Vision and Voyages for Planetary Science in the Decade 2013-2022
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LCROSS (Lunar Crater Observation and Sensing Satellite) Observation Campaign: Strategies, Implementation, and Lessons Learned
Space Sci Rev DOI 10.1007/s11214-011-9759-y LCROSS (Lunar Crater Observation and Sensing Satellite) Observation Campaign: Strategies, Implementation, and Lessons Learned Jennifer L. Heldmann · Anthony Colaprete · Diane H. Wooden · Robert F. Ackermann · David D. Acton · Peter R. Backus · Vanessa Bailey · Jesse G. Ball · William C. Barott · Samantha K. Blair · Marc W. Buie · Shawn Callahan · Nancy J. Chanover · Young-Jun Choi · Al Conrad · Dolores M. Coulson · Kirk B. Crawford · Russell DeHart · Imke de Pater · Michael Disanti · James R. Forster · Reiko Furusho · Tetsuharu Fuse · Tom Geballe · J. Duane Gibson · David Goldstein · Stephen A. Gregory · David J. Gutierrez · Ryan T. Hamilton · Taiga Hamura · David E. Harker · Gerry R. Harp · Junichi Haruyama · Morag Hastie · Yutaka Hayano · Phillip Hinz · Peng K. Hong · Steven P. James · Toshihiko Kadono · Hideyo Kawakita · Michael S. Kelley · Daryl L. Kim · Kosuke Kurosawa · Duk-Hang Lee · Michael Long · Paul G. Lucey · Keith Marach · Anthony C. Matulonis · Richard M. McDermid · Russet McMillan · Charles Miller · Hong-Kyu Moon · Ryosuke Nakamura · Hirotomo Noda · Natsuko Okamura · Lawrence Ong · Dallan Porter · Jeffery J. Puschell · John T. Rayner · J. Jedadiah Rembold · Katherine C. Roth · Richard J. Rudy · Ray W. Russell · Eileen V. Ryan · William H. Ryan · Tomohiko Sekiguchi · Yasuhito Sekine · Mark A. Skinner · Mitsuru Sôma · Andrew W. Stephens · Alex Storrs · Robert M. Suggs · Seiji Sugita · Eon-Chang Sung · Naruhisa Takatoh · Jill C. Tarter · Scott M. Taylor · Hiroshi Terada · Chadwick J. Trujillo · Vidhya Vaitheeswaran · Faith Vilas · Brian D. Walls · Jun-ihi Watanabe · William J. Welch · Charles E. Woodward · Hong-Suh Yim · Eliot F. Young Received: 9 October 2010 / Accepted: 8 February 2011 © The Author(s) 2011. -
Current Status of the EJSM Jupiter Europa Orbiter Flagship Mission Design
Current Status of the EJSM Jupiter Europa Orbiter Flagship Mission Design Presentation to the International workshop: “Europa lander: science goals and experiments” 2/09 Presented by: Karla B. Clark EJSM–JEO Study Manager Jet Propulsion Laboratory California Institute of Technology Jupiter Europa Orbiter The NASA Element of the Europa Jupiter System Mission EJSM Baseline Mission Overview • NASA & ESA share mission leadership • Two independently launched and operated flight systems with complementary payloads – Jupiter Europa Orbiter (JEO): NASA-led mission element – Jupiter Ganymede Orbiter (JGO): ESA-led mission element • Mission Timeline – Nominal Launch: 2020 – Jovian system tour phase: 2–3 years – Moon orbital phase: 6–12 months – End of Prime Missions: 2029 • ~10–11 Instruments on each flight system, including Radio Science 2/8/08 Predecisional, For Planning Purposes Only 2 JGO Baseline Mission Overview • ESA-led portion of EJSM • Objectives: Jupiter System, Callisto, Ganymede • Launch vehicle: Arianne 5 • Power source: Solar Arrays • Mission timeline: – Launch: 2020 • Uses 6-year Venus-Earth-Earth gravity assist trajectory – Jovian system tour phase: ~28 months Wide Angle and Medium Resolution Camera • Multiple satellite flybys V/NIR Imaging Spectrometer – 9 Ganymede – 21 Callisto (19 close flybys) EUV/FUV Imaging Spectrometer – Ganymede orbital phase: 260 days Ka-band transponder – End of prime mission: 2029 Ultra Stable Oscillator – Spacecraft final disposition: Ganymede surface impact Magnetometer • Radiation: ~85 krad behind -
