EDL – Lessons Learned and Recommendations
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Lessons from Insight for Future Planetary Seismology
Open Archive Toulouse Archive Ouverte (OATAO ) OATAO is an open access repository that collects the wor of some Toulouse researchers and ma es it freely available over the web where possible. This is a publisher's version published in: https://oatao.univ-toulouse.fr/26931 Official URL : https://doi.org/10.1029/2019JE006353 To cite this version : Panning, M. P. and Pike, W. T. and Lognonné, Philippe,... [et al.]On͈Deck Seismology: Lessons from InSight for Future Planetary Seismology. (2020) Journal of Geophysical Research: Planets, 125 (4). ISSN 2169-9097 Any correspondence concerning this service should be sent to the repository administrator: [email protected] RESEARCH ARTICLE On-Deck Seismology: Lessons from InSight for Future 10.1029/2019JE006353 Planetary Seismology Special Section: 1 2 3 1 4 5 InSightatMars M. P. Panning , W. T. Pike , P. Lognonné , W. B. Banerdt , N. Murdoch , D. Banfield , C. Charalambous2 , S. Kedar1, R. D. Lorenz6 , A. G. Marusiak7 , J. B. McClean2,8 ,C. 1 9 2 10 Key Points: Nunn , S. C. Stähler ,A.E.Stott , and T. Warren • Based on InSight recordings, 1 2 atmospheric noise is amplified for Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA, Department of Electrical and seismic sensors on deck, consistent Electronic Engineering, Imperial College London, London, UK, 3Planetology and Space Science Team, Université de with Viking observations Paris, Institut de Physique du Globe, CNRS, Paris, France, 4Department of Electronics, Optronics and Signal Processing, • -
Industry at the Edge of Space Other Springer-Praxis Books of Related Interest by Erik Seedhouse
IndustryIndustry atat thethe EdgeEdge ofof SpaceSpace ERIK SEEDHOUSE S u b o r b i t a l Industry at the Edge of Space Other Springer-Praxis books of related interest by Erik Seedhouse Tourists in Space: A Practical Guide 2008 ISBN: 978-0-387-74643-2 Lunar Outpost: The Challenges of Establishing a Human Settlement on the Moon 2008 ISBN: 978-0-387-09746-6 Martian Outpost: The Challenges of Establishing a Human Settlement on Mars 2009 ISBN: 978-0-387-98190-1 The New Space Race: China vs. the United States 2009 ISBN: 978-1-4419-0879-7 Prepare for Launch: The Astronaut Training Process 2010 ISBN: 978-1-4419-1349-4 Ocean Outpost: The Future of Humans Living Underwater 2010 ISBN: 978-1-4419-6356-7 Trailblazing Medicine: Sustaining Explorers During Interplanetary Missions 2011 ISBN: 978-1-4419-7828-8 Interplanetary Outpost: The Human and Technological Challenges of Exploring the Outer Planets 2012 ISBN: 978-1-4419-9747-0 Astronauts for Hire: The Emergence of a Commercial Astronaut Corps 2012 ISBN: 978-1-4614-0519-1 Pulling G: Human Responses to High and Low Gravity 2013 ISBN: 978-1-4614-3029-2 SpaceX: Making Commercial Spacefl ight a Reality 2013 ISBN: 978-1-4614-5513-4 E r i k S e e d h o u s e Suborbital Industry at the Edge of Space Dr Erik Seedhouse, M.Med.Sc., Ph.D., FBIS Milton Ontario Canada SPRINGER-PRAXIS BOOKS IN SPACE EXPLORATION ISBN 978-3-319-03484-3 ISBN 978-3-319-03485-0 (eBook) DOI 10.1007/978-3-319-03485-0 Springer Cham Heidelberg New York Dordrecht London Library of Congress Control Number: 2013956603 © Springer International Publishing Switzerland 2014 This work is subject to copyright. -
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 .................................... -
The Pancam Instrument for the Exomars Rover
ASTROBIOLOGY ExoMars Rover Mission Volume 17, Numbers 6 and 7, 2017 Mary Ann Liebert, Inc. DOI: 10.1089/ast.2016.1548 The PanCam Instrument for the ExoMars Rover A.J. Coates,1,2 R. Jaumann,3 A.D. Griffiths,1,2 C.E. Leff,1,2 N. Schmitz,3 J.-L. Josset,4 G. Paar,5 M. Gunn,6 E. Hauber,3 C.R. Cousins,7 R.E. Cross,6 P. Grindrod,2,8 J.C. Bridges,9 M. Balme,10 S. Gupta,11 I.A. Crawford,2,8 P. Irwin,12 R. Stabbins,1,2 D. Tirsch,3 J.L. Vago,13 T. Theodorou,1,2 M. Caballo-Perucha,5 G.R. Osinski,14 and the PanCam Team Abstract The scientific objectives of the ExoMars rover are designed to answer several key questions in the search for life on Mars. In particular, the unique subsurface drill will address some of these, such as the possible existence and stability of subsurface organics. PanCam will establish the surface geological and morphological context for the mission, working in collaboration with other context instruments. Here, we describe the PanCam scientific objectives in geology, atmospheric science, and 3-D vision. We discuss the design of PanCam, which includes a stereo pair of Wide Angle Cameras (WACs), each of which has an 11-position filter wheel and a High Resolution Camera (HRC) for high-resolution investigations of rock texture at a distance. The cameras and electronics are housed in an optical bench that provides the mechanical interface to the rover mast and a planetary protection barrier. -
