ABCDEFGHIJKLMNOPQR
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New entries to this spreadsheet can be made from the following link:
https://forms.gle/mJTjWAxrB1vR29zVA

To join a whitepaper effort, please email the lead author.

This list is maintained by OPAG. To update or correct entries in this form, please email Kunio Sayanagi <kunio.sayanagi@hamptonu.edu>

LPI maintains a separate coordination effort, which can be accessed from this link: https://www.lpi.usra.edu/decadal_whitepaper_proposals/

For latest information about the decadal survey, please visit the official decadal survey website:
https://www.nationalacademies.org/our-work/planetary-science-and-astrobiology-decadal-survey-2023-2032
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TimestampEmail AddressTitle & Status Color Codes:
No Color: On track to be submmitted
Yellow: Status is not reported
Red: Not on track to be submitted
Lead Author NameList of Coauthors
Are you looking for more coauthors?
Looking for cosigners?AbstractThematic AreaKeywordsLink to Whitepaper DraftURL to a form/document where Co-Signers and Endorsers can sign up
3
5/23/2020 14:40:58britneys@eas.gatech.edu
Enabling Life Detection on Ocean Worlds: Technology Roadmap for Subsurface Access (OPAG SNOW Group Paper)
SNOW Team (Britney Schmidt & Kate Craft Organizing)
B. Schmidt, K. Craft, C. Chivers, J. Lawrence, E. Spiers, S. Pierson, J. Buffo, T. Cwik, K. Zacny, J. Burnett, M. Meister, J. Bowman, E. G. Lightsey, VERNE & Europa STI teams, et al ( to join:
https://docs.google.com/spreadsheets/d/1RnIlsAPuhFmU-uXkqDPcmpz9u3qqNTHzXOY9yEzYxNE/edit?usp=sharing )
YesYes
(Draft) The horizon goal of detecting life in and exploring the oceans of the outer solar system is close to realization, and can be brought closer by a balance of near-term implementation and a 10-year technology development plan to ready new missions to fly in the next decade. We review mission-ready technology for the coming decade, present a plan for enabling advancements that can be achieved in ten years, and comment on programmatic factors that can help a wide range of ambitious and compelling missions to all targets become possible. (Link below goes to collaboration documents)
Ocean Worlds Technology & Science
Europa, Enceladus, Ocean Worlds, Cryobot, crawler, drill, power, communications
https://drive.google.com/open?id=1r3EmSAMTjwFzNzkOgk2Cesjkq1aC85DT
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5/26/2020 13:41:17geronimo.l.villanueva@nasa.gov
The Present and Future of Observational Studies of Ocean Worlds
Geronimo L. Villanueva
Nixon, Paganini, Cordiner, Milam, Chin et al.
YesYes
Do the icy moons, Europa and Enceladus, host habitable conditions at submerged hydrothermal vents? Are there other ocean worlds in our Solar System with similar potential astrobiological significance? The right balance of energy sources, temperature, pressure and chemical diversity leads to prosperous environments for life on Earth. Thanks to the plentitude of recent discoveries of extremophile organisms, the limits for such conditions have greatly expanded, and the hypothesized sub-surface oceans on these moons represent one of the most habitable niches in our Solar System.
The true composition of these habitats and that of the encompassing torus are still unknown, and key compositional studies can provide key insights into the processes sustaining the activity on these bodies and the potential habitability of their sub-surface. Measuring the composition of the plumes will test for chemical diversity of these “oceans,” perhaps indicative of geological activity. For instance, sensitive searches for volatile organics (e.g., CH3OH, H2CO) and sulfur species (e.g., SO2) would establish a rich chemical environment, representing a key parameter in the origin and development of life; while by performing high-resolution mapping, we will be able to identify the regions of active release, and the processes responsible for the activity.
As we discuss in this paper, remote sensing with space and ground-based observatories, in coordination with in-situ remote sensing of these objects will permit to reveal unique information regarding the processes acting on these astrobiologicaly relevants moons, and the potential for habitability of their sub-surface oceans.
Remote Sensing of Ocean Worlds
Astronomy, Spectroscopy, Astrobiology, Molecular, Plumes, Icy Worlds
https://docs.google.com/document/d/13VpTHqBXGm9G1Knpk7AoY9EnVuXOKw5dKyyBY-N54rc/edit
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6/4/2020 10:32:48stefanie.n.milam@nasa.gov
Volatile Sample Return in the Solar System
Stefanie Milam
Jason P. Dworkin, Jamie E. Elsila, Daniel P. Glavin, Perry A. Gerakines, Julie L. Mitchell, Keiko Nakamura-Messenger, Marc Neveu, Larry Nittler, James Parker, Elisa Quintana, Scott A. Sandford, Joshua E. Schlieder, Rhonda Stroud, Melissa G. Trainer, Meenakshi Wadhwa, Andrew J. Westphal, Michael Zolensky
NoYes
We advocate for the realization of volatile sample return from various destinations including: comet nuclei, asteroids/NEOs, the Moon, Mars, ocean worlds/satellites, and plumes. As part of recent mission studies (e.g. CAESAR and Mars Sample Return), new concepts, technologies, and protocols have been considered for specific environments and cost. Here we provide a plan for volatile sample collection and identify the associated challenges with the sampling environment, transit/storage, Earth re-entry, and curation. Laboratory and theoretical simulations are proposed to verify sample integrity during each mission phase. Sample collection mechanisms are evaluated for a given object/environment with consideration for technology and efficient techniques. Transport and curation are essential for sample return to maximize the science investment and ensure pristine samples for terrestrial analysis upon return and after years of preservation. All aspects of a volatile sample return mission are driven by the science motivation: isotope fractionation, noble gases, organics and prebiotic species; plus planetary protection considerations for collection and sample. The analyses of returned samples are not a focus of this white paper since the expectation of sample return is to promote new investigations with state-of-the-art capabilities not necessarily known/employed to date.
• The science value of sample return missions has been clearly demonstrated by previous sample return programs and missions.
• Sample return of volatile material is key to understanding (exo)planet formation, evolution, and habitability.
• Returning planetary volatiles poses unique and potentially severe technical challenges. These include preventing changes to samples between (and including) collection and analyses, and meeting planetary protection requirements.