Fe,Mg)S, the IRON-DOMINANT ANALOGUE of NININGERITE
1687 The Canadian Mineralogist Vol. 40, pp. 1687-1692 (2002) THE NEW MINERAL SPECIES KEILITE, (Fe,Mg)S, THE IRON-DOMINANT ANALOGUE OF NININGERITE MASAAKI SHIMIZU§ Department of Earth Sciences, Faculty of Science, Toyama University, 3190 Gofuku, Toyama 930-8555, Japan § HIDETO YOSHIDA Department of Earth and Planetary Science, Graduate School of Science, University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan § JOSEPH A. MANDARINO 94 Moore Avenue, Toronto, Ontario M4T 1V3, and Earth Sciences Division, Royal Ontario Museum, 100 Queens’s Park, Toronto, Ontario M5S 2C6, Canada ABSTRACT Keilite, (Fe,Mg)S, is a new mineral species that occurs in several meteorites. The original description of niningerite by Keil & Snetsinger (1967) gave chemical analytical data for “niningerite” in six enstatite chondrites. In three of those six meteorites, namely Abee and Adhi-Kot type EH4 and Saint-Sauveur type EH5, the atomic ratio Fe:Mg has Fe > Mg. Thus this mineral actually represents the iron-dominant analogue of niningerite. By analogy with synthetic MgS and niningerite, keilite is cubic, with space group Fm3m, a 5.20 Å, V 140.6 Å3, Z = 4. Keilite and niningerite occur as grains up to several hundred m across. Because of the small grain-size, most of the usual physical properties could not be determined. Keilite is metallic and opaque; in reflected light, it is isotropic and gray. Point-count analyses of samples of the three meteorites by Keil (1968) gave the following amounts of keilite (in vol.%): Abee 11.2, Adhi-Kot 0.95 and Saint-Sauveur 3.4. -
LISA, the Gravitational Wave Observatory
The ESA Science Programme Cosmic Vision 2015 – 25 Christian Erd Planetary Exploration Studies, Advanced Studies & Technology Preparations Division 04-10-2010 1 ESAESA spacespace sciencescience timelinetimeline JWSTJWST BepiColomboBepiColombo GaiaGaia LISALISA PathfinderPathfinder Proba-2Proba-2 PlanckPlanck HerschelHerschel CoRoTCoRoT HinodeHinode AkariAkari VenusVenus ExpressExpress SuzakuSuzaku RosettaRosetta DoubleDouble StarStar MarsMars ExpressExpress INTEGRALINTEGRAL ClusterCluster XMM-NewtonXMM-Newton CassiniCassini-H-Huygensuygens SOHOSOHO ImplementationImplementation HubbleHubble OperationalOperational 19901990 19941994 19981998 20022002 20062006 20102010 20142014 20182018 20222022 XMM-Newton • X-ray observatory, launched in Dec 1999 • Fully operational (lost 3 out of 44 X-ray CCD early in mission) • No significant loss of performances expected before 2018 • Ranked #1 at last extension review in 2008 (with HST & SOHO) • 320 refereed articles per year, with 38% in the top 10% most cited • Observing time over- subscribed by factor ~8 • 2,400 registered users • Largest X-ray catalogue (263,000 sources) • Best sensitivity in 0.2-12 keV range • Long uninterrupted obs. • Follow-up of SZ clusters 04-10-2010 3 INTEGRAL • γ-ray observatory, launched in Oct 2002 • Imager + Spectrograph (E/ΔE = 500) + X- ray monitor + Optical camera • Coded mask telescope → 12' resolution • 72 hours elliptical orbit → low background • P/L ~ nominal (lost 4 out 19 SPI detectors) • No serious degradation before 2016 • ~ 90 refereed articles per year • Obs -
EDL – Lessons Learned and Recommendations
