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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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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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Terry Hurford
Co-Authors: B. Buratti, A. Coustenis, A. Dombard, R. Greenberg, H. Hussmann, M. Kirchoff, C. Porco, A. Rymer |
The Case for an Enceladus New Frontiers Mission |
In this white paper, we will summarize one possible mission concept to explore Enceladus within a New Frontiers-level mission: to stay below the cost cap of $650M (FY09 dollars) and within the launch capability of the Atlas V 551. We imagine that there are other possible mission scenarios... |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
NASA Goddard Space Flight Center |
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Terry Hurford
Co-Authors: B. Buratti, A. Coustenis, A. Dombard, R. Greenberg, H. Hussmann, M. Kirchoff, C. Porco, A. Rymer, S. Vance, A. Verbiscer |
The Case for Enceladus Science |
In this white paper, we will outline important science questions regarding Enceladus and show the link between these science questions and major themes of exploration as identified by NASA. |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
NASA Goddard Space Flight Center |
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| David E. Smith |
A budget phasing approach to Europa Jupiter System Mission Science |
Due to budget constraints, the proposed Europa Jupiter System Mission is unlikely to occur as planned. We propose to split EJSM into three small, more affordable and less risky missions that return science earlier (about the same time as the launch date of ELSM) and in easier to accomodate budgets. |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
NASA Goddard Space Flight Cener |
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| Julian Nott |
Titan’s unique attraction: it is an ideal destination for humans |
With so many opportunities in the Solar System it may be hard to choose destinations. Titan has a one quality that sets it apart: it is uniquely suitable for humans. One reason for robotic Mars exploration is that humans will arrive in due course. An identical justification applies to exploring Titan |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
Nott Technology LLC |
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Julian Nott
Co-Authors: Kim Reh, Jonathan Lunine, David L. Pierce, Patricia Beauchamp, Tim Colonius, R.C. Downs, Jerrold Marsden, Carl F. Braun, Don Day, Michael Arnold, Wade Allmon, Dick Bohannnon, Alberto Elfes, John Elliot, Debora Fairbrother, Jack Jones, Jeff Hall, Greg Mungas, Michael Pauken, Rob Sinclair, Luke Brooke, David Wakefield
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Advanced Titan Balloon Design Concepts |
Numerous studies agree that Titan is of outstanding scientific interest and Montgolfiere balloons ideal for its exploration. This paper examines balloon operations, weather and steering. It suggests novel concepts that may encourage radical thinking about Titan balloon designs. |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
Nott Technology LLC |
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Athena Coustenis
Co-Authors: J. Lunine, D. Matson, K. Reh, P. Beauchamp, J.-M.Charbonnier, L. Bruzzone, M.-T. Capria, A. Coates, C. Hansen, R. Jaumann, J.-P. Lebreton, R. Lopes, R. Lorenz, I. Mueller-Wodarg, F. Raulin, E. Sittler, J. Soderblom, F. Sohl, C. Sotin, T. Spilker, N. Strange, T. Tokano, E. Turtle, H. Waite, L. Gurvits, C. Nixon, T. Livengood, J. Blamont, R. Achterberg, M. Allen, C. Anderson, D. Atkinson, T. Balint, G. Bampasidis, D. Banfield, A. Bar-Nun, J. Barnes, R. Beebe, E. Bierhaus, G. Bjoraker, D. Burr, F. Crary, J. Cui, J. Elliott, M. Flasar, A. Friedson, M. Galand, D. Gautier, M. Gurwell, J. Head, M. Hirtzig, T. Hurford, T. Johnson, K. Klaus, W. Kurth, E. Lellouch, J. Martin-Torres, K. Mitchell, X. Moussas, M. Munk, C. Neish, L. Norman, B. Noyelles, G. Orton, A. Pankine, D. Pascu , E. Pencil, S. Rafkin, T. Ray, F. Rocard, S. Rodriguez, A. Solomonidou, L. Spilker, R. West, D. Williams, E. Wilson, M. Wright, V. Zivkovic |
Future in situ balloon exploration of Titan’s atmosphere and surface |
Many of the questions remaining to be addressed after the Cassini-Huygens mission require both remote and in situ exploration. Our understanding of the lower atmosphere, surface and interior of Titan will benefit greatly from detailed investigations by a montgolfiere, reaching a variety of locations |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
Paris Observatory, France |
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Cynthia Phillips
Co-Authors: D. L. Blaney, R. T. Pappalardo, H. Hussman, G. C. Collins, R. M. Mastrapa, J. F. Cooper, R. Greeley, J. B. Dalton, T. A. Hurford, E. B. Bierhaus, F. Nimmo, D. A. Williams, D. A. Senske , D. Grinspoon, R. E. Johnson, S. Kattenhorn, P. Hayne, B. Betts, W. B. McKinnon, L. M. Prockter, A. P. Showman, J. H. Shirley, K. Khurana, S. Grasby, B. G. Bills, L. Friedman, J. Castillo, C. Sotin, G. Hansen, K. Klaus, B. J. Buratti, S. W. Asmar, M. J. S. Belton, E. Heggy, L. Sklar, A. R. Hendrix, J. R. Spear, S. Ulamec, L. Bruzzone, F. Tosi, R. Jaumann, G. Strazzulla, A. Coates, J. Emery, L. Allamandola, A. Coustenis, R. W. Carlson, W. Grundy, S. D. Vance, G. Branduardi-Raymont, M. Barmatz, P. M. Beauchamp, A. D. Anbar, C. A. Raymond, K. P. Hand, E. Shock, K. Stephan, D. L. Goldsby, D. D. Blankenship, M. Choukroun, W. Moore, E. P. Turtle, T. Pierson, S. Neuer, M. Zolotov |
Exploration of Europa |
Europa''s icy surface may hide an ocean of liquid water. We summarize the unanswered questions pertaining to Europa following the Galileo mission, and address how those questions will be answered by suggested missions such as EJSM and a lander, as well as new telescopic and laboratory measurements. |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
SETI Institute |
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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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Dirk Schulze-Makuch
Co-Authors: Francois Raulin, Cynthia Phillips, Kevin Hand, Susanne Neuer, Brad Dalton |