Sample Return
volatiles, small bodies, Mars, Moon, Ocean Worlds, Plumes
https://docs.google.com/document/d/1M9pEsJFbKXWm61-d9493dRnbTFd-bpgeuTsNldfhLBs/edit#heading=h.xpth65dldtbr
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6/7/2020 12:07:28James.O.Arnold@NASA.gov
Heatshields for Aerogravity Assist Vehicles Whose Deceleration at Titan Saves Mass for Future Flagship Class Exploration of Enceladus
James O. Arnold
T. R. Spilker, Orbital Assembly Corp, D. M. Cornelius, AMA, Inc., G. A. Allen Jr., AMA, Inc., A. M. Brandis, AMA, Inc., D. A. Saunders, AMA, Inc., M. Qu, AMA, Inc., R.W. Powell, AMA, Inc., M. L. Cable, NASA JPL, and R. A. S. Beck, NASA Ames.
NoYes
This paper reports the feasibility of using mature heatshield materials for an aerogravity assist (AGA) vehicle whose deceleration in Titan’s atmosphere is a mass-saving enabler for nine different Enceladus missions (T. Spilker et al. 2009). A geometry for the Titan AGA vehicle is recommended with accompanying high-fidelity flow computations on that shape.
Ocean Worlds, Technology, Outer Planets and their moons
Heatshields, Titan Aerogravity Assist, Enceadus Exploration, Heatshields
https://www.ippw2020.org/decadal-survey-white-papers
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6/11/2020 6:47:10soumyo.dutta@nasa.gov
Aerocapture an an Enhancing Option for Ice Giants Missions
Soumyo Dutta(see link)YesYes
Recent developments in thermal protection systems, guidance and control, and navigation capabilities enable the use of rigid, heritage entry vehicle shapes already flown at Earth, Mars, Venus, Jupiter, and Titan for Ice Giants aerocapture, which could increase the on-orbit mass by 40% and cut the transit time by 2-3 years.
Technology Development, Entry System
Aerocapture, Orbiter, Thermal Protection System, Heatshield, Guidance, Navigation, and Control
https://drive.google.com/file/d/1pWvotVrDO2_CyS_271sRVIzoCLs34RzA/view?usp=sharing
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6/12/2020 2:29:46alexander.austin@jpl.nasa.gov
Enabling and Enhancing Science Exploration Across the Solar System: Aerocapture Technology for SmallSat to Flagship Missions
Alex AustinGonçalo Afonso
Samuel Albert
Hisham Ali
James Arnold
Gilles Bailet
Alan Cassell
Jim Cutts
Rohan Deshmukh
Soumyo Dutta
Charles Edwards
Donald Ellerby
Giusy Falcone
Alberto Fedele
Jay Feldman
Athul Girija
Jeffrey Hill
Tiago Hormigo
Shayna Hume
Vandana Jha
Breanna Johnson
Craig Kluever
Marcus Lobbia
Ping Lu
Ye Lu
Rafael Lugo
Daniel Matz
Robert Moses
Michelle Munk
Adam Nelessen
Isil Sakraker Özmen
Miguel Pérez-Ayúcar
Richard Powell
Zachary Putnam
Thomas Reimer
Sachin Alexander Reddy
Sarag Saika
Stephan Schuster
Jennifer Scully
Ronald Sostaric
Christophe Sotin
Ben Tackett
Ethiraj Venkatapathy
Paul Wercinski
Michael Wright
Cindy Young
YesYes
Aerocapture technology provides a far-reaching capability for missions at destinations across the solar system, from SmallSat to Flagship class. Significant technology development and demonstration in the past decade has prepared high heritage aeroshell shapes to be ready for infusion into missions, particularly at the Ice Giants. In addition, research and focus on drag modulation control schemes has highlighted that this system can enable a new generation of small spacecraft science orbiters as secondary payloads on larger mission’s launches under programs such as SIMPLEx, leading to increased science at a fraction of the cost.
Technology Development, aerocapture
Aerocapture, Titan, Enceladus, Ice Giants, SmallSats
https://drive.google.com/file/d/147nUDAKy4RAsoDk6_0KZ_4OuZAh2w9V5/view?usp=sharing
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6/17/2020 23:24:40lli7@central.uh.edu
Measuring the Radiant Energy Budgets and Internal Heat of Planets and Moons With Future Missions
Liming Li
R.A.West, M.E.Kenyon, C.A. Nixon, P.M. Fry, D. Wenkert, M.D. Hofstadter, A. Sanchez-Lavega, K.H. Baines, A. Mallama, R. Hu, R.K. Achterberg, D. Banfield, U. Dyudina, J.J. Fortney, T. Guillot, A.P. Ingersoll, L. Fletcher, S. Limaye, M.S. Marley, M.D. Smith, K.M. Soderlund (More co-authors are welcome! please contact us.)
YesYes
Knowledge of the radiant energy budgets and internal heat of planets and moons is of wide interest in science community. Some progress has been achieved with recent studies, but there are still significant limitations in current observations and studies. We recommend future missions to better measure the radiant energy budgets and internal heat of planets and moons in our solar system.
Ice Giants and other planets & moons
radiation budget, internal heat, radiative transfer, atmsopheric circulation, and climate change
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6/19/2020 13:07:42imke@berkeley.edu
Studies of the Ice Giants' Deep Atmospheres
Imke de Pater
Bryan Butler - National Radio Astronomy Observatory
R. J. Sault - University of Melbourne
Arielle Moullet - SOFIA
Chris Moeckel - University of California, Berkeley
Joshua Tollefson - University of California, Berkeley
Katherine de Kleer - California Institute of Technology
Mark A. Gurwell - Harvard-Smithsonian Center for Astrophysics
Stefanie Milam - NASA Goddard Space Flight Center
Edward Molter - University of California, Berkeley
Eric Murphy - NRAO
Joe Lazio - JPL
Kirby D. Runyon - JHU/APL
Leigh Fletcher - Leicester Univ, UK
Michael H. Wong
Cheng Li - UC Berkeley
Statia Luszcz-Cook - Columbia Univ.