."#!(*"# 0 1(%"##" !)"#!(*"#* 0 1"!#"("#"#(-$" ."!##("""*#!#$*#( "" !#!#0 1%"#"! /!##"*!###"#" #"#!$#!##!("""-"!"##&!%%!%&# $!!# %"##"*!%#'##(#!"##"#!$$# /25-!&""$!)# %"##!""*&""#!$#$! !$# $##"##%#(# ! "#"-! *#"!,021 ""# !"$!+031 !" )!%+041 #!( !"!# #$!"+051 # #$! !%#-" $##"!#""#$#$! %"##"#!#(- IPPW Enabled International Collaborations in EDL – Lessons Learned and Recommendations: Ethiraj Venkatapathy1, Chief Technologist, Entry Systems and Technology Division, NASA ARC, 2 Ali Gülhan , Department Head, Supersonic and Hypersonic Technologies Department, DLR, Cologne, and Michelle Munk3, Principal Technologist, EDL, Space Technology Mission Directorate, NASA. 1 NASA Ames Research Center, Moffett Field, CA [email protected]. 2 Deutsches Zentrum für Luft- und Raumfahrt e.V. (DLR), German Aerospace Center, [email protected] 3 NASA Langley Research Center, Hampron, VA. [email protected] Abstract of the Proposed Talk: One of the goals of IPPW has been to bring about international collaboration. Establishing collaboration, especially in the area of EDL, can present numerous frustrating challenges. IPPW presents opportunities to present advances in various technology areas. It allows for opportunity for general discussion. Evaluating collaboration potential requires open dialogue as to the needs of the parties and what critical capabilities each party possesses. Understanding opportunities for collaboration as well as the rules and regulations that govern collaboration are essential. The authors of this proposed talk have explored and established collaboration in multiple areas of interest to IPPW community. The authors will present examples that illustrate the motivations for the partnership, our common goals, and the unique capabilities of each party. The first example involves earth entry of a large asteroid and break-up. NASA Ames is leading an effort for the agency to assess and estimate the threat posed by large asteroids under the Asteroid Threat Assessment Project (ATAP). -
Ganymede Science Questions and Future Exploration
Planetary Science Decadal Survey Community White Paper Ganymede science questions and future exploration Geoffrey C. Collins, Wheaton College, Norton, Massachusetts [email protected] Claudia J. Alexander, Jet Propulsion Laboratory Edward B. Bierhaus, Lockheed Martin Michael T. Bland, Washington University in St. Louis Veronica J. Bray, University of Arizona John F. Cooper, NASA Goddard Space Flight Center Frank Crary, Southwest Research Institute Andrew J. Dombard, University of Illinois at Chicago Olivier Grasset, University of Nantes Gary B. Hansen, University of Washington Charles A. Hibbitts, Johns Hopkins University Applied Physics Laboratory Terry A. Hurford, NASA Goddard Space Flight Center Hauke Hussmann, DLR, Berlin Krishan K. Khurana, University of California, Los Angeles Michelle R. Kirchoff, Southwest Research Institute Jean-Pierre Lebreton, European Space Agency Melissa A. McGrath, NASA Marshall Space Flight Center William B. McKinnon, Washington University in St. Louis Jeffrey M. Moore, NASA Ames Research Center Robert T. Pappalardo, Jet Propulsion Laboratory G. Wesley Patterson, Johns Hopkins University Applied Physics Laboratory Louise M. Prockter, Johns Hopkins University Applied Physics Laboratory Kurt Retherford, Southwest Research Institute James H. Roberts, Johns Hopkins University Applied Physics Laboratory Paul M. Schenk, Lunar and Planetary Institute David A. Senske, Jet Propulsion Laboratory Adam P. Showman, University of Arizona Katrin Stephan, DLR, Berlin Federico Tosi, Istituto Nazionale di Astrofisica, Rome Roland J. Wagner, DLR, Berlin Introduction Ganymede is a planet-sized (larger than Mercury) moon of Jupiter with unique characteristics, such as being the largest satellite in the solar system, the most centrally condensed solid body in the solar system, and the only solid body in the outer solar system known to posses an internally generated magnetic field. -
