The Planetary Report Is Published Six Times Yearly G, Edward Danielson, Found the Comet on October 16, 1982, and Verified Their Observations on October 19
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Appendix 1: Venus Missions
Appendix 1: Venus Missions Sputnik 7 (USSR) Launch 02/04/1961 First attempted Venus atmosphere craft; upper stage failed to leave Earth orbit Venera 1 (USSR) Launch 02/12/1961 First attempted flyby; contact lost en route Mariner 1 (US) Launch 07/22/1961 Attempted flyby; launch failure Sputnik 19 (USSR) Launch 08/25/1962 Attempted flyby, stranded in Earth orbit Mariner 2 (US) Launch 08/27/1962 First successful Venus flyby Sputnik 20 (USSR) Launch 09/01/1962 Attempted flyby, upper stage failure Sputnik 21 (USSR) Launch 09/12/1962 Attempted flyby, upper stage failure Cosmos 21 (USSR) Launch 11/11/1963 Possible Venera engineering test flight or attempted flyby Venera 1964A (USSR) Launch 02/19/1964 Attempted flyby, launch failure Venera 1964B (USSR) Launch 03/01/1964 Attempted flyby, launch failure Cosmos 27 (USSR) Launch 03/27/1964 Attempted flyby, upper stage failure Zond 1 (USSR) Launch 04/02/1964 Venus flyby, contact lost May 14; flyby July 14 Venera 2 (USSR) Launch 11/12/1965 Venus flyby, contact lost en route Venera 3 (USSR) Launch 11/16/1965 Venus lander, contact lost en route, first Venus impact March 1, 1966 Cosmos 96 (USSR) Launch 11/23/1965 Possible attempted landing, craft fragmented in Earth orbit Venera 1965A (USSR) Launch 11/23/1965 Flyby attempt (launch failure) Venera 4 (USSR) Launch 06/12/1967 Successful atmospheric probe, arrived at Venus 10/18/1967 Mariner 5 (US) Launch 06/14/1967 Successful flyby 10/19/1967 Cosmos 167 (USSR) Launch 06/17/1967 Attempted atmospheric probe, stranded in Earth orbit Venera 5 (USSR) Launch 01/05/1969 Returned atmospheric data for 53 min on 05/16/1969 M. -
CARL ZIMMER Author & Journalist
CARL ZIMMER Author & journalist carlzimmer.com @carlzimmer BIOGRAPHY The New York Times Book Review calls Carl Zimmer "as fine a science essayist as we have." He is the author of thirteen acclaimed books and a columnist for the New York Times. Zimmer first be- gan writing about science at Discover, where he served for five years as a senior editor, and has gone on to write hundreds of features for magazines including The Atlantic, The New York Times Magazine, Time, National Geographic, and Scientific American. He has also served as a scientific editor for television documentaries, consulted on museum exhibits, and contributed his writing to major science web sites. Zimmer has earned numerous honors for his work. In 2007 he won the National Academies Communication Award, and he has won the American Association for the Advancement of Sci- ences Science Journalism Award three times. In 2015, Zimmer won the Distinguished Service Award from the National Association of Biology Teachers, and in 2016, he won the Stephen Jay Gould Prize, awarded by the Society for the Study of Evolution. In 2018, Zimmer’s book She Has Her Mother’s Laugh was named by Publisher’s Weekly one of the ten best books of the year. The Guardian named it the best science book of 2018 and The New York Times Book Review chose it as a Notable Book of the Year. It was short-listed for the Baillie-Gifford Prize for Nonfiction and a fi- nalist for the PEN/E.O. Wilson Literary Science Writing Prize. His articles have been antholo- gized in both The Best American Science and Nature Writing series and The Best American Science Writing series. -
Habitable Zone ? UE Zu Habitable Planeten Präsentation 1
Venus Habitable Zone ? UE zu Habitable Planeten Präsentation 1. Juni 2006 Eisenkölbl, Grohs, Hren, Lendl Venus 1. Raumsonden zur Venus Überblick • Raumfahrt zur Venus – Allgemeines – Beweggründe – Technische Hintergründe • Venus – Missionen – Zeittafel und Überblick – erfolgreiche Missionen – Zukünftige Missionen Raumfahrt zur Venus Allgemeines • Venus ist der meistbesuchte Planet in unserem Sonnensystem. (~ 25 erfolgreiche Missionen von 44) • Heutige Daten der Venus sind ein Ergebnis der zahlreichen Raummissionen Raumfahrt zur Venus Beweggründe • Dichte Wolkendecke – keine Beobachtungsmöglichkeit von der Erde aus im sichtbaren Licht • Vorstellung von Leben auf Venus • Suche nach habitabler Zone • Ressourcensuche Raumfahrt zur Venus technische Hintergründe • Venus ist der Planet mit der geringsten Entfernung von der Erde – Minimum 38.2 x 106 km – Maximum 261.0 x 106 km • Sonden leisten Pionierarbeit – Erprobung von Raumsonden • Technik • Material • Bauart Raumfahrt zur Venus – Zeittafel 1 (1961-1967) 1961 Sputnik 7 - 4 February 1961 - Attempted Venus Impact Venera 1 - 12 February 1961 - Venus Flyby (Contact Lost) 1962 Mariner 1 - 22 July 1962 - Attempted Venus Flyby (Launch Failure) Sputnik 19 - 25 August 1962 - Attempted Venus Flyby Mariner 2 - 27 August 1962 - Venus Flyby Sputnik 20 - 1 September 1962 - Attempted Venus Flyby Sputnik 21 - 12 September 1962 - Attempted Venus Flyby 1963 Cosmos 21 - 11 November 1963 - Attempted Venera Test Flight? 1964 Venera 1964A - 19 February 1964 - Attempted Venus Flyby (Launch Failure) Venera 1964B -