Glenn Orton - JPL
Mark Hofstadter - JPL
YesYes
The deep atmospheres of the giant planets provide crucial constraints on their composition, an essential parameter in planet formation models. These deep atmospheres can only be probed remotely at radio wavelengths. The next-generation Very Large Array (ngVLA) will enable the highest sensitivity and spatial resolution observations at wavelengths of 0.25-26 cm (1.2-116 GHz), enabling one to derive the composition and atmospheric dynamics of the Ice Giants Uranus and Neptune. A comparison of the ngVLA with a future Ice-Giant mission shows that the ngVLA will provide a spatial resolution at wavelengths $\lesssim$10 cm that is superior over radio instrumentation on an Ice-Giant mission, though measurements from an Ice-Giant orbiter would aid in the calibration of the ground-based measurements. At longer wavelengths an orbiting spacecraft provides a higher spatial resolution if its periapse is within 1.2 planetary radii. The ngVLA will provide invaluable observational support, both scientifically (e.g., full maps over a broader wavelength range with finer spectral sampling than an orbiter) and as a potential ground station for spacecraft telemetry.
groundbased radio telescope
ngVLA, Ice Giants
https://www.overleaf.com/project/5ecc0e2510cd840001b19d79
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6/19/2020 15:41:38azari@berkeley.edu
Integrating Machine Learning for Planetary Science: Perspectives for the Next Decade
Abigail R. Azari
John B. Biersteker, Ryan M. Dewey, Gary Doran, Emily J. Forsberg, Camilla D. K. Harris, Hannah R. Kerner, Katherine A. Skinner, Andy W. Smith
Nono
In past decades planetary science datasets have been constrained in size and number by limited opportunities for measurements. Since the last decadal survey, data collection for planetary science has expanded by orders of magnitude. Data science techniques can help address new challenges and requirements imposed by future mission designs and growing data volumes. Within this white-paper we discuss how data science and machine learning techniques can be integrated into the full mission lifecycle from formulation to operations to archival analysis. We discuss required infrastructure needs and identify barriers and solutions toward realizing the benefits of data science in the field of planetary science. We are actively seeking early-career scientists to contribute as authors (including PhD candidates, postdoctoral researchers, and researchers and faculty). We are also seeking co-signers, participants, and supporters of this effort at all career levels.
Machine learning, Science Analysis, Mission Design
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6/26/2020 16:20:22geoffrey.landis@nasa.govA Proposed Sample Return from Titan Geoffrey A. Landis
Geoffrey A. Landis, Steven R. Oleson
YesYes
We propose to explore a Titan sample return mission using in-situ volatile propellants available on its surface.
Titan is scientifically fascinating in many ways, not the least of which is as a representative of the icy moons of the outer solar system, and a representative of the "water worlds" with liquid oceans under an ice shell. It is also the only body other than the Earth with a hydrological cycle (albeit with rains of methane taking the place of water in the phase-change cycle). Titan is also a high priority target for astrobiology. The surface and atmosphere are rich in the complex organic compounds known as tholins, which are ubiquitous in the outer solar system and Kuiper belt, yet not well understood. These are likely to be the building blocks of the early solar system from which life arose. Samples of Titan’s surface and atmospheric tholins, as well as the many other components of Titan’s surface, would be invaluable. While some analysis of such compounds may be possible using lightweight instruments on board a probe, a detailed investigation of these complex compounds will require an analysis using a full laboratory on Earth. Sample return from Triton would thus have a high science value.
We wish to suggest here that it is possible to do this with credible technology. In Situ Resource Utilization (ISRU) propellant production has been proposed for missions to Mars, the moon, and asteroids, and an initial demonstration of ISRU, production of oxygen from carbon dioxide, will fly to Mars with the Perseverance rover. Titan, however, is nearly an optimal target for ISRU propellant production, with free hydrocarbons available on the surface, and water available in the form of surface rocks. By using the available resources of Titan to produce propellant, a sample return mission would be feasible.
Titan
Titan, sample return, ISRU
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7/8/2020 0:13:44mathieu.choukroun@jpl.nasa.gov
Sampling Ocean Materials, Traces of Life or Biosignatures in Plume Deposits on Enceladus’ Surface
Mathieu Choukroun
Paul Backes, Morgan Cable, Robert Hodyss, Mircea Badescu, Eloise Marteau, Jamie L. Molaro, Scott Moreland, Tom Nordheim, Tyleer Okamoto, Dario Riccobono, Kris Zacny
NoYes
Plume deposit regions on the surface of Enceladus could provide an opportunity for low-cost missions to investigate the composition of another solar system ocean and determine if life exists independent of Earth. The plume deposits likely reflect and preserve the composition of the internal ocean and could contain potential traces of life and biosignatures, if they exist. Laboratory experiments can provide the potential range of surface mechanical properties. The Enceladus surface environment presents unique challenges for sampling including low gravity, vacuum, cryogenic temperatures, and science preference for very shallow (and therefore young) surface samples. The novel Dual-Rasp sampling system uniquely provides the capabilities necessary to acquire the required surface samples. It is under development to achieve TRL 5 in 2021 to make it available for an Enceladus landed mission in the next decade.
Enceladus surface sampling
Enceladus, surface properties, sampling systems
https://drive.google.com/file/d/15wKJ1bAH8U8uFcqDFFzPCEagHwaEiz76/view?usp=sharing
https://docs.google.com/forms/d/e/1FAIpQLSfomWb0C87qG-PAEW80qP9RMaOf1N9fq2i37W7DtlyuY6ckVg/viewform
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7/8/2020 16:24:56cindy.l.young@nasa.gov
The science enabled by a dedicated solar system space telescope
Cindy L. Young
C.L. Young, M.H. Wong, K.M. Sayanagi, S. Curry, K.L. Jessup, T. Becker, A. Hendrix, N. Chanover, S. Milam, B.J. Holler, G. Holsclaw, J. Peralta, J. Clarke, J. Spencer, M.S.P. Kelley, J. Luhmann, D. MacDonnell, R.J. Vervack Jr., K. Rutherford, L.N. Fletcher, I. de Pater, F. Vilas, L. Feaga, A. Simon, O. Siegmund, J. Bell, G. Delory, J. Pitman, T. Greathouse, E. Wishnow, N. Schneider, R. Lillis, J. Colwell, L. Bowman, R.M.C. Lopes, M. McGrath
YesYes
The National Academy Committee on Astrobiology and Planetary Science (CAPS) made a recommendation to study a large/medium-class dedicated space telescope for planetary science, going beyond the Discovery-class dedicated planetary space telescope endorsed in Visions and Voyages. Such a telescope would observe targets across the entire solar system, engaging a broad spectrum of the science community. It would ensure that the high-resolution, high-sensitivity observations of the solar system in visible and UV wavelengths revolutionized by the Hubble Space Telescope could be extended. A dedicated telescope for solar system science would a) transform our understanding of time-dependent phenomena in our solar system that cannot be studied currently under programs to observe and visit new targets and b) enable a comprehensive survey and spectral characterization of minor bodies across the solar system, which requires a large time allocation not supported by existing facilities. The time-domain phenomena to be explored are critically reliant on high spatial resolution UV-visible observations and include: interaction of planetary magnetospheres with the solar wind and internal plasma sources, Venus and giant planet atmospheric dynamics, icy satellite geologic activity and surface evolution, cometary evolution, and evolving ring phenomena. This paper presents science themes and key questions that require a long-lasting space telescope dedicated to planetary science that can capture high-quality, consistent data at the required cadences that are free from the complicating effects of the terrestrial atmosphere and differences across observing facilities. The key questions identified in this whitepaper address the crosscutting themes of planetary science from planetary habitability, origin and evolution of the solar system, and understanding processes that drive present-day dynamics. Such a telescope would have excellent synergy with astrophysical facilities by placing planetary discoveries made by astrophysics assets in temporal context, as well as triggering detailed follow-up observations using larger telescopes. The telescope would also support future missions to the Ice Giants, Ocean Worlds, and minor bodies across the solar system by placing the results of such targeted missions in the context of longer records of temporal activities and larger sample populations.

