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Total results: 198

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Authors	Title	Summary	Panel Selection	Institution	Download/ Details
Michael D. Max Co-Authors: Stephen M. Clifford, Arthur H. Johnson, Jeremie Lasue	Is a Resource-Mars a Stepping-Stone to Human Exploration of the Solar System?	Methane and water on Mars are the key to a resource base to support sustainable exploration of Mars and beyond	Mars: Not Phobos and Deimos.	MDS Research, LLC	Download File More Details
Mark Skidmore Co-Authors: John Priscu, Brent Christner	Planetary Science & Astrobiology: Cold habitats for life in the Solar system	The paper highlights that improved knowledge of the carbon and energy transformations necessary to support life at sub-zero temperatures is key to future planetary science and astrobiological research given ice is the most abundant phase of water in the Solar system.	Mars: Not Phobos and Deimos. Satellites: Galilean satellites, Titan, and the other satellites of the giant planets.	Montana State University	Download File More Details
David J. Loftus Co-Authors: Erin M. Tranfield, Jon C. Rask, Clara McCrosssin	The Chemical Reactivity of Lunar Dust Relevant to Human Exploration	As NASA prepares to return to the Moon, a clear understanding of the chemistry of lunar dust is required to set the stage for extended duration lunar surface operations. All aspects of the unique environment of the Moon—micrometeorite bombardment, UV light exposure, solar wind radiation, solar parti	Inner Planets: Mercury, Venus, and the Moon.	NASA Ames Research Center	Download File More Details
Edward R. Martinez Co-Author: Robert V. Frampton	Thermal Protection System Sensors	This paper advocates for the development of an aeroshell TPS sensor system to the benefit of all atmospheric reentry missions Agency wide.	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.	NASA Ames Research Center	Download File More Details
Andrew Pohorille Co-Authors: Leslie Bebout, Devaki Bhaya, Rocco Mancinelli	Limits of Terrestrial Life in Space	To pursue a better understanding of life in space and link it to future missions we propose a strategy aimed at determining the potential for terrestrial microbial life to adapt and evolve in space environments. This strategy involves ground-based research, small satellite missions and will culminat	None of the above.	NASA Ames Research Center	Download File More Details
Scott Sandford Co-Authors: Michael A’Hearn, Louis J. Allamandola, Daniel Britt, Benton Clark, Jason P. Dworkin, George Flynn, Danny Glavin, Robert Hanel, Martha Hanner, Fred Hörz, Lindsay Keller, Scott Messenger, Nicholas Smith, Frank Stadermann, Darren Wade, Ernst Zinner, Michael E. Zolensky	The Comet Coma Rendezvous Sample Return (CCRSR) Mission Concept – The Next Step Beyond Stardust	This paper describes the scientific goals and implementation design of the Comet Coma Rendezvous and Sample Return (CCRSR) mission, one of the concept study missions funded by the recent NASA DSCME Program.	Primitive Bodies: Asteroids, comets, Phobos, Deimos, Pluto/Charon and other Kuiper belt objects, meteorites, and interplanetary dust.	NASA Ames Research Center	Download File More Details
Robert Schingler Co-Authors: William Marshall, Alex MacDonald, Mark Lupisella, Brian Lewis	ROSI - Return on Science Investment	A system for mission evaluation based on maximizing science	None of the above.	NASA Ames Research Center	Download File More Details
Tore Straume	Solar Radiation Output: Reading the Record of Lunar Rocks	Reconstructing solar energetic particle output by measuring signatures in lunar surface samples	Inner Planets: Mercury, Venus, and the Moon.	NASA Ames Research Center	Download File More Details