Dsc Pub Edited
1965 50) just 24 kilometers from its intended target Ranger 8 point in the equatorial region of the Sea of Nation: U.S. (21) Tranquillity—an area that Apollo mission Objective(s): lunar impact planners were particularly interested in Spacecraft: Ranger-C studying. Spacecraft Mass: 366.87 kg Mission Design and Management: NASA JPL 51) Launch Vehicle: Atlas-Agena B (no. 13 / Atlas “Atlas-Centaur 5” D no. 196 / Agena B no. 6006) Nation: U.S. (22) Launch Date and Time: 17 February 1965 / Objective(s): highly elliptical orbit 17:05:00 UT Spacecraft: SD-1 Launch Site: ETR / launch complex 12 Spacecraft Mass: 951 kg Scientific Instruments: Imaging system (six TV Mission Design and Management: NASA JPL cameras) Launch Vehicle: Atlas-Centaur (AC-5 / Atlas C Results: As successful as its predecessor, no. 156D / Centaur C) Ranger 8 returned 7,137 high-resolution pho- Launch Date and Time: 2 March 1965 / tographs of the lunar surface prior to its 13:25 UT scheduled impact at 09:57:37 UT on 20 Launch Site: ETR / launch complex 36A February. Unlike Ranger 7, however, Ranger 8 Scientific Instruments: none turned on its cameras about 8 minutes earlier Results: This mission was designed to rehearse a to return pictures with resolution comparable complete Centaur upper-stage burn in support to Earth-based telescopes (for calibration and of the Surveyor lunar lander program. On a comparison purposes). Controllers attempted nominal mission, the Centaur would boost its to align the cameras along the main velocity payload on a direct-ascent trajectory to the vector (to reduce imagine smear) but aban- Moon. -
A Missing Star
A Volume 7, Number f. March 1997 Ithaca, New York FREE A Missing Star Paul West Certain much-heard voices impose themselves on posterity. My old friend, astronomer Carl Sagan, had such a voice: a tutored baritone no doubt practiced in bathroom or laboratory, bouncing about among tile and glass, a calmative among the wets and clinks, the squeaky faucets and the hoarse Bunsen burners. In the old days, when he never wore a suit, the voice wasn’t quite so manicured, so crisply mahogany in hue, when we chatted about salary, Swinburne, and stars, and in a much later year I wondered how that voice had fared when, reduced to heart broken banality, he found himself saying to his dying father, “Take care.” I knew his parents quite well, having become a fan of his mother’s potato pancakes, of his father’s burly wit; besides, his mother, Rachel, knew my books and urged them upon her son, who complied, I live in a house only a short downhill walk from where Carl now lies horizontal in a box, still a neighbor I suppose, motionless and dumb. And this new image of him fills me with ontological horror that his cherished cosmos has done this to him at sixty-two, renewing Beck ett’s warning that death does not require us to keep a day free in the calendar. We abide its w him and its deadly design with what the Greeks called frike, a hair-rais ing shudder, and then hope to think of something else. Surely it is naive of me, child of the Nazi blitz, to feel such shock and outrage at the demolition month by month of a friend. -
Venus Exploration Themes
Venus Exploration Themes VEXAG Meeting #11 November 2013 VEXAG (Venus Exploration Analysis Group) is NASA’s community‐based forum that provides science and technical assessment of Venus exploration for the next few decades. VEXAG is chartered by NASA Headquarters Science Mission Directorate’s Planetary Science Division and reports its findings to both the Division and to the Planetary Science Subcommittee of NASA’s Advisory Council, which is open to all interested scientists and engineers, and regularly evaluates Venus exploration goals, objectives, and priorities on the basis of the widest possible community outreach. Front cover is a collage showing Venus at radar wavelength, the Magellan spacecraft, and artists’ concepts for a Venus Balloon, the Venus In‐Situ Explorer, and the Venus Mobile Explorer. (Collage prepared by Tibor Balint) Perspective view of Ishtar Terra, one of two main highland regions on Venus. The smaller of the two, Ishtar Terra, is located near the north pole and rises over 11 km above the mean surface level. Courtesy NASA/JPL–Caltech. VEXAG Charter. The Venus Exploration Analysis Group is NASA's community‐based forum designed to provide scientific input and technology development plans for planning and prioritizing the exploration of Venus over the next several decades. VEXAG is chartered by NASA's Solar System Exploration Division and reports its findings to NASA. Open to all interested scientists, VEXAG regularly evaluates Venus exploration goals, scientific objectives, investigations, and critical measurement requirements, including especially recommendations in the NRC Decadal Survey and the Solar System Exploration Strategic Roadmap. Venus Exploration Themes: November 2013 Prepared as an adjunct to the three VEXAG documents: Goals, Objectives and Investigations; Roadmap; as well as Technologies distributed at VEXAG Meeting #11 in November 2013. -