To signup, please email: cindy.l.young@nasa.gov
multidisciplinary solar system science
space telescope, UV-visible, plumes, volcanism, minor bodies, irregular satellites, dynamics, atmospheres, magnetospheres, rings, comets
https://drive.google.com/file/d/1uy5DwPSQdvPj7G5psT0OAAOkz2hJSl2_/view
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10/8/2022 8:58:39lokpatit8080@gmail.comMr.Lokpati Tiwari NANoNo
OPAG funded meeting attended 2023.
Space teaching service authorized
NASA USRA OPAG funded meeting attended already authorized.
www.nasa.usra.opag.orgwww.nasa.usra.com
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christina.r.richey@jpl.nasa.govEquity, Diversity, and Inclusion (EDI)Christina RicheyJulie Rathbun, The EDI TWG, James Keane, Erin Leonard, Marc Neveu, Alex Patthoff, Amanda Hendrix, Rebecca Schindhelm, Catherine Elder, Lynnae Quick, Tom Nordheim, Richard Cartwright, James Roberts, Chloe Beddingfield, Cynthia Phillips, Michele Bannister, Kirby Runyon, Kurt Retherford, Sam Howell, Steve Vance, Chuanfei Dong, Michael Postonalwaysalways
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Kathleen.Mandt@jhuapl.edu Advancing Space Science Requires NASA Support for Coordination between the Science Mission Directorate CommunitiesKathleen Mandt(see link at right)YesYes(see link)Cross-division coordination
https://drive.google.com/file/d/15wKJ1bAH8U8uFcqDFFzPCEagHwaEiz76/view?usp=sharing
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chloe.b.beddingfield@nasa.gov & cli@gps.caltech.eduExploration of the Ice Giants, Uranus and Neptune
Chloe Beddingfield and Cheng Li
Amy Simon, Chloe Beddingfield, Richard Cartwright, Simon Porter, Erin Leonard, Sierra Ferguson, Kathy Mandt, Catherine Elder, Alex Patthoff, Frank Crary, James Keane, Amanda Hendrix, Lynnae Quick, Matt Hedman, Erika Barth, Ross Beyer, Tom Nordheim, Shawn Brueshaber, James Roberts, Ian Cohen, Timothy Holt, Caitlin Ahrens, Alex Hayes, Carly Howett, Krista Soderlund, N. Pinilla-Alonso, H.-W. Hsu, Frank PostbergYesYesTBDIce Giant systemsUranus, Neptune, Ice Giants, Giant PlanetsTBD
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rcartwright@seti.org & chloe.b.beddingfield@nasa.gov The science case for spacecraft exploration of the Uranian satellitesRichard Cartwright & Chloe BeddingfieldC. Elder, T. Nordheim, R. Pappalardo, B. Buratti, M. Showalter, I. de Pater, W. Grundy, A. Bramson, M. Sori, D. Burr, M. Neveu, J. Roser, M. Hofstadter, A. Masters, I. Cohen, C. Ahrens, K. Aplin, G. Arney, C. Bennett, R. Beyer, C. Bierson, M. Bland, V. Bray, P. Byrne, M. Cameron, J. Castillo-Rogez, N. Chanover, C. Cochrane, G. Collins, A. Coustenis, D. Cruikshank, M. Ćuk, D. DeColibus, R. Dhingra, C. Dong, A. Ermakov, S. Ferguson, R. French, K. Golder, C. Grava, L. Griton, N. Hammond, A. Hayes, P. Helfenstein, A. Hendrix, A. Hofmann, B. Holler, T. Holt, S. Howell, C. Howett, H. Hussmann, H. Hsu, N. Izenberg, R. Jacobsen, D. Jha, R. Juanola-Parramon, I. Jun, J. Keane, E. Karkoschka, S. Kattenhorn, M. Kinczyk, M. Kirchoff, P. Kollmann, E. Leonard, R. Lopes, M. Lucas, A. Lucchetti, E. Martin, J. Moses,A. Barr Mlinar, J. Moore, F. Nimmo, M. Pajola, D.A. Patthoff, S. Peel, G. Peterson, N. Pinilla-Alonso, S. Porter, F. Postberg, M. Poston, A. Probst, L. Quick, A. Ricca, A. Roberge, J. Roberts, S. Robbins, K. Runyon, P. Schenk, M. Schneegurt, F. Scipioni, K. Singer, K. Soderlund, J. Spencer, K. Stephan, T. Stryk, T. Tomlinson, E. Turtle, O. Umurhan, S. Vance, C. Walker, B. Weiss, O. WhiteYesYesSee link.
