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Browse and search white papers and mission & technology studies received by the Planetary Science Decadal Survey. Click here for basic user instructions.
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Jonathan I. Lunine
Co-Authors: A. Coustenis, P. Beauchamp, K. Reh, G. Bampasitis, L. Bruzzone, M.T. Capria, Coates, A., A.J. Friedson, D. Gautier, R. Jaumann, K.K. Klaus, J-P. Lebreton, T. Livengood, R. Lopes-Gautier, E. Lellouch, R. Lorenz, F-J. Martin-Torres, X. Moussas, C. Nixon, J. Nott, S. Rafkin, F. RaulinLISA Univ. Paris, S. Rodriguez, F. Sohl, A. Solomonidou, E.C. Sitler, J. Soderblom, R. West, M. Wright |
The Science of Titan and its Future Exploration |
This paper describes the science rationale for the next steps beyond Cassini-Huygens of exploration of Saturn''s moon Titan. |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
University of Arizona |
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E. Robert Kursinski
Co-Authors: James Lyons, Claire Newman, Mark Richardson |
A Dual Satellite Mission Concept for Martian Climate and Chemistry |
mm-wavelength satellite to satellite occultations combined with solar occultation and thermal IR emission aerosol measurements will tightly and uniquely constrain processes to answer key open questions about the chemistry and climate of Mars. |
Mars: Not Phobos and Deimos. |
University of Arizona |
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Roger Yelle
Co-Authors: S. Horst, M. Allen, R. Amils, S. K. Atreya G. Bampasidis, A. Bar-Nun, P. Beauchamp, M. Cabane, M. Capria, R. Carlson, N. Carrasco, A. Coates, J. Cooper,
M. Combes, T. Cours, H. Cottin, A. Coustenis, T. Cravens, J. Cui, R. de Kok, I. dePater, M. Dobrijevic, G. Durry, Y. Dutil, O. Dutuit, M. Fulchignoni, M. Galand,
Y. Gao, D. Gautier, M. Gurwell, E. Hebrard, F. Hersant, H. Imanaka; W. Ip, R. Jaumann, A. Jolly, S. Karoly, E. Kostiuk, L.-M. Lara, P. Lavvas, S. Lebonnois, J.-
P. Lebreton, M. Leese, S. Le Mou_elic, T. Livengood, R. Lopes, J. Lopez-Moreno, J. Lunine, P. Mahaffy, V. Mangano, T. McCord, R. Modolo, A. Morse, O. Mousis, I. Muller-Wodarg, A. Mura, G. Murthy C. Nixon, D. Nna-Mvondo, L. Norman, G. Ortega, G. Orton, M. Patel, A. Pavlov, C. Plainaki, P. Rannou K. Reh, M. Rengel, F. Robb, S. Rodriguez, R. Rodrigo, E. Schaller, B. Schmitt, D. Schulze-Makuch, E. Sciamma O''Brien, J. Soderblom, A. Somogyi, E. Sittler, D. Strobel, L. Spilker, T. Spilker, M. Smith, A. Steele, K. Stephan, N. Strange, C. Szopa, R. Thissen, F. Tosi, D. Toublanc, M. Trainer S. Tripathi, S. Ulamec, S. Vinatier, V. Vuitton, J.-E. Wahlund, J. H. Waite, M. Yamauchi, J. Zarnecki
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Prebiotic Atmospheric Chemistry on Titan |
Cassini measurements reveal that organic molecules with molecular weights of hundreds of amu are formed by photochemistry in Titan''s upper atmosphere. Investigating this chemistry is important for understanding the production of biological building blocks by naturally occurring processes. |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
University of Arizona |
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Jasper Halekas
Co-Authors: M. Fuller, I. Garrick-Bethell, L. L. Hood, C. L. Johnson, K.
