NASA Advisory Council, Planetary Sciences Subcommittee
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Mars Reconnaissance Orbiter
Chapter 6 Mars Reconnaissance Orbiter Jim Taylor, Dennis K. Lee, and Shervin Shambayati 6.1 Mission Overview The Mars Reconnaissance Orbiter (MRO) [1, 2] has a suite of instruments making observations at Mars, and it provides data-relay services for Mars landers and rovers. MRO was launched on August 12, 2005. The orbiter successfully went into orbit around Mars on March 10, 2006 and began reducing its orbit altitude and circularizing the orbit in preparation for the science mission. The orbit changing was accomplished through a process called aerobraking, in preparation for the “science mission” starting in November 2006, followed by the “relay mission” starting in November 2008. MRO participated in the Mars Science Laboratory touchdown and surface mission that began in August 2012 (Chapter 7). MRO communications has operated in three different frequency bands: 1) Most telecom in both directions has been with the Deep Space Network (DSN) at X-band (~8 GHz), and this band will continue to provide operational commanding, telemetry transmission, and radiometric tracking. 2) During cruise, the functional characteristics of a separate Ka-band (~32 GHz) downlink system were verified in preparation for an operational demonstration during orbit operations. After a Ka-band hardware anomaly in cruise, the project has elected not to initiate the originally planned operational demonstration (with yet-to-be used redundant Ka-band hardware). 201 202 Chapter 6 3) A new-generation ultra-high frequency (UHF) (~400 MHz) system was verified with the Mars Exploration Rovers in preparation for the successful relay communications with the Phoenix lander in 2008 and the later Mars Science Laboratory relay operations. -
JUICE Red Book
ESA/SRE(2014)1 September 2014 JUICE JUpiter ICy moons Explorer Exploring the emergence of habitable worlds around gas giants Definition Study Report European Space Agency 1 This page left intentionally blank 2 Mission Description Jupiter Icy Moons Explorer Key science goals The emergence of habitable worlds around gas giants Characterise Ganymede, Europa and Callisto as planetary objects and potential habitats Explore the Jupiter system as an archetype for gas giants Payload Ten instruments Laser Altimeter Radio Science Experiment Ice Penetrating Radar Visible-Infrared Hyperspectral Imaging Spectrometer Ultraviolet Imaging Spectrograph Imaging System Magnetometer Particle Package Submillimetre Wave Instrument Radio and Plasma Wave Instrument Overall mission profile 06/2022 - Launch by Ariane-5 ECA + EVEE Cruise 01/2030 - Jupiter orbit insertion Jupiter tour Transfer to Callisto (11 months) Europa phase: 2 Europa and 3 Callisto flybys (1 month) Jupiter High Latitude Phase: 9 Callisto flybys (9 months) Transfer to Ganymede (11 months) 09/2032 – Ganymede orbit insertion Ganymede tour Elliptical and high altitude circular phases (5 months) Low altitude (500 km) circular orbit (4 months) 06/2033 – End of nominal mission Spacecraft 3-axis stabilised Power: solar panels: ~900 W HGA: ~3 m, body fixed X and Ka bands Downlink ≥ 1.4 Gbit/day High Δv capability (2700 m/s) Radiation tolerance: 50 krad at equipment level Dry mass: ~1800 kg Ground TM stations ESTRAC network Key mission drivers Radiation tolerance and technology Power budget and solar arrays challenges Mass budget Responsibilities ESA: manufacturing, launch, operations of the spacecraft and data archiving PI Teams: science payload provision, operations, and data analysis 3 Foreword The JUICE (JUpiter ICy moon Explorer) mission, selected by ESA in May 2012 to be the first large mission within the Cosmic Vision Program 2015–2025, will provide the most comprehensive exploration to date of the Jovian system in all its complexity, with particular emphasis on Ganymede as a planetary body and potential habitat. -
Mars, the Nearest Habitable World – a Comprehensive Program for Future Mars Exploration