Highlights in Space 2010
International Astronautical Federation Committee on Space Research International Institute of Space Law 94 bis, Avenue de Suffren c/o CNES 94 bis, Avenue de Suffren UNITED NATIONS 75015 Paris, France 2 place Maurice Quentin 75015 Paris, France Tel: +33 1 45 67 42 60 Fax: +33 1 42 73 21 20 Tel. + 33 1 44 76 75 10 E-mail: : [email protected] E-mail: [email protected] Fax. + 33 1 44 76 74 37 URL: www.iislweb.com OFFICE FOR OUTER SPACE AFFAIRS URL: www.iafastro.com E-mail: [email protected] URL : http://cosparhq.cnes.fr Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law The United Nations Office for Outer Space Affairs is responsible for promoting international cooperation in the peaceful uses of outer space and assisting developing countries in using space science and technology. United Nations Office for Outer Space Affairs P. O. Box 500, 1400 Vienna, Austria Tel: (+43-1) 26060-4950 Fax: (+43-1) 26060-5830 E-mail: [email protected] URL: www.unoosa.org United Nations publication Printed in Austria USD 15 Sales No. E.11.I.3 ISBN 978-92-1-101236-1 ST/SPACE/57 *1180239* V.11-80239—January 2011—775 UNITED NATIONS OFFICE FOR OUTER SPACE AFFAIRS UNITED NATIONS OFFICE AT VIENNA Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law Progress in space science, technology and applications, international cooperation and space law UNITED NATIONS New York, 2011 UniTEd NationS PUblication Sales no. -
Beyond Einstein: from the Big Bang to Black Holes
The Space Congress® Proceedings 2004 (41st) Space Congress Proceedings Apr 27th, 8:00 AM Panel Session II - Beyond Einstein: From the big bang to black holes Don Kniffen Beyond Einstein Program Scientist, NASA Follow this and additional works at: https://commons.erau.edu/space-congress-proceedings Scholarly Commons Citation Kniffen, Don, "Panel Session II - Beyond Einstein: From the big bang to black holes" (2004). The Space Congress® Proceedings. 10. https://commons.erau.edu/space-congress-proceedings/proceedings-2004-41st/april-27/10 This Event is brought to you for free and open access by the Conferences at Scholarly Commons. It has been accepted for inclusion in The Space Congress® Proceedings by an authorized administrator of Scholarly Commons. For more information, please contact [email protected]. SEU Science ... accretion disks, Big Bang, black holes, cosmic magnetic fields, cosmic rays, dark energy, dark matter, extreme environments, gamma-ray bursts, jets, large-scale structure, microwave background, neutron stars, nucleosynthesis, relativity, supernovae, ... 10-25 cm (UHE Cosmic Rays) to 1015 cm (Gravitational wave Great Decade: CMB fluctuations (COBE, BOOMERanG, MAXIMA, MAP, . - Gamma-Ray Bursts (CGRO, HETE-2, Swift, Glast, .. .) Ubiquity of black holes (Chandra, ASCA, HST, ...) Top priority: Answer the most profound questior raised, but not answered, by Einstein. Einstein's Predictions Completing Einstein's Legacy theory fails to explain the Three startling predictions of Einstein's relativity: Einsteiff's legacy is incomplete, his underlying physics of the very phenomena his work predicted • The expansion of the Universe (from a big bang) BIG BANG • Black holes What powered the Big Bang? • Dark energy acting against the pull of gravity Observations confirm these predictions .. -
Road Map of HEAPA-Related Future Missions HEAPA 4Th Future Plan Review Committee 2020/10-2022/9 Lead: Kazuhiro Nakazawa (Nagoya-U/KMI)