Lawrence, R. J. Lillis, R. P. Lin, M. Manga, M. E. Purucker, B. P. Weiss
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Determining the origins of lunar remanent crustal magnetism |
The discovery of lunar magnetic fields of crustal origin was a major scientific surprise of the Apollo program. Solving the enigma of lunar remanent crustal magnetization will provide fundamental insights into the thermal history of the lunar core/dynamo, mantle, and crust, and into the processes by which crustal magnetization is acquired on airless bodies - for instance, large basin-forming impacts. Determining the origin and history of lunar crustal magnetism will require the return of oriented samples... |
Inner Planets: Mercury, Venus, and the Moon. |
University of California Berkeley |
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Robert J. Lillis
Co-Authors: J. Arkani-Hamed, D. A. Brain, J. C. Cain, J. E. P. Connerney, G. T. Delory, J. Espley, M. Fuller, J. Gattecceca, J. S. Halekas, L. L. Hood, C. L. Johnson, D. Jurdy, G. Kletetschka, B. Langlais, R. P. Lin, K. L. Louzada, M. Manga, C. Milbury, D. Mozzoni, M. Purucker, D. Ravat, J. H. Roberts, P. Rochette, C.T. Russell, S. Smrekar, S. T. Stewart, S. Vennerstrom, B. P. Weiss, K. Whaler |
Mars'' Ancient Dynamo and Crustal Remanent Magnetism |
Mars'' crustal magnetization is unique and enigmatic. It is pertinent to Mars science questions as diverse as the structure of the interior and the evolution of climate. To study it, we recommend 1) extending the MAVEN mission, 2) rover-mounted surface magnetometers and 3) oriented sample return. |
Mars: Not Phobos and Deimos. |
University of California Berkeley |
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Michael H. Wong
Co-Authors: Máté Ádámkovics, Sushil K. Atreya, Don Banfield, Jim Bell, Susan Benecchi, Gordon Bjoraker, John R. Casani, John T. Clarke, Imke de Pater, Scott G. Edgington, Leigh N. Fletcher, Richard G. French, William Grundy, Amanda R. Hendrix, Erich Karkoschka, Jian-Yang Li, Franck Marchis, Melissa A. McGrath, William J. Merline, Julianne I. Moses, Keith Noll, Glenn S. Orton, Kathy A. Rages, Kurt Retherford, Kunio Sayanagi, Nick Schneider, Eric H. Smith, Lawrence A. Sromovsky, Nathan J. Strange, Anne Verbiscer, Padmavati A. Yanamandra-Fisher
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A dedicated space observatory for time-domain solar system science |
The specific requirements for time-domain solar system science are adequate sampling rates and campaign durations. The observatory must be spaceborne both to satisfy the time-domain requirements as well as to maintain access to the dynamically significant ultraviolet spectral range. |
Inner Planets: Mercury, Venus, and the Moon.
Mars: Not Phobos and Deimos.
Giant Planets: Jupiter, Saturn, Uranus, Neptune, and exoplanets, including rings and magnetic fields, but not their satellites.
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets.
Primitive Bodies: Asteroids, comets, Phobos, Deimos, Pluto/Charon and other Kuiper belt objects, meteorites, and interplanetary dust. |
University of California Berkeley /
STScI |
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Walter Harris
Co-Authors: Walter Harris, Eric Burgh, John Clarke, Joshua Colwell, Michael Davis, Daniel Durda, Charles Hibbitts, Stephan McCandliss, Jeffrey Morgenthaler, Kurt Retherford, Ronald Vervack |
Solar System Suborbital Research: A Vital Investment in the Scientific Techniques, Technology, and Investigators of Space Exploration in the 21st Century. |
Recent calls for increased NASA technology and training development cite shortages with current trends. Suborbital and Explorer missions are key this but have been cut in the past 20 years. Planetary research supports no small missions at all. We describe how suborbital research can address this gap |
None of the above. |
University of California, Davis |
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Janet A. Vertesi
Co-Authors: Robert Pappalardo, Claudia Alexander, William J. Clancey, Barbara Cohen, Paul Dourish, Jeffrey Johnson, Barbara Larsen, Kimberly Lichtenberg, Charlotte Linde, Scott Maxwell, Zara Mirmalek, Jeff Moore |
Sociological Considerations for the Success of Planetary Exploration Missions |