Venus Exploration Themes: September 2011
Venus Exploration Themes Adjunct to Venus Exploration Goals and Objectives 2011 September 2011 Fifty Years of Venus Missions Venus Exploration Vignettes Technologies for Venus Exploration Front cover is a collage showing Venus at radar wavelength, the Magellan spacecraft, and artists’ concepts for a Venus Balloon, the Venus In Situ Explorer, and the Venus Mobile Explorer. (Collage prepared by Tibor Balint) Perspective view of Ishtar Terra, one of two main highland regions on Venus. The smaller of the two, Ishtar Terra, is located near the north pole and rises over 11 km above the mean surface level. Courtesy NASA/JPL–Caltech. Venus Exploration Themes: September 2011 Prepared as an adjunct to the Venus Exploration Goals and Objectives document to preserve extracts from the October 2009 Venus Exploration Pathways document. TABLE OF CONTENTS Table of Contents ........................................................................................................................... iii Fifty Years of Venus Missions ....................................................................................................... 1 Venus Exploration Vignettes .......................................................................................................... 3 Vignette 1: Magellan ................................................................................................................... 3 Vignette 2: Experiencing Venus by Air: The Advantages of Balloon-Borne In Situ Exploration .............................................................................................................. -
Venus Exploration Goals, Objectives, Investigations, and Priorities: 2007
Venus Exploration Goals, Objectives, Investigations, and Priorities: 2007 A Report of the Venus Exploration Analysis Group (VEXAG) October 2007 VEXAG is NASA’s community-based forum, which provides science input for planning and prioritizing Venus exploration for the next few decades. VEXAG is chartered by NASA Headquarters Planetary Science Division and reports its findings to both the Division and to the Planetary Science Sub-Committee of the NASA Advisory Council. VEXAG, which is open to all interested scientists and engineers, regularly evaluates Venus exploration goals, objectives, investigations and priorities on the basis of the widest possible community outreach. http://www.lpi.usra.edu/vexag Front cover is a collage showing Venus at optical wavelength, the Magellan spacecraft, and artists’ concepts for a Venus Balloon, the Venus In-Situ Explorer, and the Venus Mobile Explorer. Venus Exploration Goals, Objectives, Investigations, and Priorities: 2007 VEXAG (Venus Exploration Analysis Group) October 2007 Prepared by the VEXAG (Venus Exploration Analysis Group) Organizing Committee: Janet Luhmann, VEXAG Co-Chair, University of California, Berkeley, California ([email protected]) Sushil Atreya, VEXAG Co-Chair, University of Michigan, Ann Arbor, Michigan ([email protected]) Steve Mackwell, Focus Group Lead for Planetary Formation and Evolution, Lunar and Planetary Institute, Houston, Texas ([email protected]) Kevin Baines, Focus Group Lead for Atmospheric Evolution, JPL, Pasadena, California ([email protected]) James Cutts, Focus Group Lead for Venus Exploration Technologies, JPL, Pasadena, California ([email protected]) Adriana Ocampo, Venus Program Executive, NASA Headquarters, Washington DC. ([email protected]) Other supporting members of the VEXAG Organizing Committee are: Tibor Balint, JPL; Mark Bullock, Southwest Research Institute, Boulder, Colorado; Larry Esposito, LASP, University of Colorado; Ellen Stofan, Proxemy, Inc.; Tommy Thompson, JPL. -
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. -
ISU Team Project
