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1 | 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 | |||||||||||||||||
2 | Timestamp | Email Address | Title & Status Color Codes: No Color: On track to be submmitted Yellow: Status is not reported Red: Not on track to be submitted | Lead Author Name | List of Coauthors | Are you looking for more coauthors? | Looking for cosigners? | Abstract | Thematic Area | Keywords | Link to Whitepaper Draft | URL to a form/document where Co-Signers and Endorsers can sign up | ||||||
3 | 5/23/2020 14:40:58 | britneys@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 ) | Yes | Yes | (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 | |||||||
4 | 5/26/2020 13:41:17 | geronimo.l.villanueva@nasa.gov | The Present and Future of Observational Studies of Ocean Worlds | Geronimo L. Villanueva | Nixon, Paganini, Cordiner, Milam, Chin et al. | Yes | Yes | 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 | |||||||
5 | 6/4/2020 10:32:48 | stefanie.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 | No | Yes | 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 | |||||||
6 | 6/7/2020 12:07:28 | James.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. | No | Yes | 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 | |||||||
7 | 6/11/2020 6:47:10 | soumyo.dutta@nasa.gov | Aerocapture an an Enhancing Option for Ice Giants Missions | Soumyo Dutta | (see link) | Yes | Yes | 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 | |||||||
8 | 6/12/2020 2:29:46 | alexander.austin@jpl.nasa.gov | Enabling and Enhancing Science Exploration Across the Solar System: Aerocapture Technology for SmallSat to Flagship Missions | Alex Austin | Gonçalo 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 | Yes | Yes | 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 | |||||||
9 | 6/17/2020 23:24:40 | lli7@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.) | Yes | Yes | 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 | ||||||||
10 | 6/19/2020 13:07:42 | imke@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 | Yes | Yes | 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 | |||||||
11 | 6/19/2020 15:41:38 | azari@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 | No | no | 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 | |||||||||
12 | 6/26/2020 16:20:22 | geoffrey.landis@nasa.gov | A Proposed Sample Return from Titan | Geoffrey A. Landis | Geoffrey A. Landis, Steven R. Oleson | Yes | Yes | 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 | ||||||||
13 | 7/8/2020 0:13:44 | mathieu.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 | No | Yes | 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 | ||||||
14 | 7/8/2020 16:24:56 | cindy.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 | Yes | Yes | 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 | |||||||
15 | 10/8/2022 8:58:39 | lokpatit8080@gmail.com | Mr. | Lokpati Tiwari | NA | No | No | OPAG funded meeting attended 2023. | Space teaching service authorized | NASA USRA OPAG funded meeting attended already authorized. | www.nasa.usra.opag.org | www.nasa.usra.com | ||||||
16 | christina.r.richey@jpl.nasa.gov | Equity, Diversity, and Inclusion (EDI) | Christina Richey | Julie 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 Poston | always | always | ||||||||||||
17 | Kathleen.Mandt@jhuapl.edu | Advancing Space Science Requires NASA Support for Coordination between the Science Mission Directorate Communities | Kathleen Mandt | (see link at right) | Yes | Yes | (see link) | Cross-division coordination | https://drive.google.com/file/d/15wKJ1bAH8U8uFcqDFFzPCEagHwaEiz76/view?usp=sharing | |||||||||
18 | chloe.b.beddingfield@nasa.gov & cli@gps.caltech.edu | Exploration 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 Postberg | Yes | Yes | TBD | Ice Giant systems | Uranus, Neptune, Ice Giants, Giant Planets | TBD | ||||||||