Ethiraj Venkatapathy Co-Authors: Helen H. Hwang, Bernard Laub, Joseph L. Conley, James Arnold, Christine E. Szalai, Jim Tibaudo, Robert Knudsen, Andrew Chambers, David Atkinson, Sushil K. Atreva, Joseph M. Vellinga, William H. Willcockson, Janine M. Thornton, Nicholas G. Smith, Richard A. Hund, John Dec,Max L. Blosser, Michelle M. Munk, Robert Maddock, Prasun N. Desai, Walter Engelund, Stephen Sandford, David A. Gilman, Steven W. Gayle, John Kowal, Christopher B. Madden, Stan Bouslog, Brian J. Remark, Donald Curry, Scott Coughlin, Adam J. Amar, Kevin H. Baines, Tibor Balint, Bernard Bienstock, George T. Chen, James A. Cutts, Jeffery L. Hall, Samad A. Hayati, Pamela J. Hoffman, Linda Spilker, Romasso P. Rivellini, Robert Manning, Eric M. Slimko, Adam D. Steltzner, Thomas Spilker, Jeffrey Umland, Charles Kiskiras, Duane Baker, Thomas Foster, Dominic Calamito, James B. Garvin, Timothy A. Sauerwein, Sharon Seipel, Lori S. Glaze, Spencer Stolis, Mark Lippold, Francis Schwind, James Thompson, Raj Narayan, Thomas Andrews, Conley Thatcher, Edwin B. Curry, John McKinney, Robert Frampton, Todd Stever, Charley Bown, William Congdon, Jennifer Congdon, Daniel M. Empey, Joe Hartman, Dinesh Prabhu, Nancy L. Mangini, Kristina A. Skokova, Margaret M. Stackpoole, Tood White, Howard Goldstein, Melmoth Covington, Robin A. Beck, Carol W. Carroll, Charles A. Smith, Deepak Bose, Anthony Colaprete, David M. Driver, Edward Martinez, Donald T. Ellerby, Matthew J. Gasch, Aga M. Goodsell, James Reuther, Sylvia M. Johnson, Dean Kontinos, Mary Livingston, Michael J. Wright, Harry Partridge, George A. Raiche, Huy K. Tran, Kerry A. Trumble	Thermal Protection System Technologies for Enabling Future Venus Exploration	This paper discusses the capability of currently available TPS and the availability of heritage carbon phenolic used on the Pioneer-Venus probes. A prime conclusion is that there are important issues regarding the availability of the TPS required for future Venus entry probes.	Inner Planets: Mercury, Venus, and the Moon.	NASA Ames Research Center	Download File More Details
Ethiraj Venkatapathy Co-Authors: Christine E. Szalai, Bernard Laub, Helen H. Hwang, Joseph L. Conley, James Arnold, Jim Tibaudo, Robert Knudsen, Andrew Chambers, David Atkinson, Sushil K. Atreva, Joseph M. Vellinga, William H. Willcockson, Janine M. Thornton, Nicholas G. Smith, Richard A. Hund, John Dec, Max L. Blosser, Michelle M. Munk, Robert Maddock, Prasun N. Desai, Walter Engelund, Stephen Sandford, David A. Gilman, Steven W. Gayle, John Kowal, Christopher B. Madden, Stan Bouslog, Brian J. Remark, Donald Curry, Scott Coughlin, Adam J. Amar, Kevin H. Baines, Tibor Balint, Bernard Bienstock, George T. Chen, James A. Cutts, Jeffery L. Hall, Samad A. Hayati, Pamela J. Hoffman, Linda Spilker, Romasso P. Rivellini, Robert Manning, Eric M. Slimko, Adam D. Steltzner, Thomas Spilker, Jeffrey Umland, Charles Kiskiras, Duane Baker, Thomas Foster, Dominic Calamito, James B. Garvin, Timothy A. Sauerwein, Sharon Seipel, Lori S. Glaze, Spencer Stolis, Mark Lippold, Francis Schwind, James Thompson, Raj Narayan, Thomas Andrews, Conley Thatcher, Edwin B. Curry, John McKinney, Robert Frampton, Todd Stever, Charley Bown, William Congdon, Jennifer Congdon, Daniel M. Empey, Joe Hartman, Dinesh Prabhu, Nancy L. Mangini, Kristina A. Skokova, Margaret M. Stackpoole, Tood White, Howard Goldstein, Melmoth Covington, Robin A. Beck, Carol W. Carroll, Charles A. Smith, Deepak Bose, Anthony Colaprete, David M. Driver, Edward Martinez, Donald T. Ellerby, Matthew J. Gasch, Aga M. Goodsell, James Reuther, Sylvia M. Johnson, Dean Kontinos, Mary Livingston, Michael J. Wright, Harry Partridge, George A. Raiche, Huy K. Tran, Kerry A. Trumble	Thermal Protection System Technologies for Enabling Future Sample Return Missions	Currently available TPS materials can meet the needs of Sample Return missions with entry velocity <13 km/s. For entry velocity >13 km/s, heritage carbon phenolic is fully capable, but potentially unavailable and currently available TPS will need to be qualified.	Primitive Bodies: Asteroids, comets, Phobos, Deimos, Pluto/Charon and other Kuiper belt objects, meteorites, and interplanetary dust.	NASA Ames Research Center	Download File More Details