Uranian systemicy satellites, geology, composition, irregular satellites, ring moons
https://drive.google.com/file/d/1CNf0u0CKezmNP1ugFl36FI2A0r0--jBc/view?usp=sharing
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erin.j.leonard@jpl.nasa.govA New Frontiers Mission to Explore the Uranian magnetosphere, moons, and rings
Erin Leonard (replaced Catherine Elder on 5/27)
T. Nordheim, D.A. Patthoff, E. Leonard, R. Cartwright, C. Cochrane, C. Paranicas, M. Tiscareno, A. Masters, D. Hemingway, M. Sori, H. Cao, R. Pappalardo, B. Buratti, I. De Pater, W. Grundy, M. Showalter, B. Kurth, I. Jun, J. Moses, K. Aplin, J. Casani, M. Poston, E. Nathan, F. Postberg, H.-W. Hsu, Rosaly LopesYesYesUranus magnetospheres, moons, and ringsUranus, icy satellites, ocean worlds, magnetosphere, rings, mission concept, New Frontiers
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kmiller@swri.eduThe value of isotopic measurements as probes of origin, evolution, and habitabilityKelly MillerChris Glein, Amy Hofmann, Marc Neveu, Chris House, Bethany TheilingYesYes
https://docs.google.com/document/d/15jlCeqa8LdqRtUqHHx7UTElWDMc2kVOC429u1cyeD8g/edit?usp=sharing
composition, cosmochemistry, origins, evolution, habitability, biosignaturesTBD
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arh@psi.eduThe value of ultraviolet-based science in the solar systemAmanda HendrixKathy Mandt, Richard Cartwright, Tracy Becker, Joshua Kammer, Kurt Retherford, Tim Livengood, Cesare Grava, N. Pinilla-Alonso, Nick Schneider, Dennis Bodewits, Josh Colwell, Emilie Royer, Jian-Yang Li, Lorenz Roth, Mario De Pra, Greg Holsclaw, John Clarkeyesyes
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jkeane@caltech.eduIoJames T. KeaneCatherine Elder, Alfred McEwen, Kathy Mandt, Paul Schenk, Amanda Hendrix, Ross Beyer, James Roberts, Julie Rathbun, Rosaly Lopes, Kurt Retherford, Cesare Grava, Nick Schneider, Lorenz Roth, Alyssa MillsYesYesTBDTBDIo, Jupiter, Ocean Worlds, Tidal HeatingTBD
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porter@boulder.swri.eduFuture Telescopes in Support of Outer PlanetsSimon PorterRichard Cartwright, Amanda Hendrix, James Keane, Rebecca Schindhelm, Cindy Young, Michael H. Wong, Kurt Retherford, Tim Livengood, N. Pinilla-AlonsoYesYesTDBHard InfrastructureIce Giants, Gas Giants, Dwarf Planets, Long term monitoring, Mission support
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cynthia.b.phillips@jpl.nasa.govEuropa Exploration StrategyCynthia PhillipsChris German, Kate Craft, Sam Howell, Erin Leonard, Marc Neveu, James Keane, Alyssa Rhoden, Amanda Hendrix, Amy Hofmann, Lynnae Quick, Ross Beyer, Catherine Walker, Catherine Elder, Tom Nordheim, James Roberts, Richard Mathies, Anna Butterworth, Alyssa C. Mills, Leonardo Regoli, Kurt Retherford, Anna Kotova, Steve Vance, Wes Patterson YesYesTBDOcean WorldsEuropa, life, icy satellites, ocean worldsTBD
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orkan.umurhan@gmail.comExploration of Dwarf Planets, KBOs and Centaurs
Orkan Omurhan & Kathy Mandt
Amy Simon, Chloe Beddingfield, Richard Cartwright, Simon Porter, Erin Leonard, Sierra Ferguson, Kathy Mandt, Catherine Elder, Alex Patthoff, Frank Crary, James Keane, Amanda Hendrix, Lynnae Quick, Matt Hedman, Erika Barth, Ross Beyer, Tom Nordheim, Shawn Brueshaber, James Roberts, Ian Cohen, Timothy Holt, Kirby Runyon, N. Pinilla-AlonsoYesYesTBDOuter planet small body explorationTNOs, Centaurs, Pluto, Charon, Solar System Formation, Solar System EvolutionTBD
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cjhansen@psi.eduTritonCandy HansenRoss Beyer, Paul Schenk, Alyssa Rhoden, James Keane, Jason Hofgartner, Bonnie Burrati, Walt Harris, Alan Stern, Rebecca Schindhelm, Anne Verbiscer, Simon Porter, Chloe Beddingfield, Marc Neveu, Alex Patthoff, Kathy Mandt, Sierra Ferguson, Raluca Rufu, Vishaal Singh, Erin Leonard, Amanda Hendrix, Lynnae Quick, K.-Michael Aye, Ganna Portyankina, Tom Nordheim, Terry Hurford, Richard Cartwright, Mallory Kinczyk, James Roberts, Zach Ulibarri, Kirby Runyon, Julie Castillo, Alex Hayes, Carly Howett, Rosaly Lopes, Kurt Retherford, Chuanfei Dong, Cesare Grava, Steve Vance, Michael PostonYesYes
Neptune’s moon Triton has been explored by just one spacecraft, Voyager 2, in 1989. Images revealed a unique geologically young surface with cryovolcanic landforms found nowhere else in the solar system. Geysers erupt from a surface with a temperature of just 38K. Triton is noteworthy for its retrograde, highly inclined orbit, making it almost certainly a captured Kuiper Belt dwarf planet. Is Triton an ocean world? Crater counts suggest that Triton’s surface age is <100 Ma, possibly <10 Ma old. Although Triton’s orbit has long since circularized and eccentricity tides are negligible today, obliquity tides could be particularly strong on Triton because of its high inclination orbit. These tides could supply the necessary energy for surface processes that would erase craters, and possibly maintain a liquid layer below the surface. Do the oceans of moons of outer planets provide habitable environments and host life? A mission to Triton answers the call to explore ocean worlds.
