Summary of Russian Planetary Lander Missions by Tibor Balint, Deep Space Mission Architecture Group, 311B, NASA-JPL December 19, 2002
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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. -
Jjmonl 1603.Pmd
alactic Observer GJohn J. McCarthy Observatory Volume 9, No. 3 March 2016 GRAIL - On the Trail of the Moon's Missing Mass GRAIL (Gravity Recovery and Interior Laboratory) was a NASA scientific mission in 2011/12 to map the surface of the moon and collect data on gravitational anomalies. The image here is an artist's impres- sion of the twin satellites (Ebb and Flow) orbiting in tandem above a gravitational image of the moon. See inside, page 4 for information on gravitational anomalies (mascons) or visit http://solarsystem. nasa.gov/grail. The John J. McCarthy Observatory Galactic Observer New Milford High School Editorial Committee 388 Danbury Road Managing Editor New Milford, CT 06776 Bill Cloutier Phone/Voice: (860) 210-4117 Production & Design Phone/Fax: (860) 354-1595 www.mccarthyobservatory.org Allan Ostergren Website Development JJMO Staff Marc Polansky It is through their efforts that the McCarthy Observatory Technical Support has established itself as a significant educational and Bob Lambert recreational resource within the western Connecticut Dr. Parker Moreland community. Steve Barone Jim Johnstone Colin Campbell Carly KleinStern Dennis Cartolano Bob Lambert Mike Chiarella Roger Moore Route Jeff Chodak Parker Moreland, PhD Bill Cloutier Allan Ostergren Cecilia Dietrich Marc Polansky Dirk Feather Joe Privitera Randy Fender Monty Robson Randy Finden Don Ross John Gebauer Gene Schilling Elaine Green Katie Shusdock Tina Hartzell Paul Woodell Tom Heydenburg Amy Ziffer In This Issue "OUT THE WINDOW ON YOUR LEFT" ............................... 4 SUNRISE AND SUNSET ...................................................... 13 MARE HUMBOLDTIANIUM AND THE NORTHEAST LIMB ......... 5 JUPITER AND ITS MOONS ................................................. 13 ONE YEAR IN SPACE ....................................................... 6 TRANSIT OF JUPITER'S RED SPOT .................................... -
Jjmonl 1710.Pmd
alactic Observer John J. McCarthy Observatory G Volume 10, No. 10 October 2017 The Last Waltz Cassini’s final mission and dance of death with Saturn more on page 4 and 20 The John J. McCarthy Observatory Galactic Observer New Milford High School Editorial Committee 388 Danbury Road Managing Editor New Milford, CT 06776 Bill Cloutier Phone/Voice: (860) 210-4117 Production & Design Phone/Fax: (860) 354-1595 www.mccarthyobservatory.org Allan Ostergren Website Development JJMO Staff Marc Polansky Technical Support It is through their efforts that the McCarthy Observatory Bob Lambert has established itself as a significant educational and recreational resource within the western Connecticut Dr. Parker Moreland community. Steve Barone Jim Johnstone Colin Campbell Carly KleinStern Dennis Cartolano Bob Lambert Route Mike Chiarella Roger Moore Jeff Chodak Parker Moreland, PhD Bill Cloutier Allan Ostergren Doug Delisle Marc Polansky Cecilia Detrich Joe Privitera Dirk Feather Monty Robson Randy Fender Don Ross Louise Gagnon Gene Schilling John Gebauer Katie Shusdock Elaine Green Paul Woodell Tina Hartzell Amy Ziffer In This Issue INTERNATIONAL OBSERVE THE MOON NIGHT ...................... 4 SOLAR ACTIVITY ........................................................... 19 MONTE APENNINES AND APOLLO 15 .................................. 5 COMMONLY USED TERMS ............................................... 19 FAREWELL TO RING WORLD ............................................ 5 FRONT PAGE ............................................................... -
Long-Term Venus Lander