Additional copies of the Project Report or the Executive Summary for this project may be ordered from the International Space University (ISU) Headquarters. The Executive Summary and the Project Report also can be found on the ISU website. International Space University Strasbourg Central Campus Attention: Publications Parc d’Innovation 1 rue Jean-Dominque Cassini 67400 Illkirch-Graffenstaden France Tel : +33 (0)3 88 65 54 30 Fax: +33(0) 88 65 54 47 http://www.isunet.edu Copyright 2003 by the International Space University All Rights Reserved TRACKS TO SPACE ACKNOWLEDGEMENTS The following individuals and organisations have generously contributed their time, resources, expertise and facilities to help us make TRACKS to Space possible. PROJECT SPONSOR European Space Agency — Industrial Matters and Technology Programmes Hans Kappler Director Marco Guglielmi Head of Technology Strategy Section Marco Freire Technology Strategy Engineer PROJECT FACULTY AND TA Project Initiator Walter Peeters Co-chair Nicolas Peter Co-chair Ray Williamson Teaching Associate Philippos Beveratos English Tutor Sarah Delaveaud English Tutor Carol Carnett EXTERNAL EXPERTS Andrew Aldrin Boeing, NASA Systems Randall Correll Science Applications International Corporation Dan Glover NASA Glenn Research Center Tetsuichi Ito NASDA, ISU Faculty Joan Johnson-Freese United States Naval War College Chiaki Mukai NASDA Astronaut Ichiro Nakatani Institute of Space and Astronautical Science (ISAS) Jean-Claude Piedboeuf Canadian Space Agency Roy Sach Director Defence Space, Australia Gongling Sun EurasSpace GmbH Simon P. Worden Brigadier General, United States Air Force PERSONAL THANKS The authors would like to extend a heartfelt thanks to those who made the greatest sacrifices during this two-month space odyssey. -
Submitted Draft That Was Published As “Cruisin’ the Solar System: the Past and Future of Planetary Exploration”, Ad Astra, Volume 12, Number 2, Pp
"Visiting Our Neighbors: A History of Planetary Exploration" by Andrew J. LePage Submitted draft that was published as “Cruisin’ The Solar System: The Past and Future of Planetary Exploration”, Ad Astra, Volume 12, Number 2, pp. 25-29, March/April 2000 The First Steps For much of the first half of the Twentieth Century, planetary studies were a quiet backwater in the field of astronomy. But the confluence of rapidly advancing rocket technology and Cold War competition at the dawn of the Space Age was about change that. The technology finally existed to send probes to the planets and make useful close up observations - a development which would totally transform our understanding of all the planets including Earth. By 1960, NASA planners hoped to flyby Venus in 1962 and Mars in 1964 with heavily instrumented half-ton probes called Mariner using the powerful Atlas-Centaur then under development. Ambitious Soviet engineers This Soviet model is representative of their early Object MV probe design. The planetary compartment at the bottom intended to send two or more spacecraft could carry a package of cameras as here or a simple towards Mars and Venus during every launch lander. (NASA) window using their new Molniya rocket. Unfortunately launch vehicle failures doomed Before the end of 1961, NASA's plans were the first pair of Soviet Mars flyby probes already in trouble because of lagging Atlas- launched in October of 1960 and stranded their Centaur development. With only the Atlas- first Venus probe in Earth orbit the following Agena available, Mariner had to shed half its February. -
Low-Frequency Turbulence in the Anisotropic Plasma Namig Dzhalilov
Solar Wind: Low-frequency Turbulence in the Anisotropic Plasma Namig Dzhalilov Shamakhy Astrophysical Observatory, Azerbaijan 1 A g e n d a • Global structure of the heliosphere - general views • Solar wind measurements • The solar wind as a turbulence laboratory • MHD - Wave instability theory • Conclusions 2 3 The solar corona • Hot rarefied atmosphere above visible surface • Plasma beta <<1 in corona • magnetic field dominates • Closed magnetic field: plasma trapped • Open magnetic field: plasma can expand into interplanetary space 4 Eclipse: RED 1.1 106 K Iron X‐XI (RED) GREEN 2 106 K Iron XIII‐XIV (GREEN) This eclipse image shows the magnetic topology of the corona. 5 There is a clear separation of the high and low latitude solar wind. 6 This SOHO extreme ultraviolet (EIT) and scattered visible light (LASCO) composite image shows the outward streaming solar corona forming the supersonic solar wind 7 Expansion of the upper corona • Corona is very hot • Pressure is higher than ambient interstellar medium • Expands into interplanetary space (Parker, 1958): solar wind • Carves a cavity in interstellar medium: heliosphere • Nearly radial flow • Accelerates to full speed by ~20 solar radii SoHO coronagraph (LASCO) Artificial eclipse 8 9 What is the solar wind? • Collisionless, magnetised plasma • Continual, but variable, outflow from Sun’s corona • Blows a cavity in interstellar medium: heliosphere • Carries magnetic field, waves and turbulence from Sun’s corona • At edge of heliosphere, merges with interstellar medium • Interacts with