Mars, the Nearest Habitable World – A Comprehensive Program for Future Mars Exploration Report by the NASA Mars Architecture Strategy Working Group (MASWG) November 2020 Front Cover: Artist Concepts Top (Artist concepts, left to right): Early Mars1; Molecules in Space2; Astronaut and Rover on Mars1; Exo-Planet System1. Bottom: Pillinger Point, Endeavour Crater, as imaged by the Opportunity rover1. Credits: 1NASA; 2Discovery Magazine Citation: Mars Architecture Strategy Working Group (MASWG), Jakosky, B. M., et al. (2020). Mars, the Nearest Habitable World—A Comprehensive Program for Future Mars Exploration. MASWG Members • Bruce Jakosky, University of Colorado (chair) • Richard Zurek, Mars Program Office, JPL (co-chair) • Shane Byrne, University of Arizona • Wendy Calvin, University of Nevada, Reno • Shannon Curry, University of California, Berkeley • Bethany Ehlmann, California Institute of Technology • Jennifer Eigenbrode, NASA/Goddard Space Flight Center • Tori Hoehler, NASA/Ames Research Center • Briony Horgan, Purdue University • Scott Hubbard, Stanford University • Tom McCollom, University of Colorado • John Mustard, Brown University • Nathaniel Putzig, Planetary Science Institute • Michelle Rucker, NASA/JSC • Michael Wolff, Space Science Institute • Robin Wordsworth, Harvard University Ex Officio • Michael Meyer, NASA Headquarters ii Mars, the Nearest Habitable World October 2020 MASWG Table of Contents Mars, the Nearest Habitable World – A Comprehensive Program for Future Mars Exploration Table of Contents EXECUTIVE SUMMARY .......................................................................................................................... -
Why Mars Sample Return Is of Increasingly Compelling Interest to the International Mars Exploration Community
Geophysical Research Abstracts Vol. 21, EGU2019-12245, 2019 EGU General Assembly 2019 © Author(s) 2019. CC Attribution 4.0 license. Why Mars Sample Return is of Increasingly Compelling Interest to the International Mars Exploration Community David Beaty (1), Elliot Sefton-Nash (2), Sanjay Vijendran (2), Michael Meyer (3), Brandi Carrier (1), Monica Grady (4), Harry McSween (5), Charles Edwards (1), Thiag Kumaraswamy (2), and Yael Asher (2) (1) Jet Propulsion Laboratory, Mars Program Office, PASADENA, United States ([email protected]), (2) European Space Agency, European Space Research and Technology Centre, Noordwijk, Netherlands, (3) NASA Headquarters, Washington, DC, United States, (4) Open University, Milton-Keynes, United Kingdom, (5) University of Tennessee, Knoxville, United States The transport to Earth of martian samples was first proposed within NASA’s space science program in the 1970s. Since then it has progressively gained support from the international Mars exploration community. There have been developments in several areas surrounding Mars Sample Return (MSR) that have changed within the past decade or so that have caused interest to increase: 1. Martian meteorites.: Although the number of martian meteorites has now grown to over 100, it has become apparent that thelimited types of samples which survive the ejection process and the loss of sample context will continue to constrain what is possible using meteorites. 2. Mission results: Fabulous new results have been obtained by the in-situ exploration program (of particular note, MSL and the expected results to come from Exo-Mars). These results have emphasize the additional value that would come from analyzing Mars samples using the greater spatial focus, increased resolution and large diversity of instrumentation available in terrestrial laboratories. -
1 Cross-Calibration of Laser-Induced Breakdown Spectroscopy (LIBS)