20th HEAPA WS 2021/3/8-10 Road map of HEAPA-related future missions HEAPA 4th Future Plan Review Committee 2020/10-2022/9 Lead: Kazuhiro Nakazawa (Nagoya-U/KMI) JAXA Summary of the 3rd committee outcome Vision Preface Astronomical X-ray and Gamma-ray observations are directly related with understanding the how matter and energy exits within the Universe, not only celestial objects, but also the volume itself. They are also key enablers to dig into the extreme physics. In the two broadest aims of astrophysical research, understand the Universe as of now, and understand how it came to be as such, high-energy astrophysics plays an essential role. Summary of the 3rd committee outcome Vision: three big goals Understand our Universe; matter, energy and spacetime, and its origin Dark matter : LSS/clusters to see where DM are, and search for DM direct signal Missing baryon : how the baryon and metals are distributed in the Universe Origins of the large diversity in Universe and celestial objects Galaxy and SMBH co-evolution and their impact on re-ionization Metal synthesis in the Universe Relativistic high-energy phenomena in the Universe Verifying fundamental physics in extreme condition Extreme gravitation : stellar-mass BH, SMBH Extreme high-density matter EoS : Neutron star, quark star Extreme magnetism : Magnetar Diffusive shock : wide variety of yet to be known interactions therein Dark Matter (Re): search for its direct signal Summary of the 3rd committee outcome Mission Categories by JAXA class How to launch Definition and budget Strategic H-IIA, H-III Top science. Flagship mission of Large class each community. -
Hi-Resolution Map Sheet
Controlled Mosaic of Enceladus Hamah Sulci Se 400K 43.5/315 CMN, 2018 GENERAL NOTES 66° 360° West This map sheet is the 5th of a 15-quadrangle series covering the entire surface of Enceladus at a 66° nominal scale of 1: 400 000. This map series is the third version of the Enceladus atlas and 1 270° West supersedes the release from 2010 . The source of map data was the Cassini imaging experiment (Porco et al., 2004)2. Cassini-Huygens is a joint NASA/ESA/ASI mission to explore the Saturnian 350° system. The Cassini spacecraft is the first spacecraft studying the Saturnian system of rings and 280° moons from orbit; it entered Saturnian orbit on July 1st, 2004. The Cassini orbiter has 12 instruments. One of them is the Cassini Imaging Science Subsystem 340° (ISS), consisting of two framing cameras. The narrow angle camera is a reflecting telescope with 290° a focal length of 2000 mm and a field of view of 0.35 degrees. The wide angle camera is a refractor Samad with a focal length of 200 mm and a field of view of 3.5 degrees. Each camera is equipped with a 330° 300° large number of spectral filters which, taken together, span the electromagnetic spectrum from 0.2 60° 320° 310° to 1.1 micrometers. At the heart of each camera is a charged coupled device (CCD) detector 60° consisting of a 1024 square array of pixels, each 12 microns on a side. MAP SHEET DESIGNATION Peri-Banu Se Enceladus (Saturnian satellite) 400K Scale 1 : 400 000 43.5/315 Center point in degrees consisting of latitude/west longitude CMN Controlled Mosaic with Nomenclature Duban 2018 Year of publication IMAGE PROCESSING3 Julnar Ahmad - Radiometric correction of the images - Creation of a dense tie point network 50° - Multiple least-square bundle adjustments 50° - Ortho-image mosaicking Yunan CONTROL For the Cassini mission, spacecraft position and camera pointing data are available in the form of SPICE kernels. -
Arcus: the X-Ray Grating Spectrometer Explorer R