Alongside scientific and technical considerations, the Planetary Science Decadal Survey should require that missions incorporate deeper consideration of the social science of spacecraft operations to maximize their missions’ scientific, technical and fiscal success. |
None of the above. |
University of California, Irvine |
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Jonathan J. Fortney
Co-Authors: Kevin Zahnle, Isabelle Baraffe, Adam Burrows, Sarah E. Dodson-Robinson, Gilles Chabrier, Tristan Guillot, Ravit Helled, Franck Hersant, William B. Hubbard, Jack J. Lissauer, Mark S. Marley |
Planetary Formation and Evolution Revealed with a Saturn Entry Probe: The Importance of Noble Gases |
The determination of Saturn’s atmospheric noble gas abundances are critical to understanding the formation and evolution of Saturn, and giant planets in general. These measurements can only be performed with an entry probe. |
Giant Planets: Jupiter, Saturn, Uranus, Neptune, and exoplanets, including rings and magnetic fields, but not their satellites. |
University of California, Santa Cruz |
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Yan Fernandez
Co-Authors: P. A. Abell, E. Ammannito, M. Aung, J. M. Bauer, J. Bellerose, H. Campins, J. Castillo-Rogez, A. F. Cheng, C. M. Dalle Ore, M. C. de Sanctis, J. P. Emery, T. Grav, W. M. Grundy, N. Haghighipour, M. J. Kuchner, J.-Y. Li, K. J. Meech, B. E. A. Mueller, K. S. Noll, C. B. Olkin, W. M. Owen, N. Pinilla-Alonso, D. Ragozzine, J. E. Riedel, E. L. Schaller, D. J. Scheeres, S. S. Sheppard, J. A. Stansberry, M. V. Sykes, J. M. Trigo-Rodríguez, D. E. Trilling, A. J. Verbiscer, H. A. Weaver, H. Yano, E. Young |
Small Bodies Community White Paper: Goals and Priorities for the Study of Centaurs and Trans-Neptunian Objects in the Next Decade |
This paper identifies the top-level science issues, mission priorities, research and technology needs, and programmatic balance for the exploration of Centaurs and Small Irregular TNOs. This paper was organized by the Small Bodies Assessment Group. |
Primitive Bodies: Asteroids, comets, Phobos, Deimos, Pluto/Charon and other Kuiper belt objects, meteorites, and interplanetary dust. |
University of Central Florida |
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Dan Britt
Co-Authors: Paul Abell, Eleonora Ammannito, Erik Asphaug, MiMi Aung, Jim Bell, Julie Bellerose, Mehdi Benna, Lance Benner, David Blewett, William Bottke, Frank Brenker, Humberto Campins, Julie Castillo-Rogez, Andrew Cheng, Clark Chapman, Harold C. Connolly Jr., Maria Cristina De Sanctis, Richard Dissley, Dan Durda, Joshua Emery, Eugene Fahnestock, Yanga Fernandez, Michael J. Gaffey, Nader Haghighipour, Mark Hammergren, Paul Hardersen, Mihaly Horanyi, Ellen Howell, Robert Jedicke, Andrew Klesh, Steve Kortenkamp, Marc Kuchner, Stephen Larson, Dante Lauretta, Larry Lebofsky, Jian-Yang Li, Amy Lovell, Franck Marchis, Joseph Masiero, Lucy McFadden, Karen Meech, William Merline, Patrick Michel, Beatrice Mueller, David Nesvorny, Michael Nolan, Joseph Nuth, David O''Brien, William Owen, Vishnu Reddy, Joseph Riedel, Andrew Rivkin, Chris Russell, Daniel Scheeres, Michael Shepard, Mark V. Sykes, Paolo Tanga, Josep M. Trigo-Rodriguez, David Trilling, Ronald Vervack, Faith Vilas, James Walker, Benjamin Weiss, Hajime Yano, Eliot Young, Michael Zolensky
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Small Bodies Community White Paper: Asteroids |
This paper identifies the top-level science issues, mission priorities, research and technology needs, and programmatic balance for the exploration of Asteroids. This paper was organized by the Small Bodies Assessment Group. |
Primitive Bodies: Asteroids, comets, Phobos, Deimos, Pluto/Charon and other Kuiper belt objects, meteorites, and interplanetary dust. |
University of Central Florida |
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Andrew M. Davis
Co-Authors: Meenakshi Wadhwa, Christine Floss, Bradley L. Jolliff, Scott Messenger, Dimitri A. Papanastassiou, Allan Treiman, Andrew J. Westphal |
Development of Capabilities and Instrumentation for Curation and Analysis of Returned Samples |
The purpose of this white paper is to emphasize the importance of investments in sample curation and analytical instrument development for the full realization of the science objectives of any sample return missions in the coming decade. |
Inner Planets: Mercury, Venus, and the Moon.
Mars: Not Phobos and Deimos.
