"Do Not Look at Stars As Bright Spots Only. Try to Take in the Vastness Of
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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 .................................... -
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. -
Rak a Malý Lev Na Rozhraní Zimní a Jarní Oblohy Uprostřed Jarního Trojúhelníku Leží Malé Souhvězdí, Po Němž Máme Na Zemi Pojmenovaný Obratník
Pozorování © Nigel Sharp, Mark Hanna/NOAO/AURA/NSF Rak a Malý lev Na rozhraní zimní a jarní oblohy uprostřed jarního trojúhelníku leží malé souhvězdí, po němž máme na Zemi pojmenovaný obratník. Souhvězdí Raka. V minulosti totiž právě v tomto souhvězdí dosahovalo Slunce největší deklinace. Dnes, díky precesi, k tomu dochází v souhvězdí Blíženců. Rak je v antice zpodobňován jako krab pomáhající Hydře v boji proti Herkulovi. Chaldejci zde zase viděli místo, kudy sestupují duše na Zem, aby zde přijaly fyzické tělo. Ve starověkém Egyptě toto souhvězdí znali již v roce 2 000 př. n. l. Nenápadné souhvězdí Malého lva najdeme mezi Lvem a Velkou medvědicí. Toto nenápadné a ve městě v podstatě neviditelné souhvězdí se na oblohu dostalo až v novověku díky Janu Heveliovi, definitivně se Malý lev na obloze zabydlel až ve 20. století, kdy byla na Valném shromáždění IAU přijata dnešní podoba souhvězdí. M 67 Rak leží na ekliptice, proto můžeme být někdy svědky zákrytu jeho hvězd Měsícem, asi 580 ly. Skutečný rektascenze deklinace jasnost rozměry výjimečně i planetou. Nejjasnější hvězda, průměr je asi 13 ly. α Cnc, se jmenuje Acubens, což znamená Stáří se odhaduje na α Cnc 8h 58,9m 11° 50′ 4,3+11,8 11″ „klepeto“, a dosahuje 4. velikosti. Jedná se 730 mil. let. První ι Cnc 8h 47,1m 28° 44′ 4,1+6,0 30″ o dvojhvězdu. Ve vzdálenosti 11″ se nachází pozoroval M 44 již druhá složka 11. velikosti. Celý systém je Galileo Galilei a roz- M 44 8h 40m 19° 40′ 3,5 95′ od nás vzdálen asi 170 ly. -
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. -
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. -
Solar System Space Exploration Timeline Challenge Cards
SOLAR SYSTEM Timeline cards SPACE GRAB BAG H.G. Wells´ novel The War of the Worlds was published, inspiring Robert Goddard to investigate rocketry 1898 SOLAR SYSTEM Timeline cards SPACE GRAB BAG Based on Jules Verne’s novel From the Earth to the Moon, the first work that suggested space exploration was possible was published in Russia entitled “The Exploration of Cosmic Space by Means of Reaction Devices” 1903 SOLAR SYSTEM Timeline cards SPACE GRAB BAG Confirmation of the existence of the Van Allen radiation belts 1958 SOLAR SYSTEM Timeline cards SPACE GRAB BAG First detection of solar wind 1959 SOLAR SYSTEM Timeline cards SPACE GRAB BAG First photographs transmitted from the moon 1966 SOLAR SYSTEM Timeline cards SPACE GRAB BAG Closest flyby of the sun, 44 million kilometers, by the spacecraft Helios 2 1976 SOLAR SYSTEM Timeline cards SPACE GRAB BAG Hubble Space telescope launched 1990 SOLAR SYSTEM Timeline cards SPACE GRAB BAG First asteroid flyby, the asteroid 951 Gaspra by the spacecraft Galileo 1991 SOLAR SYSTEM Timeline cards SPACE GRAB BAG Launch of Ulysses, a collaboration between NASA and the European Space Agency, the first spacecraft to orbit the sun at its poles 1992 SOLAR SYSTEM Timeline cards SPACE GRAB BAG First landing on an asteroid, 433 Eros 2001 SOLAR SYSTEM Timeline cards SPACE GRAB BAG First sample returned from an asteroid by the Japanese spacecraft Hayabusa 2010 SOLAR SYSTEM Timeline cards SPACE GRAB BAG First man-made probe to make a planned and soft landing on a comet, the European Space Agency spacecraft Rosetta -
The Sudden Death of the Nearest Quasar Hannyʼs Voorwerp and Its Cousins Shed Light on Black Hole Accretion
The Sudden Death of the Nearest Quasar Hannyʼs Voorwerp and its cousins shed light on black hole accretion Dan Evans Harvard-Smithsonian Center for Astrophysics & Elon University Key collaborators: Kevin Schawinski, William Keel, Meg Urry, Shanil Virani, Chris Lintott, Priyamvada Natarajan Hanny van Arkel, Richard Proctor, Hannah Hutchins, Elizabeth Baeten, Massimo Mezzoprete, Elizabeth Siegel, Aida Berges, voyager1682002, Caro, Christian Manteuffel... 430,000+ Zooniverse Citizen Scientists Schawinski et al. 2010, ApJ Letters, 724, L30 Science Questions What is the time scale on which quasar phases turn on and off? What do rapid “deaths” tell us about black hole accretion physics? Are “dead” quasars the real culprits in quasar feedback? Discovered by citizen scientist Hanny van Arkel in 2007 Named by GZ forum members after discoverer Spectroscopic Properties z=0.05 - same as IC 2497 Lintott, Schawinski et al. (2009) Spectroscopic Properties Low Density Gas: [S II] λ6717/6731 ratio is density sensitive and lies in the low density limit (ne < 50 cm−3) AGN Photoionized: He II λ4616 and [NeV] λλ3346,3426 + [OIII] imply high ionization parameter, log U = −2.2 (need v ~ 400km/s to get lines due to shock) Low Metallicity: [N II]/Hα and [S II]/Hα indicate low metallicity of ~0.1-0.2 Zsolar Lintott, Schawinski et al. (2009) 1.4 GHz continuum 9 10 Msun of HI From: WSRT, Jozsa et al. (2010) HST F184W How luminous? • Template SED from Elvis et al. (1994) • Scaled SED to match the minimum UV luminosity to ionize the Voorwerp • Find Lbol ~ 1046 erg/s • L2-10 keV ~ 8x1044 erg/s Quasar - Lbol ~1046 erg/s! Why donʼt we see a quasar? 1. -