Mobile Lunar and Planetary Base Architectures
Space 2003 AIAA 2003-6280 23 - 25 September 2003, Long Beach, California Mobile Lunar and Planetary Bases Marc M. Cohen, Arch.D. Advanced Projects Branch, Mail Stop 244-14, NASA-Ames Research Center, Moffett Field, CA 94035-1000 TEL 650 604-0068 FAX 650 604-0673 [email protected] ABSTRACT This paper presents a review of design concepts over three decades for developing mobile lunar and planetary bases. The idea of the mobile base addresses several key challenges for extraterrestrial surface bases. These challenges include moving the landed assets a safe distance away from the landing zone; deploying and assembling the base remotely by automation and robotics; moving the base from one location of scientific or technical interest to another; and providing sufficient redundancy, reliability and safety for crew roving expeditions. The objective of the mobile base is to make the best use of the landed resources by moving them to where they will be most useful to support the crew, carry out exploration and conduct research. This review covers a range of surface mobility concepts that address the mobility issue in a variety of ways. These concepts include the Rockwell Lunar Sortie Vehicle (1971), Cintala’s Lunar Traverse caravan, 1984, First Lunar Outpost (1992), Frassanito’s Lunar Rover Base (1993), Thangavelu’s Nomad Explorer (1993), Kozlov and Shevchenko’s Mobile Lunar Base (1995), and the most recent evolution, John Mankins’ “Habot” (2000-present). The review compares the several mobile base approaches, then focuses on the Habot approach as the most germane to current and future exploration plans. -
18Th EANA Conference European Astrobiology Network Association
18th EANA Conference European Astrobiology Network Association Abstract book 24-28 September 2018 Freie Universität Berlin, Germany Sponsors: Detectability of biosignatures in martian sedimentary systems A. H. Stevens1, A. McDonald2, and C. S. Cockell1 (1) UK Centre for Astrobiology, University of Edinburgh, UK ([email protected]) (2) Bioimaging Facility, School of Engineering, University of Edinburgh, UK Presentation: Tuesday 12:45-13:00 Session: Traces of life, biosignatures, life detection Abstract: Some of the most promising potential sampling sites for astrobiology are the numerous sedimentary areas on Mars such as those explored by MSL. As sedimentary systems have a high relative likelihood to have been habitable in the past and are known on Earth to preserve biosignatures well, the remains of martian sedimentary systems are an attractive target for exploration, for example by sample return caching rovers [1]. To learn how best to look for evidence of life in these environments, we must carefully understand their context. While recent measurements have raised the upper limit for organic carbon measured in martian sediments [2], our exploration to date shows no evidence for a terrestrial-like biosphere on Mars. We used an analogue of a martian mudstone (Y-Mars[3]) to investigate how best to look for biosignatures in martian sedimentary environments. The mudstone was inoculated with a relevant microbial community and cultured over several months under martian conditions to select for the most Mars-relevant microbes. We sequenced the microbial community over a number of transfers to try and understand what types microbes might be expected to exist in these environments and assess whether they might leave behind any specific biosignatures. -
Raman Spectroscopy of Shocked Gypsum from a Meteorite Impact Crater