ISSI/ISSI-BJ Joint Call for Proposals 2018 International Teams in Space and Earth Sciences Cross-calibration of Laser-Induced Breakdown Spectroscopy (LIBS) instruments for planetary exploration. 1 Summary of the project : A revolutionary technique for planetary science: Laser-induced Breakdown Spectroscopy (LIBS) is an active analytical technique that makes use of a pulsed laser to ablate material of interest at a distance. The atoms in the high temperature plasma emit at specific wavelengths from the UV to near- IR and the light can be analyzed by spectrometry to determine the composition of the target [1]. Since 2012, LIBS has been successfully used under low atmospheric pressure for exploring the geology of Mars at Gale Crater with the Mars Science Laboratory rover’s ChemCam instrument [2-4]. LIBS can be used to analyze single regolith mineral particles and larger rocks, giving major and minor elements compositions. Moreover, LIBS is sensitive to volatile elements (H, Na, etc.) that are of intrinsic interest to understand key planetary processes. The generated shock wave can also ablate dust covering rocks to allow further analysis by other instruments on the mission platform (rover, lander). In order to quantify the elemental composition of various targets, large laboratory samples analyses are required for calibration, with ChemCam’s calibration database containing more than 400 standards [5-6]. LIBS is becoming international: Due to its ease of deployment and rapidity of analysis, LIBS has shown a great potential as a chemistry survey instrument for the next generation of in situ space missions to planets, satellites and small bodies. In the next couple of years, three more LIBS space instruments will be sent for planetary exploration by teams representing several different nationalities In 2018, the Indian space mission to the Moon Chandrayaan 2 will comprise a rover equipped with a small portable LIBS instrument for regolith reconnaissance around the landing site [7]. -
Exploration of Mars by the European Space Agency 1
Exploration of Mars by the European Space Agency Alejandro Cardesín ESA Science Operations Mars Express, ExoMars 2016 IAC Winter School, November 20161 Credit: MEX/HRSC History of Missions to Mars Mars Exploration nowadays… 2000‐2010 2011 2013/14 2016 2018 2020 future … Mars Express MAVEN (ESA) TGO Future ESA (ESA- Studies… RUSSIA) Odyssey MRO Mars Phobos- Sample Grunt Return? (RUSSIA) MOM Schiaparelli ExoMars 2020 Phoenix (ESA-RUSSIA) Opportunity MSL Curiosity Mars Insight 2020 Spirit The data/information contained herein has been reviewed and approved for release by JPL Export Administration on the basis that this document contains no export‐controlled information. Mars Express 2003-2016 … First European Mission to orbit another Planet! First mission of the “Rosetta family” Up and running since 2003 Credit: MEX/HRSC First European Mission to orbit another Planet First European attempt to land on another Planet Original mission concept Credit: MEX/HRSC December 2003: Mars Express Lander Release and Orbit Insertion Collission trajectory Bye bye Beagle 2! Last picture Lander after release, release taken by VMC camera Insertion 19/12/2003 8:33 trajectory Credit: MEX/HRSC Beagle 2 was found in January 2015 ! Only 6km away from landing site OK Open petals indicate soft landing OK Antenna remained covered Lessons learned: comms at all time! Credit: MEX/HRSC Mars Express: so many missions at once Mars Mission Phobos Mission Relay Mission Credit: MEX/HRSC Mars Express science investigations Martian Moons: Phobos & Deimos: Ionosphere, surface, -
Estimated Attenuation Rates Using GPR and TDR in Volcanic Depos
PUBLICATIONS Journal of Geophysical Research: Planets RESEARCH ARTICLE Electromagnetic signal penetration in a planetary soil 10.1002/2016JE005192 simulant: Estimated attenuation rates using GPR Key Points: and TDR in volcanic deposits on Mount Etna • GPR methodologies for evaluating the loss tangent of volcanic sediments S. E. Lauro1 , E. Mattei1 , B. Cosciotti1 , F. Di Paolo1 , S. A. Arcone2, M. Viccaro3,4 , • Characterization of electrical 1 properties of a planetary soil simulant and E. Pettinelli • Comparison between GPR and TDR 1 2 measurements Dipartimento di Matematica e Fisica, Università degli Studi Roma TRE, Rome, Italy, US Army ERDC-CRREL, Hanover, New Hampshire, USA, 3Dipartimento di Scienze Biologiche Geologiche e Ambientali, Università degli Studi di Catania, Catania, Italy, 4Osservatorio Etneo, Istituto Nazionale di Geofisica e Vulcanologia, Catania, Italy Correspondence to: S. E. Lauro, Abstract Ground-penetrating