News News from the State shoulders we maintain the strength of the department and their legacies. -
X Band Model of Venus Atmosphere Permittivity
RADIO SCIENCE, VOL. 45, RS2003, doi:10.1029/2009RS004169, 2010 Click Here for Full Article X band model of Venus atmosphere permittivity Xueyang Duan,1 Mahta Moghaddam,1 Daniel Wenkert,2 Rolando L. Jordan,2 and Suzanne E. Smrekar2 Received 5 March 2009; revised 3 November 2009; accepted 18 November 2009; published 2 April 2010. [1] A model of Venus’ atmosphere permittivity profile up to 300 km is developed in this paper for X band. The model includes both the real and imaginary parts of the atmospheric permittivity, derived using data sets inferred or directly measured from past exploration missions to Venus: the real part is obtained by calculating the total polarization of the mixture of the atmospheric components including CO2,N2, H2O, SO2,H2SO4, CO, etc.; the imaginary part is derived using the superposition of the absorption of each component. The properties of the atmospheric components such as polarization and absorption are modeled with respect to frequency, temperature, and pressure. The validity of this model is verified by comparing simulation results with available measurements of Venus’ atmosphere. This permittivity model is intended as a critical tool for the design of next‐generation orbiting radar systems, in particular interferometric radars. Citation: Duan, X., M. Moghaddam, D. Wenkert, R. L. Jordan, and S. E. Smrekar (2010), X band model of Venus atmosphere permittivity, Radio Sci., 45, RS2003, doi:10.1029/2009RS004169. 1. Introduction small fraction of the planet; also, the stereo data have only limited relative vertical precision (∼10 m) [Howington‐ [2] During the past 30 years, several satellite missions Kraus et al., 2001]. -
Astronautics and Aeronautics, 1979-1984
ASTRONAUTICS AND AERONAUTICS, I9794984 A Chronology by Bette R. Janson and Eleanor H. Ritchie THE NASA HISTORY SERIES National Aeronautics and Space Administration Office of Management NASA Scientific and Technical information Division Washington, DC 1990 NASA maintains an internal history program for two principal reasons. (1) Spon- sorship of research in NASA-related history is one wiy in which NASA responds to the provision of the National Aeronautics and :Space Act of 1958 that re- quires NASA to “provide for the widest practicable and appropriate dissemina- tion of information concerning its activities and the results thereof.” (2) Thoughtful study of NASA history can help agency managers accomplish the missions assigned to the agency. Understanding NASA’s past aids in understan- ding its present situation and illuminates possible future directions. Selection of items for inclusion in the chronology is the responsibility of the History Office employee assigned to assemble them; omission or manner of treatment has no relationship to agency policy. For sale by the Superintendent of Documents, US. Government Printing Office, Washington, D.C. 20402 (paper cover). Library of Congress catalog number 656038 Preface Astronautics ana' Aeronautics for 159-1984 completes the series of annual chronologies of events in aeronautics, aviation, and space science and explora- tion prepared by the History Division of the National Aeronautics and Space Administration since 1961. The concluding volume of the series, Astronautics and Aeronautics for 1985, was published in 1988. The present volume was written by Bette R. Janson and Eleanor H. Ritchie under the editorial supervision of the director of the NASA History Division. -
John D. Mihalov Papers, 1960-1997
http://oac.cdlib.org/findaid/ark:/13030/kt7f59s32f No online items Guide to the John D. Mihalov Papers, 1960-1997 Guide prepared by Holly (Thomason) Trechter NASA Ames History Office NASA Ames Research Center Mail Stop 207-1 Moffett Field, California 94035 Phone: (650) 604-1032 Email: [email protected] URL: http://history.arc.nasa.gov ©2011 NASA Ames Research Center. All rights reserved. Guide to the John D. Mihalov PP05.22-JM 1 Papers, 1960-1997 Guide to the John D. Mihalov Papers, 1960-1997 NASA Ames History Office NASA Ames Research Center Contact Information: NASA Ames History Office NASA Ames Research Center Mail Stop 207-1 Moffett Field, CA 94035 Phone: (650) 604-1032 Email: [email protected] URL: http://history.arc.nasa.gov Collection processed by: Holly (Thomason) Trechter Date Completed: May 2011 Descriptive Summary Title: John D. Mihalov Papers Date (inclusive): 1960-1997 Collection Number: PP05.22-JM Creator: Mihalov, John D. (John Donald) Extent: Volume: 18 cubic feet Repository: Ames Research Center, Ames History Office Moffett Field, California 94035 Abstract: The John D. Mihalov Papers include record books, meeting notes, project proposals, correspondence, design reviews, experiment plans, circuit diagrams, instrument descriptions, test reports, data, charts, plots, presentations for international meetings, publications, peer reviews, press kits, and reference materials documenting Mihalov's solar physics contributions to Pioneers 6 through 11, Pioneer 12 (Pioneer Venus Orbiter), and the Galileo Probe during his career as a research scientist at the NASA Ames Research Center. Language: English Access Collection is open for research.