http://planetarynews.org/decadal/Triton_case_6_26_2020.pdf
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Peter.Kollmann@jhuapl.eduMagnetospheric Studies: A requirement for addressing interdisciplinary mysteries in the Ice Giant systemsPeter KollmannP. Kollmann, I. Cohen, R. C. Allen, G. Clark, E. Roussos, S. Vines, W. Dietrich, J. Wicht, I. de Pater, K. D. Runyon, R. Cartwright, A. Masters, D. Brain, K. Hibbits, B. Mauk, L. Regoli, Q. Nenon, M. Gkioulidou, A. Rymer, R. McNutt Jr., V. Hue, S. Stanley, G. A. DiBraccio, A. R. Azari, T. Nordheim, L. Wang, A. Kotova, K. Retherford, F. Crary, P. Brandt, C. Dong
YESYESIce Giant magnetospheres and their interaction with all other Ice Giant science.Uranus, Neptune, Ice Giants, Magnetospheres, Radiation Belts, Interiors, Atmospheres, Rings, Moons
https://drive.google.com/file/d/1I1kFQWKLUqnBYZeMwuug2ccDt11gTsu7/view?usp=sharing
29
dahlek@nmsu.eduIce Giant Atmospheric ScienceEmma DahlErika Barth, Rick Cosentino, Kunio Sayanagi, Leigh Fletcher, Heidi Hammel, Csaba Palotai, Raul Morales-Juberias, Amy Simon, Kurt Retherford, Tim Livengood, Shawn BrueshaberYesYes
30
shawn.r.brueshaber@wmich.eduThe need for noble gas measurements for the Giant Planets
POC Shawn Brueshaber (will defer to another person, especially whoever is leading atmospheric probe white paper)
YesYes
31
jrcasani@jpl.nasa.govEnabling a New Generation of Outer Solar System Missions: Engineering Design Studies for Nuclear Electric PropulsionJohn Casani
Alternate contact: Susan D.J. Foster, Technical Editor/Writer,
SDFoster@shipleywins.com
Marc A. Gibson, GRC
David I. Poston, LANL
Nathan J. Strange, JPL
John O. Elliott, JPL
Ralph L. McNutt, Jr., APL
Steven L. McCarty, GRC
Patrick R. McClure, LANL
Steven R. Oleson, GRC
Christophe J. Sotin, JPL
YesYes
https://trs.jpl.nasa.gov/handle/2014/47277
Outer Solar System Exploration
Saturn, Enceladus, Titan, Neptune, Triton, Centaurs, KBO, Pluto, Chiron, Ocean Worlds, Ice Giants, Icy Satellites
https://trs.jpl.nasa.gov/handle/2014/47277
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timothy.holt@usq.edu.auCaptured small bodies in the Ice Giant regionTimothy HoltJulie Castillo, Tilmann Denk4, David Nesvorny2, Simon Porter2, Alyssa Rhoden2, Rebecca Schindhelm5, Anne Verbiscer, N. Pinilla-Alonso, Bonnie BurattiYesYesTrojans, Irregular Satellites in the Ice Giant Region
https://docs.google.com/document/d/1p7uVy5Uf1sTcg6dPPAAUd2zp4tk4d8RjoCq7fHoofic/edit?usp=sharing
33
helen.hwang@nasa.govThermal Protection System Technologies for Enabling Outer Planet MissionsHelen HwangDon Ellerby, Conor NixonYesYes
34
helen.hwang@nasa.govThermal Protection System Technologies for Mars/Titan Science MissionsHelen HwangRobin Beck, Conor NixonYesYes
35
helen.hwang@nasa.govThermal Protection System SensorsHelen HwangJose SantosYesYes
36
strappolee@gmail.comEuropa lander as the South Akinson basin lander infusion of funded cold techSteven RappoleeYes
Cross-division coordination
37
strappolee@gmail.comEuropa Lander as a template for a serialy produced ROW world lander systemSteven Rappoleeyes
Cross-division coordination
38
strappolee@gmail.comCommon science goals and instruments; Row Worlds and Lunar South PoleSteven RappoleeMichael PostonyesCross-division coordination
39
ian.cohen@jhuapl.eduNew Frontiers-class Uranus Orbiter: Exploring the feasibility of achieving multidisciplinary science with a mid-scale missionIan CohenChloe Beddingfield (added-ijc), Richard Cartwright (added-ijc), Shawn Brueshaber (added-ijc), Caitlin Ahrens (added-ijc), Leonardo Regoli (added-ijc), Chuanfei Dong (added-ijc), Athul P. Girija (added-ijc), George Clark (added-ijc), Kathy Mandt (added-ijc)YesYesTBDUranian systemUranus
https://drive.google.com/open?id=1LlGSjbd8uCbgILS7RCKgCgYdF250iuda
40
Kate.Craft@jhuapl.eduOcean World Cryovolcanism and Detection StrategiesKate CraftKate Craft, Catherine Walker, Mike Sori, Conor Nixon, Cindy Young, Julie Rathbun, Kurt Retherford, Wes Patterson, Rosaly Lopes, Jessica Noviello, Rosaly Lopes, Kelsi SingeryesyesTBDOcean Worlds
41
nicolas.andre@irap.omp.euMagnetospheric science onboard ice giant atmospheric probesNicolas AndréLea Griton, Quentin Nenon, Ian Cohen, Anna Kotova, Chuanfei Dong, etcyesyes
42
Programmatic BalanceFrank Crary as contactYesYes
43
Frank.Crary@lasp.colorado.eduInvolving terrestrial scientists: What can we learn from their experience studying EarthFrank CraryIan Cohen, YesYes
44
Frank.Crary@lasp.colorado.eduSomething about Jupiter's magnetosphere (I'm working on a better title...)Frank CraryGeorge Clark, Chuanfei Dong, Liang Wang, Sean Hsu, Anna Kotova, Kurt Retherford, Tim Livengood, Peter Delamere, Elias RoussosYesYes
45
ebering@central.uh.eduSolar and Hybrid Electric Propulsion to the Kuiper Belt and BeyondEdgar BeringAlex Parker, Franklin Chang Diaz, Jared Squire, Mark Carter, Matthew Giambusso and moreyesyessee link at rightEnabling technologyVASIMR®, mission concept, electric propulsion, Saturn, Ice Giants, KBO’s
https://www.dropbox.com/s/29vmc78c4pg9nky/outerPlanetSEP.pdf?dl=0
46
ca006@email.uark.eduGeologic Science Research Priorities for the Moons of UranusCaitlin AhrensKatherine Dzurilla, Sierra Ferguson, Kathleen Mandt, Kirby Runyon, Mark Hofstadter, Rosaly Lopesyesyes
https://drive.google.com/open?id=18xER3ak2t2lN62zwa-ahb075D_QtUsCT
47
sean.hsu@lasp.colorado.eduRing-planet interactionsSean HsuFrank Crary, Matt Hedman, Luke Mooreyesyes