19 | rcartwright@seti.org & chloe.b.beddingfield@nasa.gov | The science case for spacecraft exploration of the Uranian satellites | Richard Cartwright & Chloe Beddingfield | C. 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. White | Yes | Yes | See link. | Uranian system | icy satellites, geology, composition, irregular satellites, ring moons | https://drive.google.com/file/d/1CNf0u0CKezmNP1ugFl36FI2A0r0--jBc/view?usp=sharing | ||||||||
20 | erin.j.leonard@jpl.nasa.gov | A 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 Lopes | Yes | Yes | Uranus magnetospheres, moons, and rings | Uranus, icy satellites, ocean worlds, magnetosphere, rings, mission concept, New Frontiers | ||||||||||
21 | kmiller@swri.edu | The value of isotopic measurements as probes of origin, evolution, and habitability | Kelly Miller | Chris Glein, Amy Hofmann, Marc Neveu, Chris House, Bethany Theiling | Yes | Yes | https://docs.google.com/document/d/15jlCeqa8LdqRtUqHHx7UTElWDMc2kVOC429u1cyeD8g/edit?usp=sharing | composition, cosmochemistry, origins, evolution, habitability, biosignatures | TBD | |||||||||
22 | arh@psi.edu | The value of ultraviolet-based science in the solar system | Amanda Hendrix | Kathy 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 Clarke | yes | yes | ||||||||||||
23 | jkeane@caltech.edu | Io | James T. Keane | Catherine 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 Mills | Yes | Yes | TBD | TBD | Io, Jupiter, Ocean Worlds, Tidal Heating | TBD | ||||||||
24 | porter@boulder.swri.edu | Future Telescopes in Support of Outer Planets | Simon Porter | Richard Cartwright, Amanda Hendrix, James Keane, Rebecca Schindhelm, Cindy Young, Michael H. Wong, Kurt Retherford, Tim Livengood, N. Pinilla-Alonso | Yes | Yes | TDB | Hard Infrastructure | Ice Giants, Gas Giants, Dwarf Planets, Long term monitoring, Mission support | |||||||||
25 | cynthia.b.phillips@jpl.nasa.gov | Europa Exploration Strategy | Cynthia Phillips | Chris 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 | Yes | Yes | TBD | Ocean Worlds | Europa, life, icy satellites, ocean worlds | TBD | ||||||||
26 | orkan.umurhan@gmail.com | Exploration 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-Alonso | Yes | Yes | TBD | Outer planet small body exploration | TNOs, Centaurs, Pluto, Charon, Solar System Formation, Solar System Evolution | TBD | ||||||||
27 | cjhansen@psi.edu | Triton | Candy Hansen | Ross 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 Poston | Yes | Yes | 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 | ||||||||||
28 | Peter.Kollmann@jhuapl.edu | Magnetospheric Studies: A requirement for addressing interdisciplinary mysteries in the Ice Giant systems | Peter Kollmann | P. 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 | YES | YES | Ice 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.edu | Ice Giant Atmospheric Science | Emma Dahl | Erika Barth, Rick Cosentino, Kunio Sayanagi, Leigh Fletcher, Heidi Hammel, Csaba Palotai, Raul Morales-Juberias, Amy Simon, Kurt Retherford, Tim Livengood, Shawn Brueshaber | Yes | Yes | ||||||||||||
30 | shawn.r.brueshaber@wmich.edu | The 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) | Yes | Yes | |||||||||||||
31 | jrcasani@jpl.nasa.gov | Enabling a New Generation of Outer Solar System Missions: Engineering Design Studies for Nuclear Electric Propulsion | John 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 | Yes | Yes | 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 | ||||||||
32 | timothy.holt@usq.edu.au | Captured small bodies in the Ice Giant region | Timothy Holt | Julie Castillo, Tilmann Denk4, David Nesvorny2, Simon Porter2, Alyssa Rhoden2, Rebecca Schindhelm5, Anne Verbiscer, N. Pinilla-Alonso, Bonnie Buratti | Yes | Yes | Trojans, Irregular Satellites in the Ice Giant Region | https://docs.google.com/document/d/1p7uVy5Uf1sTcg6dPPAAUd2zp4tk4d8RjoCq7fHoofic/edit?usp=sharing | ||||||||||
33 | helen.hwang@nasa.gov | Thermal Protection System Technologies for Enabling Outer Planet Missions | Helen Hwang | Don Ellerby, Conor Nixon | Yes | Yes | ||||||||||||