Arcus: The X-ray Grating Spectrometer Explorer R. K. Smith*a, M. Abrahamb, R. Allureda, M. Bautzc, J. Bookbinderd, J. Bregmane, L. Brennemana, N. S. Brickhousea, D. Burrowsf, V. Burwitzg, P. N. Cheimetsa, E. Costantinih, S. Dawsonc, C. DeRooa, A. Falconef, A. R. Fostera, L. Galloi, C. E. Grantc, H. M. Güntherc, R. K. Heilmannc, E. Hertza, B. Hined, D. Huenemoerderc, J. S. Kaastrah, I. Kreykenbohmj, K. K. Madsenk, R. McEntafferf, E. Millerc, J. Millere, E. Morsel, R. Mushotzkym, K. Nandrag, M. Nowakc, F. Paerelsn, R. Petreo, K. Poppenhaegerp, A. Ptako, P. Reida, J. Sandersg, M. Schattenburgc, N. Schulzc, A. Smaleo, P. Temid, L. Valencicq, S. Walkerd, R. Willingaler, J. Wilmsj, S. J. Wolka aSmithsonian Astrophysical Observatory, 60 Garden St, Cambridge, MA, US; bThe Aerospace Corp, Pasadena, CA, US, cMassachusetts Institute of Technology, Cambridge, MA, US; dNASA Ames Research Center, Moffet Field, CA US; eUniversity of Michigan, Ann Arbor, MI, US; fThe Pennsylvania State University, University Park, PA, US; gMax-Planck-Institut für extraterrestrische Physik, Garching, DE; hS- RON Netherlands Institute for Space Research, Utrecht, NL; iSaint Mary’s University, Halifax, Canada; jFrie- drich-Alexander-Universitaet, Erlangen-Nürnberg, DE; kCalifornia Institute of Technology, Pasadena, CA, US; lOrbital ATK, Dulles, VA, US; mUniversity of Maryland, College Park, MD, US; nColumbia University, New York, NY, US; oNASA Goddard Space Flight Center, Greenbelt, MD, US, pQueen’s University, Belfast, UK; qJohns Hopkins University, Baltimore, MD, US; rUniversity of Leicester, Leicester, UK 1. ABSTRACT Arcus, a Medium Explorer (MIDEX) mission, was selected by NASA for a Phase A study in August 2017. The observatory provides high-resolution soft X-ray spectroscopy in the 12-50Å bandpass with unprecedent- ed sensitivity: effective areas of >450 cm2 and spectral resolution >2500. -
M Iei1canjlusellm PUBLISHED by the AMERICAN MUSEUM of NATURAL HISTORY CENTRAL PARK WEST at 79TH STREET, NEW YORK 24, N.Y
jovitatesM iei1canJlusellm PUBLISHED BY THE AMERICAN MUSEUM OF NATURAL HISTORY CENTRAL PARK WEST AT 79TH STREET, NEW YORK 24, N.Y. NUMBER 2173 APRIL I4, I964 The Chainpur Meteorite BY KLAUS KEIL,1 BRIAN MASON,2 H. B. WIIK,3 AND KURT FREDRIKSSON4 INTRODUCTION This remarkable meteorite fell on May 9, 1907, at 1.30 P.M. as a shower of stones at and near the village of Chainpur (latitude 210 51' N., longi- tude 83° 29' E.) on the Ganges Plain. Some 8 kilograms were recovered. The circumstances of the fall and the recovery of the stones, and a brief description of the material, were given by Cotter (1912). One of us (Mason), when examining the Nininger Meteorite Collection in Arizona State University in January, 1962, noticed the unusual ap- pearance of a fragment of this meteorite, particularly the large chondrules and the friable texture, and obtained a sample for further investigation. Shortly thereafter, Keil was studying the Nininger Meteorite Collection, also remarked on this meteorite, and began independently to investigate it. In the meantime, Mason had sent a sample to Wiik for analysis. Under these circumstances, it seems desirable to report all these investi- gations in a single paper. 1 Ames Research Center, Moffett Field, California. 2 Chairman, Department of Mineralogy, the American Museum of Natural History. 3Research Associate, Department of Mineralogy, the American Museum of Natural History. 4Scripps Institution of Oceanography, La Jolla. 2 AMERICAN MUSEUM NOVITATES NO. 2173 FIG. 1. Photomicrograph of a thin section of the Chainpur meteorite, showing chondrules of olivine and pyroxene in a black matrix.