48
arh@psi.eduEnceladusPOC: Amanda HendrixMorgan Cable, Shannon MacKenzie, Marc Neveu, Jen Eigenbrode, Edwin Kite, Alex Patthoff, Richard Cartwright, Kathy Mandt, Erin Leonard, Alyssa Rhoden, Sierra Ferguson, Vishaal Singh, James Keane, Amy Hofmann, Anya Portyankina, K.-Michael Aye, Catherine Elder, Tom Nordheim, Mallory Kinczyk, James Roberts, Chloe Beddingfield, Zach Ulibarri, Richard Mathies, Anna Butterworth, Kirby Runyon, Joshua Kammer, Kurt Retherford, Tim Livengood, Sam Howell, Wes Patterson, Michael Poston, Rosaly Lopeshttps://forms.gle/kjY4HLhAT1b2PRb26
49
svance@jpl.caltech.eduEnceladus Distributed Geophysical ExplorationSteven VanceMarie Behounkova, Bruce Bills, Ondrej Cadek, Gael Choblet, Kynan Hughson, Ana Lobo, Angela Marusiak, Mohit Melwani Daswani, Ceri Nunn, Mark Panning, Britney Schmidt, Ondrej Soucek, Simon Stähler, Saikiran Tharimena, Andrew Thompson, Gabriel Tobieyesyes
50
Potential Ocean WorldsTerry HurfordMarc Neveu, Alex Patthoff, Erin Leonard, Alyssa Rhoden, Amanda Hendrix, Kathy Mandt, Lynnae Quick, Kate Craft, Chloe, Beddingfield, Kirby Runyon, Julie Castillo, Sam Howell, Wes Patterson, Michael Poston, Rosaly Lopes, Jessica Noviello, Alyssa Mills
51
robert.pappalardo@jpl.nasa.govEuropa Clipper Mission (with 3 themes)Bob PappalardoZach Ulibarri
52
abigail.rymer@jhuapl.eduSynergy between Ice Giant and Exoplanet ExplorationAbi RymerLynnae Quick, Anna Kotova, Tim Livengood
53
geronimo.l.villanueva@nasa.govOcean Worlds Telescope ObservationsGeronimo VillanuevaMarc Neveu, Jen Eigenbrode, Amanda Hendrix, Conor Nixon, Richard Cartwright, Kurt Retherford, Tim Livengood, Cesare Grava
54
william.m.farrell@nasa.govOcean World Modeling/TheoryBill FarrellMarc Neveu, Jen Eigenbrode, Amanda Hendrix, Lynnae Quick, Catherine Elder, James Roberts, Conor Nixon, Cesare Grava
55
ca006@email.uark.eduThe Need for a Facility to Understand Volatile Ice RheologyCaitlin AhrensOrkan Umurhan
56
reggie.hudson@nasa.govLab research supporting Ocean Worlds explorationReggie HudsonJen Eigenbrode, Vishaal Singh, Marc Neveu, Zach Ulibarri, Conor Nixon, Julie Castillo, Ellen Czaplinski, Tim Livengood, Kurt Retherford, Michael Poston
57
5/27/2020 17:20jennifer.c.stern@nasa.govBuilding Consensus and Capability for Ocean Worlds Field ScienceJen SternHeather Graham, Margaret Weng, Marc Neveu, Jeff Bowman, Lynnae Quick, Pablo SabronYesYesField WorkContact me for a copy!
58
conor.a.nixon@nasa.gov; stefanie.n.milam@nasa.govOcean Worlds Interdisciplinary Science
Conor Nixon and Stefanie Milam
Jen Eigenbrode, Tim Livengood
59
Neptune + Triton: A flagship for everyone
Contacts: Abi Rymer, Carol Paty
Draft Outline to be posted 7/21
Frank Crary, Amanda Hendrix, Lynnae Quick, Matt Hedman, Ganna Portyankina, K.-Michael Aye, Kathy Mandt, Shawn Brueshaber, James Roberts, Timothy Holt, Chloe Beddingfield, Kirby Runyon, Julie Rathbun, Alex Hayes, Ian Cohen, Joe Caggiano, Paul Regensburger, Angela Olsen, Rosaly Lopes, Caitlin Ahrens, Katherine Dzurilla, Tracy Becker, Abigail Azari, George Clark, Liang Wang, Wes Patterson, Chuanfei Dong, Frank Postberg, Kurt Retherford
60
jwbarnes@uidaho.eduNew Frontiers Titan OrbiterJason BarnesShannon MacKenzie, Kathy Mandt, Amanda Hendrix, Paul Hayne, Erika Barth, Conor Nixon, Shawn Brueshaber, Sam Birch, Ellen Czaplinski., Alex Hayes, Rosaly Lopes, Leonardo Regoli, Tim Livengood, Chuanfei DongNo distinction between coauthors and cosigners/endorsersYes
http://barnesos.net/publications/NF_Titan_Orbiter_whitepaper.pdf
61
arh@psi.eduNeed for an Ocean Worlds ProgramPOC: Amanda HendrixCatherine Elder, Cynthia Phillips, Erin Leonard, Lynnae Quick, Zach Ulibarri, Conor Nixon, Julie Castillo, Jeff Bowman, Joshua Kammer, Richard Cartwright, Wes Patterson, Kurt Retherford, Michael Poston
62
kevin.p.hand@jpl.nasa.govAstrobiology as a lens into solar system explorationKevin HandCynthia Phillips, Richard Mathies, Anna Butterworth, Heather Graham
63
trspilker@yahoo.comTechnologies for Outer Solar System exploration in the decade 2023-2032Tom SpilkerE. Venkatapathy, J. Zakrajsek, R. Reeve, V. Singh, R Frampton, R Schindhelm, Heather Graham, Tim Livengood
64
slee@dmns.orgAdvanced Developments for In Situ Ocean Worlds ExplorationSteve LeeJulie Castillo, Tim Livengood
65
matt@seti.orgSaturn Ring SkimmerMatt TiscarenoMatt Hedman, Mar Vaquero, Carol Paty, Frank Crary, Rebecca Schindhelm, the Saturn Ring Skimmer TeamYesYesTBDOuter Solar System ExplorationSaturn, Rings, Magnetospheres, Atmospheres, InteriorsTBD
66
sbrooks@jpl.nasa.govFuture of Planetary Rings ExplorationPOC: Shawn BrooksTracy Becker, Matt HedmanYesYes
67
Glenn.S.Orton@jpl.nasa.govScience from Atmospheric Entry Probes in the Outer Solar SystemPOC: Tom Spilker
Lead: Glenn Orton
 Shawn Brueshaber, Michael H. Wong, Tim Livengood, Kunio Sayanagi, Dave Atkinson
68
Shannon.MacKenzie@jhuapl.eduTitan Science
POC: Shannon MacKenzie
Amy Hofmann, Erika Barth, Conor Nixon, Ellen Czaplinski, Sam Birch, Alex Hayes, Rosaly Lopes, Leonardo Regoli, Tim Livengood
69
mikewong@astro.berkeley.eduGas Giant AtmospheresMike WongErika Barth, Shawn Brueshaber, Conor Nixon, Michael H. Wong, Amy Simon, Tim Livengood, Dave Atkinson
70
Noam.Izenberg@jhuapl.eduHopper Missions to Triton and Pluto using a Vehicle with In-Situ RefuelingNoam Izenberg