Primitive Bodies: Asteroids, comets, Phobos, Deimos, Pluto/Charon and other Kuiper belt objects, meteorites, and interplanetary dust. |
University of Chicago |
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Jack Burns
Co-Authors: E. Hallman, D. Duncan, J. Darling, & J. Stocke, J. Lazio, K. Weiler, J. Hewitt, C. Carilli, R. Bradley, T. Bastian, J. Ulvestad, J. Kasper & L. Greenhill, R. MacDowall, S. Merkowitz, J. McGarry, Zagwodzki, P. Yeh, H. Thronson, S. Ne, D. Currie, T. Murphy, S. Furlanetto & A. Mesinger, A. Loeb, J. Pritchard & E. Visbal, D. Jones, G. Taylor, K. Nordtvedt, J. Bowman, J. Grunsfeld, S. Bale, B. Wandelt, H. Falcke
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Science from the Moon: The NASA/NLSI Lunar University Network for Astrophysics Research (LUNAR) |
The Moon is a unique platform for fundamental astrophysical measurements of gravitation, the Sun, and the Universe. With the aim of providing additional perspective on the Moon as a scientific platform, this white paper describes key research projects involving astrophysics from the Moon. |
Inner Planets: Mercury, Venus, and the Moon. |
University of Colorado |
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Bruce Jakosky
Co-Authors: Richard W. Zurek, Jan Amend, Michael H. Carr, Daniel J. McCleese, John F. Mustard, Kenneth Nealson, Roger Summons |
Update: Are There Signs of Life on Mars? A Scientific Rationale for a Mars Sample-Return Campaign As The Next Step in Solar System Exploration |
Update: Discussion of the scientific rationale for Mars sample return as the next step in understanding solar-system exploration and Mars astrobiology. Sample return is discussed in the context of a Mars exploration program and the fiscal reality of the Mars program. |
Mars: Not Phobos and Deimos. |
University of Colorado |
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Ashley Espy
Co-Authors: Amara Graps, Nicolas Altobelli, Jürgen Blum, Don Brownlee, Humberto Campins, Sigrid Close, William Cooke, Stanley Dermott, Gerhard Drolshagen, Eberhard Grün, Doug Hamilton, Matthew Hedman, Mihaly Horányi, Peter Jenniskens, Thomas Kehoe, Steve Kortenkamp, Harald Krüger, Marc Kuchner, J.-C. Liou, Carey Lisse, Greg Madsen, Ingrid Mann, Brian May, Scott Messenger, Nicole Meyer-Vernet, David Nesvorny, Pasquale Palumbo, William Reach, Chris Russell, Ralf Srama, Mark Sykes, Josep Trigo-Rodríguez, Jeremie Vaubaillon, Harold Weaver, Hajime Yano, Michael Zolensky
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Small Bodies Community White Paper: Interplanetary Dust |
This paper identifies the top-level science issues, mission priorities, research and technology needs, and programmatic balance for the exploration of Interplanetary Dust. This paper was organized by the Small Bodies Assessment Group. |
Primitive Bodies: Asteroids, comets, Phobos, Deimos, Pluto/Charon and other Kuiper belt objects, meteorites, and interplanetary dust. |
University of Florida,
Southwest Research Institute |
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Alan Tokunaga
Co-Authors: S.J. Bus, J.T. Rayner, E.V. Tollestrup |
The NASA Infrared Telescope Facility |
This white paper describes the NASA Infrared Telescope Facility, its capabilities, and its role in current and future research in planetary astronomy. |
None of the above. |
University of Hawaii |
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David H. Atkinson
Co-Authors: Thomas R. Spilker, Linda Spilker, Tony Colaprete, Tibor Balint, Robert Frampton, Sushil Atreya, Athena Coustenis, Jeff Cuzzi, Kim Reh, Ethiraj Venkatapathy, Y. Alibert, N. K. Alonge, S. Asmar, G. Bampasidis, K.H. Baines, D. Banfield, J. Barnes, R. Beebe , B. Bezard, G. Bjoraker, B. Buffington, E. Chester, A. Christou, P. DeSai, M.W. Evans, L.N. Fletcher, J. Fortney, R. Gladstone, T. Guillot, M. Hedman, G. Herdrich, M. Hofstadter, A. Howard, R. Hueso, H. Hwang, A. Ingersoll, B. Kazeminejad, J.-P. Lebreton, M. Leese, R. Lorenz, P. Mahaffy, E. Martinez, B. Marty, J. Moses, O. Mousis, G. Orton, M. Patel, S. Pogrebenko, P. Read, S. Rodriguez, H. Salo, J. Schmidt, A. Sole, P. Steffes, P. Withers |