Ethiraj Venkatapathy Co-Authors: James Arnold,Bernard Laub, Helen H. Hwang, Christine E. Szalai, Joseph L. Conley, Jim Tibaudo, Robert Knudsen, Andrew Chambers, David Atkinson, Sushil K. Atreva, Joseph M. Vellinga, William H. Willcockson, Janine M. Thornton, Nicholas G. Smith, Richard A. Hund, John Dec, Max L. Blosser, Michelle M. Munk, Robert Maddock, Prasun N. Desai, Walter Engelund, Stephen Sandford, David A. Gilman, Steven W. Gayle, John Kowal, Christopher B. Madden, Stan Bouslog, Brian J. Remark, Donald Curry, Scott Coughlin, Adam J. Amar, Kevin H. Baines, Tibor Balint, Bernard Bienstock, George T. Chen, James A. Cutts, Jeffery L. Hall, Samad A. Hayati, Pamela J. Hoffman, Linda Spilker, Romasso P. Rivellini, Robert Manning, Eric M. Slimko, Adam D. Steltzner, Thomas Spilker, Jeffrey Umland, Charles Kiskiras, Duane Baker, Thomas Foster, Dominic Calamito, James B. Garvin, Timothy A. Sauerwein, Sharon Seipel, Lori S. Glaze, Spencer Stolis, Mark Lippold, Francis Schwind, James Thompson, Raj Narayan, Thomas Andrews, Conley Thatcher, Edwin B. Curry, John McKinney, Robert Frampton,Todd Stever, Charley Bown, William Congdon, Jennifer Congdon, Daniel M. Empey, Joe Hartman, Dinesh Prabhu, Nancy L. Mangini, Kristina A. Skokova, Margaret M. Stackpoole, Tood White, Howard Goldstein, Melmoth Covington, Robin A. Beck, Carol W. Carroll, Charles A. Smith, Deepak Bose, Anthony Colaprete, David M. Driver, Edward Martinez, Donald T. Ellerby, Matthew J. Gasch, Aga M. Goodsell, James Reuther, Sylvia M. Johnson, Dean Kontinos, Mary Livingston, Michael J. Wright, Harry Partridge, George A. Raiche, Huy K. Tran, Kerry A. Trumble	Thermal Protection System Technologies for Enabling Future Outer Planet Missions	This paper discusses the capability of heritage TPS technology used on the Galileo probe and new materials required for future outer planet probe missions. A prime conclusion is that there are important issues regarding the availability of the TPS required for Outer Planet entry probes.	Giant Planets: Jupiter, Saturn, Uranus, Neptune, and exoplanets, including rings and magnetic fields, but not their satellites.	NASA Ames Research Center	Download File More Details
Ethiraj Venkatapathy Co-Authors: Bernard Laub, Joseph L. Conley, Helen H. Hwang, James Arnold, Christine E. Szalai, Jim Tibaudo, Robert Knudsen, Andrew Chambers, David Atkinson, Sushil K. Atreva, Joseph M. Vellinga, William H. Willcockson, Janine M. Thornton, Nicholas G. Smith, Richard A. Hund, John Dec, Max L. Blosser, Michelle M. Munk, Robert Maddock, Prasun N. Desai, Walter Engelund, Stephen Sandford, David A. Gilman, Steven W. Gayle, John Kowal, Christopher B. Madden, Stan Bouslog, Brian J. Remark, Donald Curry, Scott Coughlin, Adam J. Amar, Kevin H. Baines, Tibor Balint, Bernard Bienstock, George T. Chen, James A. Cutts, Jeffery L. Hall, Samad A. Hayati, Pamela J. Hoffman, Linda Spilker, Romasso P. Rivellini, Robert Manning, Eric M. Slimko, Adam D. Steltzner, Thomas Spilker, Jeffrey Umland, Charles Kiskiras, Duane Baker, Thomas Foster, Dominic Calamito, James B. Garvin, Timothy A. Sauerwein, Sharon Seipel, Lori S. Glaze, Spencer Stolis, Mark Lippold, Francis Schwind, James Thompson, Raj Narayan, Thomas Andrews, Conley Thatcher, Edwin B. Curry, John McKinney, Robert Frampton, Todd Stever, Charley Bown, William Congdon, Jennifer Congdon, Daniel M. Empey, Joe Hartman, Dinesh Prabhu, Nancy L. Mangini, Kristina A. Skokova, Margaret M. Stackpoole, Tood White, Howard Goldstein, Melmoth Covington, Robin A. Beck, Carol W. Carroll, Charles A. Smith, Deepak Bose, Anthony Colaprete, David M. Driver, Edward Martinez, Donald T. Ellerby, Matthew J. Gasch, Aga M. Goodsell, James Reuther, Sylvia M. Johnson, Dean Kontinos, Mary Livingston, Michael J. Wright, Harry Partridge, George A. Raiche, Huy K. Tran, Kerry A. Trumble	Thermal Protection System Technologies for Enabling Future Mars/Titan Science Missions	This paper describes currently available TPS technologies and identifies new technologies needed to support Mars missions in the 2013 - 2022 timeframe, drawing on past mission studies, recent Mars Technology workshop for Mars Sample Return Mission, and the Solar System Exploration road map.	Mars: Not Phobos and Deimos.Satellites: Galilean satellites, Titan, and the other satellites of the giant planets.	NASA Ames Research Center	Download File More Details