Geoffrey A. Landis, Steven R. Oleson, Phillip Abel, Michael Bur, Anthony Colozza, Brent Faller, James Fittje, John Gyekenyesi, Jason Hartwig, Robert Jones, Nicholas Lantz, Steven McCarty, Thomas Packarb, Paul Schmitz, David Smith, Elizabeth Turnbull, Miles McKaig, and Thomas O’Brien
71
samuel.m.howell@jpl.nasa.govPlanetary Ice Shells as a Science DestinationSam HowellJulie Castillo
72
Morgan.L.Cable@jpl.nasa.govDistinguishing Biotic from Abiotic Signatures in Ocean WorldsPOC: Morgan CableMarc Neveu, Zach Ulibarri, Conor Nixon, Cindy Young, Jeff Bowman
73
terry.a.hurford@nasa.govCallistoTerry HurfordAlex Patthoff, Sierra Ferguson, Richard Cartwright, Amanda Hendrix, Catherine Walker, Tim Livengood, Wes Patterson, Jessica Noviello, Alyssa Mills
74
krista@ig.utexas.eduIce Giant InteriorsPOC: Krista SoderlundShawn BrueshaberYesYes
75
schenk@lpi.usra.eduChronology (specific to the Outer Solar System)POC: Paul Schenk
76
Giant planet migration and the influence of solar system architectureTimothy Holt
77
terry.a.hurford@nasa.govSmall sats and cube sats for outer solar system sciencePOC: Terry HurfordK.-Michael Aye, Catherine Walker, Conor Nixon, Cindy Young, Julie Castillo, Michele Bannister, George Clark, Robert Ebert, Michael H. Wong, Frank Crary, Leonardo Regoli, Tim Livengood, Padma A. Yanamandra-Fisher, Kurt Retherford
78
m.bannister@qub.ac.uk, bholler@stsci.eduExpanding horizons: the need for direct exploration of the diverse trans-Neptunian Solar System
Michele Bannister and Bryan Holler
Susan D. Benecchi, Cristina M. Dalle Ore, Leigh N. Fletcher, Aurelie Guilbert–Lepoutre, Csaba Kiss, Pedro Lacerda, Michael Marsset, Alex Parker, Noemi Pinilla-Alonso, Amy Simon, Kelsi Singer, Alan Stern, Darin Ragozzine, Mark Tapley, Chad Trujillo, Hajime Yano, Leslie Young, Kirby RunyonyesOuter Solar System exploration
79
amy.simon@nasa.gov, mark.hofstadter@jpl.nasa.gov
Outer Solar System Exploration: A Compelling and Unified Dual Mission Decadal Strategy for Exploring Uranus, Neptune, Triton, Dwarf Planets, and Small KBOs and CentaursLead TBDmany - original at link at the right, will be updated for submission to DecadalYesOuter Solar System explorationUranus, Neptune, KBO, Centaurs
https://arxiv.org/abs/1807.08769
80
stuart@boulder.swri.eduA White Paper on Pluto Follow On Missions: Background, Rationale, and New Mission RecommendationsStuart robbins(see link at right)Yessee link at rightPluto SystemPluto, KBO, Outer Solar System, Water World
https://arxiv.org/abs/1808.07446
81
sean.hsu@lasp.colorado.eduJupiter System Dynamics Observatory at Sun-Jupiter Lagrangian Point OneSean HsuFrak Crary, Tim Livengoodyesyes
82
nenon@berkeley.eduThe in-situ exploration of Jupiter's radiation beltsQuentin NénonQ. Nénon, I. Jun, P. Kollmann, E. Roussos and everyone else interested; George Clark; Ian Cohen
83
strappolee@gmail.comIce Giant ballistic escape after satellite tour to #SBAG target worldsSteven Rappolee
84
strappolee@gmail.comNeptune Triton B-plane for a retrograde brake on helioscentric access speeds for a sunword trajectory to ChironSteven Rappolee
85
morgan.l.cable@jpl.nasa.govAstrobiology Investigations via Plume Flythroughs: 'Impact' of Hypervelocity Sampling on Assessment of Biosignatures and Implications for Enceladus, Europa and BeyondMorgan CableYesYes
Enceladus, Europa, Triton, comets
86
cindy.l.young@nasa.govScience that can be accomplished with a space telescope dedicated to planetary scienceCindy Young
87
cynthia.b.phillips@jpl.nasa.govEuropa Lander mission concept
Kevin Hand, Cynthia Phillips
Europa Lander mission concept team
88
conor.a.nixon@nasa.govTitan Orbiter With Probes - Mission ConceptConor Nixon, James Abshire, Mathieu Choukroun, Jason D. Hofgartner, Juan Lora, Ralph D. Lorenz, Kathleen Mandt, Darci Snowden, Melissa G. Trainer, Xi Zhang, J. Barnes, N. Carrasco, A. Coustenis, N. Edberg, L. Iess, R. Lopes, A. Luspay-Kuti, M. Mastrogiuseppe, E. Mazarico, A. Solomonidou, X. Sun, N. Teanby, O. Tucker, E. Turtle,
G. Tobie, U. Nantes, V. Vuitton
NY
https://docs.google.com/document/d/1y6AHKDM1JYGaL0mL6jh6b3c0leBkAQ0d8HFZwkbAbEc/edit?usp=sharing
89
shuvo.mustafi@nasa.govCryogenic Propulsion for Planetary MissionsShuvo Mustafi
Conor Nixon, Lloyd Purves, Alber Douglawi, Steven Simpson, Ali Hedayat
90
bethany.p.theiling@nasa.govNon-Robotic Science Autonomy DevelopmentBethany TheilingBrian Powell, Heather Graham, Lu Chou, Eric Lyness, Jamie Cook, Jennifer Stern, Alex Pavlov, Will Brinckerhoff, Jennifer Eigenbrode, Andrej Grubisic, James McKinnon, Barbara Thompsonyesyesmachine learning, artificial intelligence, outer solar system explorationmachine learning, Europa, Enceladus, Titan, Mars
https://docs.google.com/document/d/1mGqljtgHVZ5qKz9SXSodg5I347R6nmMkKTn0Pev28Ms/edit?ts=5e30d837
91
marc.f.neveu@nasa.govReturning Samples from Enceladus for Life DetectionMarc NeveuAriel Anbar, Alfonso Davila, Daniel Glavin, Shannon MacKenzie, Charity Phillips-Lander, Brent Sherwood, Yoshinori Takano, Peter Williams, Hajime YanoYesYesSee link --->astrobiology, sample return, ocean world plumesEnceladus, life detection, sample return
https://docs.google.com/document/d/18OMyf2QMV85ISKKtz6enc6bFJxGXiFe1W5K1f46yvRg/edit?usp=sharing
92
mark.s.marley@nasa.govOvercoming barriers to
exoplanet/planetary
collaborative science
Mark Marley
93
giada.n.arney@nasa.govExoplanets in our Backyard: A report from an interdisciplinary community workshop and a call to combined action
Giada Arney, Noam Izenberg
see google docyesyes
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