Western Michigan University ScholarWorks at WMU Honors Theses Lee Honors College 4-20-2021 Long-Term Venus Lander Scott Miller Western Michigan University, [email protected] Follow this and additional works at: https://scholarworks.wmich.edu/honors_theses Part of the Space Vehicles Commons Recommended Citation Miller, Scott, "Long-Term Venus Lander" (2021). Honors Theses. 3383. https://scholarworks.wmich.edu/honors_theses/3383 This Honors Thesis-Open Access is brought to you for free and open access by the Lee Honors College at ScholarWorks at WMU. It has been accepted for inclusion in Honors Theses by an authorized administrator of ScholarWorks at WMU. For more information, please contact [email protected]. Long-Duration Venus Explorer Aidan Wales, Ethan Reid, and Scott Miller Group #04-21-01 Faculty Advisor: Dr. Kristina Lemmer Western Michigan University College of Engineering and Applied Sciences Table of Contents Abstract .............................................................................................................. pg. 1 Disclaimer .......................................................................................................... pg. 1 Introduction ....................................................................................................... pg. 2 Methodology ...................................................................................................... pg. 2 Preliminary Research ............................................................................. pg. 2 Decision Matrices -
18Th Meeting of the Venus Exploration Analysis Group (Vexag)
18TH MEETING OF THE VENUS EXPLORATION ANALYSIS GROUP (VEXAG) Program and Abstracts LPI Contribution No. 2356 18th Meeting of the Venus Exploration Analysis Group November 16–17, 2020 Institutional Support Lunar and Planetary Institute Universities Space Research Association Convener Noam Izenberg Johns Hopkins Applied Physics Laboratory Darby Dyar Mount Holyoke College Science Organizing Committee Darby Dyar Planetary Science Institute, Mount Holyoke College Noam Izenberg JHU Applied Physics Laboratory Megan Andsell NASA Headquarters Natasha Johnson NASA Goddard Jennifer Jackson California Institute of Technology Jim Cutts Jet Propulsion Laboratory Tommy Thompson Jet Propulsion Laboratory Lunar and Planetary Institute 3600 Bay Area Boulevard Houston TX 77058-1113 Compiled in 2020 by Meeting and Publication Services Lunar and Planetary Institute USRA Houston 3600 Bay Area Boulevard, Houston TX 77058-1113 This material is based upon work supported by NASA under Award No. 80NSSC20M0173. Any opinions, findings, and conclusions or recommendations expressed in this volume are those of the author(s) and do not necessarily reflect the views of the National Aeronautics and Space Administration. The Lunar and Planetary Institute is operated by the Universities Space Research Association under a cooperative agreement with the Science Mission Directorate of the National Aeronautics and Space Administration. Material in this volume may be copied without restraint for library, abstract service, education, or personal research purposes; however, republication of any paper or portion thereof requires the written permission of the authors as well as the appropriate acknowledgment of this publication. ISSN No. 0161-5297 Abstracts for this meeting are available via the meeting website at https://www.hou.usra.edu/meetings/vexag2020/ Abstracts can be cited as Author A. -
Terrestrial Planets 1- 4 from the Sun Mercury in Sight
Terrestrial Planets 1- 4 from the Sun Image courtesy: http://commons.wikimedia.org/wiki/Image:Terrestrial_planet_size_comparisons_edit.jpg First ever ‘whole Earth’ picture from deep space, taken by Bill Anders on Apollo 8 Apollo 8 crew, Bill Anders centre: courtesy Nasa Mercury, Venus, Earth and Mars are four The Earth is just a planet astonishingly different planets Mercury and Venus have only been seen in any detail within the last 30 years Mercury in sight Mercury Mercury is like the Earth inside and the Moon outside Courtesy NASA (Mariner 10) Mercury has had a cooling and bombardment history Mercury is visible only soon after the setting similar to the moon sun or shortly before dawn It appears as cratered lava the Mariner 10 probe (1974/75) is the source of most information about Mercury – Messenger, launched 2004, with scarps first flypast in 2008 and orbit Mercury in 2011. ESA’s Its rocks are Earth-like BepiColombo, to be launched in 2013 Mariner 10 image Messenger images Messenger image ↑ Double-ringed crater – a Mercury feature courtesy: http://messenger.jhuapl.edu/gallery/sciencePhotos/pics/S trom02.jpg ← Courtesy: http://messenger.jhuapl.edu/gal lery/sciencePhotos/pics/EN010 8828161M.jpg Courtesy: http://messenger.jhuapl.edu/gallery/sciencePhotos/pics/Prockter06.jpg Messenger image Mercury Close-up Mercury’s topography was formed under stronger The gravity than on the Moon caloris The Caloris basin is an impact crater ~1400 km across, basin is the beneath which is thought to be a dense mass large 2 Mercury’s rotation period is exactly /3 of its orbital circular period of 87.97 days. -