Astrobiology Research Priorities for the Outer Solar System |
The outer solar system provides a rewarding assortment of planetary diversity of high interest to astrobiology. This White Paper for the 2009-2011 Planetary Science Decadal Survey evaluates the planetary bodies in the outer solar system and their value to the search for life and astrobiology. |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
Washington State University |
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Mark Allen
Co-Authors: Carrie Anderson, Andrew Coates, A. James Friedson, Murthy Gudipati, Kostas Kalogerakis, Ralph Lorenz, Jonathan Lunine, Catherine Neish, Conor Nixon, Lucy Norman
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Astrobiological Research Priorities for Titan |
Titan, the haze-enshrouded moon of Saturn, has the largest accessible inventory of organic molecules in the Solar System outside of the Earth. The prospects are high for the formation of prebiotic compounds not unlike what might have preceded the origin of life in the early history of the Earth. |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
Jet Propulsion Laboratory |
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J. Hunter, Jr. Waite
Co-Authors: T. Brockwell, D.T. Young, W.S. Lewis, C.P. McKay, Francois Raulin, G. Schubert |
Titan Lake Probe |
This White Paper describes the concept for a Titan Lake Probe, which could be implemented either as an element of a TSSM-type mission or as a stand-alone New Frontiers mission. The Lake Probe could be configured either as a boat or, for increased science return, as a submersible. |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
Southwest Research Institute |
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Candice Hansen
Co-Authors: A.S.Aljabri, D.Banfield, E.B.Bierhaus, M.Brown, J.E.Colwell, M.Dougherty, A.R.Hendrix, H.Hussmann, K.Khurana, D.Landau, A.McEwen, D.A.Paige, C.Paranicas, C.M.Satter, B.Schmidt, M.Showalter, L.J.Spilker, T.Spilker, J.Stansberry, N.Strange, M.Tiscareno, Steve Vance |
Triton science with Argo - A Voyage through the Outer Solar System |
Argo is an innovative pragmatic concept for a New Frontiers 4 mission to significantly expand our knowledge of the outer Solar System. It exploits an upcoming launch window that permits a close Triton encounter during a flyby through the Neptune system, and then continues on to a scientifically-sel |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
Jet Propulsion Laboratory |
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Peter Tsou
Co-Authors: Donald E. Brownlee, Isik Kanic, Christophe Sotin, Linda J. Spilker, Nathan Strange, Joseph Vellinga |
Enceladus Flyby Sample Return, LIFE (Life Investigation For Enceladus) |
One of the most significant discoveries made by the Cassini Mission was finding water ice particles containing organic compounds in the plume emanating from the south pole of Enceladus. Several theories for the origin of life on Earth would also apply to Enceladus. Therefore, it should be of utmos |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
Jet Propulsion Laboratory |
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Ralph Lorenz
Co-Authors: Terry Hurford, Bruce Bills, Frank Sohl, James Roberts, Christophe Sotin, Hauke Hussmann |
The Case for a Titan Geophysical Network Mission |
Notes the science value of a network of small inexpensive landers focussed on Titan geophysics and that if appropriate radioisotope sources are available, this mission could be affordable under New Frontiers. |
Satellites: Galilean satellites, Titan, and the other satellites of the giant planets. |
Johns Hopkins University/
Applied Physics Laboratory |
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Steve Vance
Co-Authors: Ariel Anbar, Donald D. Blankenship, Bonnie Buratti, Julie Castillo, Geoffrey C. Collins, James B. Dalton III, Jack Farmer, Eberhard Grun, Candice Hansen, Terry Hurford, Hauke Hussmann, Jeff Moore, Robert Pappalardo, Cynthia B. Phillips, Frank Postberg, Elizabeth Turtle, Robert Tyler
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Icy Satellite Processes in the Solar System: A plurality of worlds |
A comprehensive strategy for Solar System exploration must identify processes common to icy worlds. Such an approach requires continued investment in discovery focused on icy satellites in the size regime 100 km and larger. We elaborate on this concept, giving specific examples and recommendations |
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. |
Jet Propulsion Laboratory |
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Robert Hodyss
Co-Authors: Paul D. Cooper, Reggie Hudson, Robert Carlson, Paul V. Johnson, Arthur L. Lane, Marla Moore, Louis J. Allamandola |
Recommended Laboratory Studies in Support of Planetary Science: Surface Chemistry of Icy Bodies |
We identify several areas where an increased emphasis on laboratory activities would lead to a significant return in scientific results, based on an enhanced understanding of the fundamental surface chemistry of icy bodies. |
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. |
Jet Propulsion Laboratory |
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Robert J. Noble
Co-Authors: Rashied Amini, Patricia M. Beauchamp, Gary L. Bennett, John R. Brophy, Bonnie J. Buratti, Joan Ervin, Yan R. Fernandez, Will Grundy, Mohammed Omair Khan, David Q. King, Jared Lang, Karen J. Meech, Alan Newhouse, Steven R. Oleson, George R. Schmidt, Thomas Spilker, John L. West
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New Opportunities for Outer Solar System Science using Radioisotope Electric Propulsion |
This whitepaper discusses how mobility provided by radioisotope electric propulsion (REP) opens up entirely new science opportunities for robotic missions to distant primitive bodies. We also give an overview of REP technology developments and the required next steps to realize REP. |
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. |
SLAC National Accelerator Laboratory |
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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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