Friedemann T. Freund	Previously Overlooked/Ignored Electronic Charge Carriers in Rocks	I would like to draw the attention of members of the Decadal Survey Committee to a rather fundamental discovery, which (I believe) will have a major impact on the Earth and Planetary Sciences in the coming years.	Inner Planets: Mercury, Venus, and the Moon. Mars: Not Phobos and Deimos.	NASA Ames Research Center/ SETI Institute	Download File More Details
Carl Pilcher Co-Authors: Kevin P. Hand, Patricia M. Beauchamp, David Des Marais, David Grinspoon, Karen J. Meech, Sean N. Raymond	Astrobiology Priorities for Planetary Science Flight Missions	We have posited in another white paper that all of Planetary System Science can be seen through an astrobiological lens. In this paper we present priorities for flight mission investigations derived by applying that lens to the Planetary Science flight mission program.	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.	NASA Astrobiology Institute, NASA Ames Research Center	Download File More Details
Carl Pilcher Co-Authors: Kevin P. Hand, Patricia M. Beauchamp, David Des Marais, David Grinspoon, Karen J. Meech, Sean N. Raymond	An Astrobiological Lens on Planetary System Science	Astrobiology provides a lens through which all of planetary science and solar system exploration, as well as life on Earth, can be viewed. Astrobiology, like planetary science, is a systems-level science. In planetary science, one must understand connections be [CHARACTERS NOT ACCEPTED BEYOND THIS	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.	NASA Astrobiology Institute, NASA Ames Research Center	Download File More Details
Michael R. Collier Co-Authors: Thomas E. Cravens, Mats Holmstrom, James Burch, Konrad Dennerl, Herbert Gunell, David G. Sibeck, Steven Snowden, F. Scott Porter, Ina P. Robertson, Nick Omidi, Kip Kuntz, Steven Sembay, Jennifer Carter, Andrew Read, Dimitra Koutroumpa, Massimiliano Galeazzi, Susan Lepri, K.C. Hansen, Dan McCammon, Ruth Skoug, H. Kent Hills, Timothy J. Stubbs, Pavel M. Travnicek, George Fraser, Mark Lester	Global Imaging of Solar Wind-Planetary Body Interactions using Soft X-ray Cameras	We show in this white paper that, with suitable instrumentation on planetary and terrestrial spacecraft, soft X-ray emission associated with the solar wind interaction with planetary neutral atoms can map out the solar wind distribution around planets, including the locations of plasma boundaries.	Inner Planets: Mercury, Venus, and the Moon.	NASA Goddard Space Flight Center	Download File More Details
John F. Cooper Co-Authors: Steven J. Sturner, Chris Paranicas, Matthew E. Hill, Abigail M. Rymer, Paul D. Cooper, Dan Pascu, Robert E. Johnson, Timothy A. Cassidy, Thomas M. Orlando, Kurt D. Retherford, Nathan A. Schwadron, Ralf I. Kaiser, François Leblanc, Louis J. Lanzerotti, Claudia J. Alexander, Henry B. Garrett, Amanda R. Hendrix, Wing H. Ip	Space Weathering Impact on Solar System Surfaces and Mission Science	Space weathering is the collection of physical processes acting to erode and chemically modify planetary surfaces directly exposed to space environments of planetary magnetospheres, the heliosphere, and the local interstellar environment of the solar system. Space weathering affects the physical and	Inner Planets: Mercury, Venus, and the Moon. 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.	NASA Goddard Space Flight Center	Download File More Details
James B. Garvin Co-Authors: Lori S. Glaze, Sushil Atreya, Bruce Campbell, Don Campbell, Peter Ford, Walter Kiefer, Frank Lemoine, Greg Neumann, Roger Phillips, Keith Raney	Venus: Constraining Crustal Evolution from Orbit Via High-Resolution Geophysical and Geological Reconnaissance	Major gaps in understanding Venus include how planetary-scale crustal resurfacing operated, the formation and evolution of highlands, and whether evidence of past environments is preserved. These questions can be addressed through an orbiting radar altimeter and high resolution SAR imager.	Inner Planets: Mercury, Venus, and the Moon.	NASA Goddard Space Flight Center	Download File More Details
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	Download File More Details
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	Download File More Details

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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.