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 -
Deep Space Chronicle Deep Space Chronicle: a Chronology of Deep Space and Planetary Probes, 1958–2000 | Asifa
dsc_cover (Converted)-1 8/6/02 10:33 AM Page 1 Deep Space Chronicle Deep Space Chronicle: A Chronology ofDeep Space and Planetary Probes, 1958–2000 |Asif A.Siddiqi National Aeronautics and Space Administration NASA SP-2002-4524 A Chronology of Deep Space and Planetary Probes 1958–2000 Asif A. Siddiqi NASA SP-2002-4524 Monographs in Aerospace History Number 24 dsc_cover (Converted)-1 8/6/02 10:33 AM Page 2 Cover photo: A montage of planetary images taken by Mariner 10, the Mars Global Surveyor Orbiter, Voyager 1, and Voyager 2, all managed by the Jet Propulsion Laboratory in Pasadena, California. Included (from top to bottom) are images of Mercury, Venus, Earth (and Moon), Mars, Jupiter, Saturn, Uranus, and Neptune. The inner planets (Mercury, Venus, Earth and its Moon, and Mars) and the outer planets (Jupiter, Saturn, Uranus, and Neptune) are roughly to scale to each other. NASA SP-2002-4524 Deep Space Chronicle A Chronology of Deep Space and Planetary Probes 1958–2000 ASIF A. SIDDIQI Monographs in Aerospace History Number 24 June 2002 National Aeronautics and Space Administration Office of External Relations NASA History Office Washington, DC 20546-0001 Library of Congress Cataloging-in-Publication Data Siddiqi, Asif A., 1966 Deep space chronicle: a chronology of deep space and planetary probes, 1958-2000 / by Asif A. Siddiqi. p.cm. – (Monographs in aerospace history; no. 24) (NASA SP; 2002-4524) Includes bibliographical references and index. 1. Space flight—History—20th century. I. Title. II. Series. III. NASA SP; 4524 TL 790.S53 2002 629.4’1’0904—dc21 2001044012 Table of Contents Foreword by Roger D. -
The Science Return from Venus Express the Science Return From
The Science Return from Venus Express Venus Express Science Håkan Svedhem & Olivier Witasse Research and Scientific Support Department, ESA Directorate of Scientific Programmes, ESTEC, Noordwijk, The Netherlands Dmitri V. Titov Max Planck Institute for Solar System Studies, Katlenburg-Lindau, Germany (on leave from IKI, Moscow) ince the beginning of the space era, Venus has been an attractive target for Splanetary scientists. Our nearest planetary neighbour and, in size at least, the Earth’s twin sister, Venus was expected to be very similar to our planet. However, the first phase of Venus spacecraft exploration (1962-1985) discovered an entirely different, exotic world hidden behind a curtain of dense cloud. The earlier exploration of Venus included a set of Soviet orbiters and descent probes, the Veneras 4 to14, the US Pioneer Venus mission, the Soviet Vega balloons and the Venera 15, 16 and Magellan radar-mapping orbiters, the Galileo and Cassini flybys, and a variety of ground-based observations. But despite all of this exploration by more than 20 spacecraft, the so-called ‘morning star’ remains a mysterious world! Introduction All of these earlier studies of Venus have given us a basic knowledge of the conditions prevailing on the planet, but have generated many more questions than they have answered concerning its atmospheric composition, chemistry, structure, dynamics, surface-atmosphere interactions, atmospheric and geological evolution, and plasma environment. It is now high time that we proceed from the discovery phase to a thorough -
Planetary Science Division Update to VEXAG
Planetary Science Division Update to VEXAG Jim Green August 29, 2011 The Environment We Are In • Congress has started debang NASA’s budget for FY12 • The House has a proposed NASA budget from its Subcommiee • We expect to be under a “Connuing Resoluon” for the 1st Q of FY12 • In the meanme PSD is developing its FY13 budget supported by acvies delineated in the Planetary decadal • This is a crical me in securing our internaonal partnerships • We are also aggressively pursuing a ghter connecon with HEOMD (formally ESMD) over areas of overlap and interest • We are also engaging the Office of Chief Technologist for help in developing key technologies (Opcal Comm, Aero‐capture…) • Historic me in planetary science is now • Discoveries are