Extended X-Ray Emission in the IC€2497 – Hanny's Voorwerp System
MNRAS 457, 3629–3636 (2016) doi:10.1093/mnras/stw230 Advance Access publication 2016 January 29 Extended X-ray emission in the IC 2497 – Hanny’s Voorwerp system: energy injection in the gas around a fading AGN Downloaded from https://academic.oup.com/mnras/article-abstract/457/4/3629/2589023 by Pontificia Universidad Catolica de Chile user on 11 June 2019 Lia F. Sartori,1‹ Kevin Schawinski,1‹ Michael Koss,1 Ezequiel Treister,2 W. Peter Maksym,3 William C. Keel,4 C. Megan Urry,5 Chris J. Lintott6 and O. Ivy Wong7 1Institute for Astronomy, Department of Physics, ETH Zurich,¨ Wolfgang-Pauli-Strasse 27, CH-8093 Zurich,¨ Switzerland 2Departamento de Astronom´ıa, Universidad de Concepcion,´ Casilla 160-C, Concepcion,´ Chile 3Harvard–Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 4Department of Physics and Astronomy, University of Alabama, Tuscaloosa, AL 35487, USA 5Yale Center for Astronomy & Astrophysics, Physics Department, PO Box 208120, New Haven, CT 06520, USA 6Oxford Astrophysics, Denys Wilkinson Building, Keble Road, Oxford OX1 3RH, UK 7ICRAR, The University of Western Australia M468, 35 Stirling Highway, Crawley, WA 6009, Australia Accepted 2016 January 25. Received 2016 January 25; in original form 2015 November 27 ABSTRACT We present deep Chandra X-ray observations of the core of IC 2497, the galaxy associated with Hanny’s Voorwerpand hosting a fading AGN. We find extended soft X-ray emission from 42 44 −1 hot gas around the low intrinsic luminosity (unobscured) AGN (Lbol ∼ 10 –10 erg s ). The temperature structure in the hot gas suggests the presence of a bubble or cavity around the 54 55 fading AGN (Ebub ∼ 10 –10 erg). -
Joel R. Primack ! Distinguished Professor of Physics, University of California, Santa Cruz
April 18, 2014 GalaxyZoo and the Zooniverse of Astronomy Citizen Science Joel R. Primack ! Distinguished Professor of Physics, University of California, Santa Cruz Director, University of California High-Performance AstroComputing Center (UC-HiPACC) Galaxy Zoo started back in July 2007, with a data set made up of a million galaxies imaged by the Sloan Digital Sky Survey. Within 24 hours of launch we were stunned to be receiving almost 70,000 classifications an hour. More than 50 million classifications were received by the project during its first year, contributed by more than 150,000 people.! ! That meant that each galaxy was seen by many different participants. This is deliberate; having multiple independent classifications of the same object is important, as it allows us to assess how reliable our results are. For example, for projects where we may only need a few thousand galaxies but want to be sure they're all spirals before using up valuable telescope time on them, there's no problem - we can just use those that 100% of classifiers agree are spiral. For other projects, we may need to look at the properties of hundreds of thousands of galaxies, and can use those that a majority say are spiral.! ! In that first Galaxy Zoo all we asked volunteers to do was to split the galaxies into ellipticals, mergers and spirals and - if the galaxy was spiral - to record the direction of the arms. But it was enough to show that the classifications Galaxy Zoo provides were as good as those from professional astronomers, and were of use to a large number of researchers. -
We Need Your Colouring Skills!
We need your colouring skills! What do you think the colours of Mercury are? DID YOU KNOW? ercury • Mercury is the smallest planet in our solar system. • It is only slightly larger than the Earth’s Moon. • One day on Mercury is as long as 59 days on Earth. • A year on Mercury is as long as 88 Earth days • Temperatures on Mercury are extreme, reaching 430°C during the day, and -180°C at night. DID YOU KNOW? The Erth Depending on where you are on the globe, you could be spinning through space at just over 1,000 miles per hour. Water covers 70 percent of Earth's surface. 1 million Earths could fit in the Sun. Earth's atmosphere is composed of about 78 percent nitrogen, 21 percent oxygen, 0.9 percent argon, and 0.1 percent other gases. Earth is the only planet not named after a god. We need your colouring skills! What colours will you choose? We need your colouring skills! What do you think the colours of Jupiter are? DID YOU KNOW? Jupiter • Jupiter is the largest planet in the solar system. • Jupiter is as large as 1,300 Earths. • It's the 3rd brightest object in the night sky. • There's a big red spot on Jupiter, which is in fact a storm that has been raging for more than 350 years. DID YOU KNOW? Saturn • Saturn is the 2nd largest planet in the Solar System. • 764 Earths could fit inside Saturn. • Saturn's rings are made of ice and rock. They span 175,000 miles We need your and yet they’re only 20 metres thick.