International Journal of Astrobiology 16 (3): 286–292 (2017) doi:10.1017/S1473550416000367 © Cambridge University Press 2016 This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited. Raman spectroscopy of shocked gypsum from a meteorite impact crater Connor Brolly, John Parnell and Stephen Bowden Department of Geology & Petroleum Geology, University of Aberdeen, Meston Building, Aberdeen, UK e-mail: c.brolly@ abdn.ac.uk Abstract: Impact craters and associated hydrothermal systems are regarded as sites within which life could originate onEarth,and onMars.The Haughtonimpactcrater,one ofthemost well preservedcratersonEarth,is abundant in Ca-sulphates. Selenite, a transparent form of gypsum, has been colonized by viable cyanobacteria. Basementrocks, which havebeenshocked,aremoreabundantinendolithicorganisms,whencomparedwithun- shocked basement. We infer that selenitic and shocked gypsum are more suitable for microbial colonization and have enhanced habitability. This is analogous to many Martian craters, such as Gale Crater, which has sulphate deposits in a central layered mound, thought to be formed by post-impact hydrothermal springs. In preparation for the 2020 ExoMars mission, experiments were conducted to determine whether Raman spectroscopy can distinguish between gypsum with different degrees of habitability. Ca-sulphates were analysed using Raman spectroscopyand resultsshow nosignificant statistical difference between gypsumthat has experienced shock by meteorite impact and gypsum, which has been dissolved and re-precipitated as an evaporitic crust. Raman spectroscopy is able to distinguish between selenite and unaltered gypsum. This showsthat Raman spectroscopy can identify more habitable forms of gypsum, and demonstrates the current capabilities of Raman spectroscopy for the interpretation of gypsum habitability. -
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. -
Reusable Rocket Upper Stage Development of a Multidisciplinary Design Optimisation Tool to Determine the Feasibility of Upper Stage Reusability L
Reusable Rocket Upper Stage Development of a Multidisciplinary Design Optimisation Tool to Determine the Feasibility of Upper Stage Reusability L. Pepermans Technische Universiteit Delft Reusable Rocket Upper Stage Development of a Multidisciplinary Design Optimisation Tool to Determine the Feasibility of Upper Stage Reusability by L. Pepermans to obtain the degree of Master of Science at the Delft University of Technology, to be defended publicly on Wednesday October 30, 2019 at 14:30 AM. Student number: 4144538 Project duration: September 1, 2018 – October 30, 2019 Thesis committee: Ir. B.T.C Zandbergen , TU Delft, supervisor Prof. E.K.A Gill, TU Delft Dr.ir. D. Dirkx, TU Delft This thesis is confidential and cannot be made public until October 30, 2019. An electronic version of this thesis is available at http://repository.tudelft.nl/. Cover image: S-IVB upper stage of Skylab 3 mission in orbit [23] Preface Before you lies my thesis to graduate from Delft University of Technology on the feasibility and cost-effectiveness of reusable upper stages. During the accompanying literature study, it was determined that the technology readiness level is sufficiently high for upper stage reusability. However, it was unsure whether a cost-effective system could be build. I have been interested in the field of Entry, Descent, and Landing ever since I joined the Capsule Team of Delft Aerospace Rocket Engineering (DARE). During my time within the team, it split up in the Structures Team and Recovery Team. In September 2016, I became Chief Recovery for the Stratos III student-built sounding rocket. During this time, I realised that there was a lack of fundamental knowledge in aerodynamic decelerators within DARE. -
Sanjay Limaye US Lead-Investigator Ludmila Zasova Russian Lead-Investigator Steering Committee K
Answer to the Call for a Medium-size mission opportunity in ESA’s Science Programme for a launch in 2022 (Cosmic Vision 2015-2025) EuropEan VEnus ExplorEr An in-situ mission to Venus Eric chassEfièrE EVE Principal Investigator IDES, Univ. Paris-Sud Orsay & CNRS Universite Paris-Sud, Orsay colin Wilson Co-Principal Investigator Dept Atm. Ocean. Planet. Phys. Oxford University, Oxford Takeshi imamura Japanese Lead-Investigator sanjay Limaye US Lead-Investigator LudmiLa Zasova Russian Lead-Investigator Steering Committee K. Aplin (UK) S. Lebonnois (France) K. Baines (USA) J. Leitner (Austria) T. Balint (USA) S. Limaye (USA) J. Blamont (France) J. Lopez-Moreno (Spain) E. Chassefière(F rance) B. Marty (France) C. Cochrane (UK) M. Moreira (France) Cs. Ferencz (Hungary) S. Pogrebenko (The Neth.) F. Ferri (Italy) A. Rodin (Russia) M. Gerasimov (Russia) J. Whiteway (Canada) T. Imamura (Japan) C. Wilson (UK) O. Korablev (Russia) L. Zasova (Russia) Sanjay Limaye Ludmilla Zasova Eric Chassefière Takeshi Imamura