happening almost daily ‐ this is not by accident NASA’s Year of the Solar System Events 2010 • September 16 – Lunar Reconnaissance Orbiter in PSD • November 4 ‐ EPOXI encounters Comet Hartley 2 • November 19 ‐ Launch of O/OREOS • Completed •2011 hp://solarsystem.nasa.gov • February 14 ‐ Stardust NExT encounters comet Tempel 1 • March 7 – Planetary Science Decadal Survey released • March 17 ‐ MESSENGER orbit inseron at Mercury • May 5 ‐ Selecon of 3 Discovery‐class missions for study • May ‐ Selecon of the next New Froner mission for flight, OSIRIS‐Rex • July 16 ‐ Dawn orbit inseron at asteroid Vesta • August 5 ‐ Juno launched to Jupiter • August 9 ‐ Mars Opportunity Rover gets to Endeavour Crater • September 8 ‐ GRAIL launch to the Moon • November 25 ‐ Mars Science Laboratory launch to Mars • December 31 ‐ GRAIL‐A -
Atmospheric Planetary Probes And
SPECIAL ISSUE PAPER 1 Atmospheric planetary probes and balloons in the solar system A Coustenis1∗, D Atkinson2, T Balint3, P Beauchamp3, S Atreya4, J-P Lebreton5, J Lunine6, D Matson3,CErd5,KReh3, T R Spilker3, J Elliott3, J Hall3, and N Strange3 1LESIA, Observatoire de Paris-Meudon, Meudon Cedex, France 2Department Electrical & Computer Engineering, University of Idaho, Moscow, ID, USA 3Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA 4University of Michigan, Ann Arbor, MI, USA 5ESA/ESTEC, AG Noordwijk, The Netherlands 6Dipartment di Fisica, University degli Studi di Roma, Rome, Italy The manuscript was received on 28 January 2010 and was accepted after revision for publication on 5 November 2010. DOI: 10.1177/09544100JAERO802 Abstract: A primary motivation for in situ probe and balloon missions in the solar system is to progressively constrain models of its origin and evolution. Specifically, understanding the origin and evolution of multiple planetary atmospheres within our solar system would provide a basis for comparative studies that lead to a better understanding of the origin and evolution of our Q1 own solar system as well as extra-solar planetary systems. Hereafter, the authors discuss in situ exploration science drivers, mission architectures, and technologies associated with probes at Venus, the giant planets and Titan. Q2 Keywords: 1 INTRODUCTION provide significant design challenge, thus translating to high mission complexity, risk, and cost. Since the beginning of the space age in 1957, the This article focuses on the exploration of planetary United States, European countries, and the Soviet bodies with sizable atmospheres, using entry probes Union have sent dozens of spacecraft, including and aerial mobility systems, namely balloons. -
Venus Geophysical Explorer
Destination Venus: Science, Technology and Mission Architectures Overview: Purpose of Workshop James Cutts, Jet Propulsion Lab, California Institute of Technology International Planetary Probe Workshop 2016 June 11, 2016 Outline • Venus in a historical context • A Brief History of Robotic Exploration of Venus • Future Venus Mission Opportunities • International Collaboration • Venus Exploration Assessment Group (VEXAG) • Objectives of this course • Conclusions IPPW-13 Short Course-1 Venus throughout history • Brightest planet in the sky – The morning star – The evening star • Mythology and ancient astronomers – Mayan –Babylonian • Age of the telescope – Discovery of the first planetary atmosphere – Transits of sun – the distance between Earth and Sun [Hall IPPW-13 Short Course-2 International Collaboration for Venus Explorattion-3 Venus in a Historical Context and Popular Culture Lucky Starr and the Oceans of Venus, Juvenile Sci Fi Novel, 1955 The Mekon Ruler of Venus, British SF Comic Book, 1958 Queen of Outer Space, Movie, 1958 with Zsa New York Times Zsa Gabor 11/16/1928 IPPW-13 Short Course-4 A brief history of Venus Robotic Exploration • The first spacecraft to reach Venus was Mariner 2, a flyby mission in 1962. • The Soviet Union played the dominant role in Venus Exploration for the next 20 years with a series of orbiters, landers and the VeGa (Venus-Halley) mission in 1985 which also deployed two balloons at Venus. • From 1989-1994, the NASA Magellan mission produced detailed radar maps of the surface of Venus following earlier less capable US and Soviet radar missions. • In 2005, the ESA Venus Express mission was launched and for the last decade has investigated the atmosphere of Venus.