radar (GPR) is a well-established geophysical terrestrial exploration method [email protected] and has recently become one of the most promising for planetary subsurface exploration. Several future landing vehicles like EXOMARS, 2020 NASA ROVER, and Chang’e-4, to mention a few, will host GPR. A GPR Citation: survey has been conducted on volcanic deposits on Mount Etna (Italy), considered a good analogue for Lauro, S. E., E. Mattei, B. Cosciotti, F. Di Paolo, S. A. Arcone, M. Viccaro, and Martian and Lunar volcanic terrains, to test a novel methodology for subsoil dielectric properties estimation. E. Pettinelli (2017), Electromagnetic The stratigraphy of the volcanic deposits was investigated using 500 MHz and 1 GHz antennas in two different signal penetration in a planetary soil configurations: transverse electric and transverse magnetic. -
Range Resolution Enhancement of WISDOM/Exomars
Range resolution enhancement of WISDOM/ExoMars radar soundings by the Bandwidth Extrapolation technique: Validation and application to field campaign measurements Nicolas Oudart, Valérie Ciarletti, Alice Le Gall, Marco Mastrogiuseppe, Yann Herve, Wolf-Stefan Benedix, Dirk Plettemeier, Vivien Tranier, Rafik Hassen-Khodja, Christoph Statz, et al. To cite this version: Nicolas Oudart, Valérie Ciarletti, Alice Le Gall, Marco Mastrogiuseppe, Yann Herve, et al.. Range resolution enhancement of WISDOM/ExoMars radar soundings by the Bandwidth Extrapolation tech- nique: Validation and application to field campaign measurements. Planetary and Space Science, Elsevier, 2021, 197 (March), pp.105173. 10.1016/j.pss.2021.105173. insu-03114236v2 HAL Id: insu-03114236 https://hal-insu.archives-ouvertes.fr/insu-03114236v2 Submitted on 28 Jan 2021 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Distributed under a Creative Commons Attribution| 4.0 International License Planetary and Space Science 197 (2021) 105173 Contents lists available at ScienceDirect Planetary -
March 21–25, 2016
FORTY-SEVENTH LUNAR AND PLANETARY SCIENCE CONFERENCE PROGRAM OF TECHNICAL SESSIONS MARCH 21–25, 2016 The Woodlands Waterway Marriott Hotel and Convention Center The Woodlands, Texas INSTITUTIONAL SUPPORT Universities Space Research Association Lunar and Planetary Institute National Aeronautics and Space Administration CONFERENCE CO-CHAIRS Stephen Mackwell, Lunar and Planetary Institute Eileen Stansbery, NASA Johnson Space Center PROGRAM COMMITTEE CHAIRS David Draper, NASA Johnson Space Center Walter Kiefer, Lunar and Planetary Institute PROGRAM COMMITTEE P. Doug Archer, NASA Johnson Space Center Nicolas LeCorvec, Lunar and Planetary Institute Katherine Bermingham, University of Maryland Yo Matsubara, Smithsonian Institute Janice Bishop, SETI and NASA Ames Research Center Francis McCubbin, NASA Johnson Space Center Jeremy Boyce, University of California, Los Angeles Andrew Needham, Carnegie Institution of Washington Lisa Danielson, NASA Johnson Space Center Lan-Anh Nguyen, NASA Johnson Space Center Deepak Dhingra, University of Idaho Paul Niles, NASA Johnson Space Center Stephen Elardo, Carnegie Institution of Washington Dorothy Oehler, NASA Johnson Space Center Marc Fries, NASA Johnson Space Center D. Alex Patthoff, Jet Propulsion Laboratory Cyrena Goodrich, Lunar and Planetary Institute Elizabeth Rampe, Aerodyne Industries, Jacobs JETS at John Gruener, NASA Johnson Space Center NASA Johnson Space Center Justin Hagerty, U.S. Geological Survey Carol Raymond, Jet Propulsion Laboratory Lindsay Hays, Jet Propulsion Laboratory Paul Schenk, -
SATELLITE DATA for Weather Forecasting