Colin Wilson University of IKI IDES ISAS/JAXA University of Oxford Wisconsin-Madison Laboratory of Planetary Space Science and Spectroscopy Univ. Paris-Sud Orsay & Engineering Center Space Research Institute CNRS 3-1-1, Yoshinodai, 1225 West Dayton Street Russian Academy of Sciences Universite Paris-Sud, Bat. 504. Sagamihara Dept of Physics Madison, Wisconsin, Profsoyusnaya 84/32 91405 ORSAY Cedex Kanagawa 229-8510 Parks Road 53706, USA Moscow 117997, Russia FRANCE Japan Oxford OX1 3PU Tel +1 608 262 9541 Tel +7-495-333-3466 Tel 33 1 69 15 67 48 Tel +81-42-759-8179 Tel 44 (0)1-865-272-086 Fax +1 608 235 4302 Fax +7-495-333-4455 Fax 33 1 69 15 49 11 Fax +81-42-759-8575 Fax 44 (0)1-865-272-923 [email protected] [email protected] [email protected] [email protected] [email protected] European Venus Explorer – Cosmic Vision 2015 – 2025 List of EVE Co-Investigators NAME AFFILIATION NAME AFFILIATION NAME AFFILIATION AUSTRIA Migliorini, A. -
Celebrate Apollo
National Aeronautics and Space Administration Celebrate Apollo Exploring The Moon, Discovering Earth “…We go into space because whatever mankind must undertake, free men must fully share. … I believe that this nation should commit itself to achieving the goal before this decade is out, of landing a man on the moon and returning him safely to Earth. No single space project in this period will be more exciting, or more impressive to mankind, or more important for the long-range exploration of space; and none will be so difficult or expensive to accomplish …” President John F. Kennedy May 25, 1961 Celebrate Apollo Exploring The Moon, Discovering Earth Less than five months into his new administration, on May 25, 1961, President John F. Kennedy, announced the dramatic and ambitious goal of sending an American safely to the moon before the end of the decade. Coming just three weeks after Mercury astronaut Alan Shepard became the first American in space, Kennedy’s bold challenge that historic spring day set the nation on a journey unparalleled in human history. Just eight years later, on July 20, 1969, Apollo 11 commander Neil Armstrong stepped out of the lunar module, taking “one small step” in the Sea of Tranquility, thus achieving “one giant leap for mankind,” and demonstrating to the world that the collective will of the nation was strong enough to overcome any obstacle. It was an achievement that would be repeated five other times between 1969 and 1972. By the time the Apollo 17 mission ended, 12 astronauts had explored the surface of the moon, and the collective contributions of hundreds of thousands of engineers, scientists, astronauts and employees of NASA served to inspire our nation and the world. -
A I -Fligat INVESTIGATIUN N83-13110 of PILOT-INDUCED
1983004840 (H&SA-CS-163116) A_ I_-FLIGaT INVESTIGATIUN N83-13110 OF PILOT-INDUCED OSCILLATION SUPPRESSIO_ FILTERS _JflING TtI_ FIGHTER APP_O&CH AND LANDING TASK (Calspan Corp., B_ffalo, N.Y.) Haclas 147 p HC AO7/MF AO| CSCL 01C G3/08 01450 NASA Contractor Report 16x_16 AN IN"FUQHT INVEST'RATION OF PILOT-INDUCED OSCILLATION SUPPRESSION FILTERS DURING THE FIGHTER AI_;_OACH AND LANDING TASK J R. E. Bailey and R. E. Smith CNarchontract 1982F336! 5-79-C--3618 . _Si_;_ _ -] i t ° t" ' Nal_c,na I Ae'onaut,c_ and Sl:)aceAdm,n,strabor" t j ', 1983004840-002 ._ASA Contractor Report 163116 • AN EqI-FLI_'IT INVESTIGATION OF PlLOT,-EIXJICi[D 08¢LL,ATION SUPPImESINONFILI'I[I_ _ THE FIGHTER _ACH AND LANDING TASK R. E. Bailey and R. E. Smith Calspan Advanced Technology Center Buffalo, New York Prepared for Ames Research Center Hugh L. Dryden Research Facility under Contract F33615-79-C-3618 • Nal_ona I Aeronaulics and Spa( e Administration Scientific a_IdTechnical Information Office 1982 1983004840-003 FOREWORD This report was prepared for the National Aeronautics and Space Administration by Calspan Corporation, Buffalo, New York, in partial fulfill- ment of USA/=Contract No. F35615-79-C-3618• This report describes an in-flight investigati , of the effects of pilot-induced oscillation filters on the long- " itudinal flying qualities of fighter aircraft during the landing task• The in-flight program reported herein was performed by the Flight • Research Department of Calspan under sponsorship of the NASA/Dryden Flight Research Center, Edwards, California, working through a Calspan contract with the Flight Dynamics Laboratory of the Air Force Wright Aeronautical Labora- tory, Wright-Patterson Air Force Base, Ohio.