Entry Probe Missions to the Giant Planets |
It is recommended that probe missions to the giant planets be performed to help constrain models of solar system formation and the origin and evolution of atmospheres, to provide a basis for comparative studies of the gas and ice giants, and to provide a valuable link to extrasolar planetary systems |
Giant Planets: Jupiter, Saturn, Uranus, Neptune, and exoplanets, including rings and magnetic fields, but not their satellites. |
University of Idaho |
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Conor A. Nixon
Co-Authors: Carrie M. Anderson, F. Michael Flasar, Christophe Sotin, J. Hunter Waite Jr., V. Malathy Devi, Olivier Mousis, Kim R. Reh, Konstantinos Kalogerakis, A. James Friedson, Henry Roe, Yuk L. Yung, Valeria Cottini, Giorgos Bampasidis, Richard K. Achterberg, Nicholas A. Teanby, Gordon L. Bjoraker, Eric H. Wilson, Tilak Hewagama, Mark A. Gurwell, Roger Yelle, Mark A. Allen, Nathan J. Strange, Linda J. Spilker, Glenn Orton, Candice J. Hansen, Jason W. Barnes, Jason M. Soderblom, Vladimir B. Zivkovic, Anezina Solomonidou, David L. Huestis, Mark A. Smith, David H. Atkinson, Patrick G. J. Irwin, Mathieu Hirtzig, Simon B. Calcutt, Timothy A. Livengood, Sandrine Vinatier, Theodor Kostiuk, Antoine Jolly, Nasser Moazzen-Ahmadi, Darrell F. Strobel, Mao-Chang Liang, Patricia M. Beauchamp, Remco de Kok, Robert Pappalardo, Imke de Pater, Véronique Vuitton, Paul N. Romani, Robert A. West, Lucy H. Norman, Mary Ann H. Smith, Kathleen Mandt, Sebastien Rodriguez, Máté Ádámkovics, Jean-Marie Flaud, Kurt K. Klaus, Michael Wong, Jean-Pierre Lebreton, Neil Bowles |
Titan''s Greenhouse Effect and Climate |
Herein we examine the atmospheric parallels between the Earth and Titan including the possibility of dramatic climate change. In the next decade, we urge extending the duration of the Cassini mission, planning for a future mission focused on Titan’s climate and other measures. |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
University of Maryland |
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Erin Lee Ryan
Co-Authors: Sarah M. Hörst, Michael P.J. Benfield, Fred Calef III, Dario Cersosimo, Valeria Cottini, Robert Citron, Katherine E. Gibson, Joel A. Hesch, Dana Ionita, Craig C. Jolley, Driss Takir, Matthew Turner, Elizabeth A. Jensen
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The TRACER mission: a proposed Trojan and Centaur flyby mission |
This paper presents a proposed flyby mission for one Trojan and one Centaur as designed by the participants of the JPL Planetary Science Summer School. This mission meets the current New Horizons guidelines and will address fundamental questions about the history of the solar system. |
Primitive Bodies: Asteroids, comets, Phobos, Deimos, Pluto/Charon and other Kuiper belt objects, meteorites, and interplanetary dust. |
University of Minnesota |
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Clive R. Neal
Co-Authors: Charles K. Shearer, Meenakshi Wadwha, Lars Borg,
Bradley Jolliff, Allan Treiman
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Developing Sample Return Technology using the Earth''s Moon as a Testing Ground |
Lowering cost and risk through development of sample return technologies that can be used on various sample return mission styles is emphasized, as is using the Moon as a testing ground for such technologies. |
Inner Planets: Mercury, Venus, and the Moon.
Mars: Not Phobos and Deimos.
Primitive Bodies: Asteroids, comets, Phobos, Deimos, Pluto/Charon and other Kuiper belt objects, meteorites, and interplanetary dust. |
University of Notre Dame |
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These documents have been prepared in coordination with the National Academies of Science in support of the National Academies Planetary Science Decadal Survey. These documents are being made available for information purposes only, and any views and opinions expressed herein do not necessarily state or reflect those of NASA, JPL, or the California Institute of Technology.
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