VOL. 98 NO. 3 MAR 2017 Mars 2020 Mission Earth Science Jobs: Seven Projections Earth & Space Science News Landsat Archive of Greenland Glaciers SATELLITE DATA for Weather Forecasting Earth & Space Science News Contents MARCH 2017 VOLUME 98, ISSUE 3 PROJECT UPDATE 20 Using LANDSAT to Take the Long View on Greenland Glaciers A new web-based data portal gives scientists access to more than 40 years of satellite imagery, providing seasonal to long-term insights into outflows from Greenland’s ice sheet. PROJECT UPDATE 32 Seeking Signs of Life and More: NASA’s Mars 2020 Mission The next Mars rover will be able to land near rugged terrain, giving scientists access to diverse landscapes. It will also cache core samples, a first step in the quest 26 to return samples to Earth. COVER OPINION Transforming Satellite Data Seven Projections 14 for Earth and Space into Weather Forecasts Science Jobs What do recent political changes mean A NASA project spans the gap between research and operations, for the job market? In the short term, not introducing new composites of satellite imagery to weather much. But long term, expect privatization, forecasters. contract employment, and more. Earth & Space Science News Eos.org // 1 Contents DEPARTMENTS Editor in Chief Barbara T. Richman: AGU, Washington, D. C., USA; eos_ [email protected] Editors Christina M. S. Cohen Wendy S. Gordon Carol A. Stein California Institute Ecologia Consulting, Department of Earth and of Technology, Pasadena, Austin, Texas, USA; Environmental Sciences, Calif., USA; wendy@ecologiaconsulting University of Illinois at cohen@srl .caltech.edu .com Chicago, Chicago, Ill., José D. -
The Supercam Remote Raman Spectrometer for Mars 2020 R.C
Lunar and Planetary Science XLVIII (2017) 2600.pdf THE SUPERCAM REMOTE RAMAN SPECTROMETER FOR MARS 2020 R.C. Wiens1, R. Newell1, S. Clegg1, S.K. Sharma2, A. Misra2, P. Bernardi3, S. Maurice4, K. McCabe1, P. Cais5, and the SuperCam Science Team (1LANL, Los Alamos, NM; [email protected], 2U. Hawaii; 3LESIA; 4IRAP; 5LAB) Overview: The Mars 2020 Science Definition length calibration as well as to have reasonable Team developed criteria for advanced instrumen- resolution; b) to identify a mineral by resolving tation for the next NASA rover. One important two of its closely-spaced peaks. Examples of this criterion is to provide mineral compositions at are olivine or albite whose twin peaks are gener- remote distances [1]. Hence, the SuperCam in- ally characteristic of their spectra; and c) to iden- strument that was selected provides two remote tify the presence of two or more minerals in the mineralogy techniques: passive visible and infra- same spectrum by resolving their respective red (VISIR) reflectance spectroscopy and remote peaks. An example is quartz and albite, which Raman spectroscopy. These are in addition to often occur together. A FWHM of 12 cm-1 vali- providing co-bore-sighted remote elemental com- dated on a naturally narrow emission line meets positions, color images, and acoustic spectra all of the above needs. There are other ways of (sounds) [2]. SuperCam’s remote Raman spec- specifying resolution, such as the pixel spread or troscopy complements the rover’s in-situ Raman the theoretical resolution of a system. For exam- experiment, SHERLOC (see below; [3]), and ple, the 12 cm-1 FWHM criterion is better than RLS on ExoMars, as the first Raman spectrome- examples labeled in [4] as “4 cm-1”, the highest ters to be built for another planet. -
Supercam Calibration Targets: Design and Development J
SuperCam Calibration Targets: Design and Development J. Manrique, G. Lopez-Reyes, A. Cousin, F. Rull, S. Maurice, R. Wiens, M. Madsen, J. Madariaga, O. Gasnault, J. Aramendia, et al. To cite this version: J. Manrique, G. Lopez-Reyes, A. Cousin, F. Rull, S. Maurice, et al.. SuperCam Calibration Tar- gets: Design and Development. Space Science Reviews, Springer Verlag, 2020, 216 (8), pp.138. 10.1007/s11214-020-00764-w. hal-03048873 HAL Id: hal-03048873 https://hal.archives-ouvertes.fr/hal-03048873 Submitted on 3 Jan 2021 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Space Sci Rev (2020) 216:138 https://doi.org/10.1007/s11214-020-00764-w SuperCam Calibration Targets: Design and Development J.A. Manrique1 · G. Lopez-Reyes1 · A. Cousin2 · F. Rull 1 · S. Maurice2 · R.C. Wiens3 · M.B. Madsen4 · J.M. Madariaga5 · O. Gasnault2 · J. Aramendia5 · G. Arana5 · P. Beck6 · S. Bernard7 · P. Bernardi 8 · M.H. Bernt4 · A. Berrocal9 · O. Beyssac7 · P. Caïs 10 · C. Castro11 · K. Castro5 · S.M. Clegg3 · E. Cloutis12 · G. Dromart13 · C. Drouet14 · B. Dubois15 · D. Escribano16 · C. Fabre17 · A. Fernandez11 · O. Forni2 · V.