34 | helen.hwang@nasa.gov | Thermal Protection System Technologies for Mars/Titan Science Missions | Helen Hwang | Robin Beck, Conor Nixon | Yes | Yes | ||||||||||||
35 | helen.hwang@nasa.gov | Thermal Protection System Sensors | Helen Hwang | Jose Santos | Yes | Yes | ||||||||||||
36 | strappolee@gmail.com | Europa lander as the South Akinson basin lander infusion of funded cold tech | Steven Rappolee | Yes | Cross-division coordination | |||||||||||||
37 | strappolee@gmail.com | Europa Lander as a template for a serialy produced ROW world lander system | Steven Rappolee | yes | Cross-division coordination | |||||||||||||
38 | strappolee@gmail.com | Common science goals and instruments; Row Worlds and Lunar South Pole | Steven Rappolee | Michael Poston | yes | Cross-division coordination | ||||||||||||
39 | ian.cohen@jhuapl.edu | New Frontiers-class Uranus Orbiter: Exploring the feasibility of achieving multidisciplinary science with a mid-scale mission | Ian Cohen | Chloe 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) | Yes | Yes | TBD | Uranian system | Uranus | https://drive.google.com/open?id=1LlGSjbd8uCbgILS7RCKgCgYdF250iuda | ||||||||
40 | Kate.Craft@jhuapl.edu | Ocean World Cryovolcanism and Detection Strategies | Kate Craft | Kate Craft, Catherine Walker, Mike Sori, Conor Nixon, Cindy Young, Julie Rathbun, Kurt Retherford, Wes Patterson, Rosaly Lopes, Jessica Noviello, Rosaly Lopes, Kelsi Singer | yes | yes | TBD | Ocean Worlds | ||||||||||
41 | nicolas.andre@irap.omp.eu | Magnetospheric science onboard ice giant atmospheric probes | Nicolas André | Lea Griton, Quentin Nenon, Ian Cohen, Anna Kotova, Chuanfei Dong, etc | yes | yes | ||||||||||||
42 | Programmatic Balance | Frank Crary as contact | Yes | Yes | ||||||||||||||
43 | Frank.Crary@lasp.colorado.edu | Involving terrestrial scientists: What can we learn from their experience studying Earth | Frank Crary | Ian Cohen, | Yes | Yes | ||||||||||||
44 | Frank.Crary@lasp.colorado.edu | Something about Jupiter's magnetosphere (I'm working on a better title...) | Frank Crary | George Clark, Chuanfei Dong, Liang Wang, Sean Hsu, Anna Kotova, Kurt Retherford, Tim Livengood, Peter Delamere, Elias Roussos | Yes | Yes | ||||||||||||
45 | ebering@central.uh.edu | Solar and Hybrid Electric Propulsion to the Kuiper Belt and Beyond | Edgar Bering | Alex Parker, Franklin Chang Diaz, Jared Squire, Mark Carter, Matthew Giambusso and more | yes | yes | see link at right | Enabling technology | VASIMR®, mission concept, electric propulsion, Saturn, Ice Giants, KBO’s | https://www.dropbox.com/s/29vmc78c4pg9nky/outerPlanetSEP.pdf?dl=0 | ||||||||
46 | ca006@email.uark.edu | Geologic Science Research Priorities for the Moons of Uranus | Caitlin Ahrens | Katherine Dzurilla, Sierra Ferguson, Kathleen Mandt, Kirby Runyon, Mark Hofstadter, Rosaly Lopes | yes | yes | https://drive.google.com/open?id=18xER3ak2t2lN62zwa-ahb075D_QtUsCT | |||||||||||
47 | sean.hsu@lasp.colorado.edu | Ring-planet interactions | Sean Hsu | Frank Crary, Matt Hedman, Luke Moore | yes | yes | ||||||||||||
48 | arh@psi.edu | Enceladus | POC: Amanda Hendrix | Morgan 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 Lopes | https://forms.gle/kjY4HLhAT1b2PRb26 | |||||||||||||
49 | svance@jpl.caltech.edu | Enceladus Distributed Geophysical Exploration | Steven Vance | Marie 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 Tobie | yes | yes | ||||||||||||
50 | Potential Ocean Worlds | Terry Hurford | Marc 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.gov | Europa Clipper Mission (with 3 themes) | Bob Pappalardo | Zach Ulibarri | ||||||||||||||
52 | abigail.rymer@jhuapl.edu | Synergy between Ice Giant and Exoplanet Exploration | Abi Rymer | Lynnae Quick, Anna Kotova, Tim Livengood | ||||||||||||||
53 | geronimo.l.villanueva@nasa.gov | Ocean Worlds Telescope Observations | Geronimo Villanueva | Marc Neveu, Jen Eigenbrode, Amanda Hendrix, Conor Nixon, Richard Cartwright, Kurt Retherford, Tim Livengood, Cesare Grava | ||||||||||||||
54 | william.m.farrell@nasa.gov | Ocean World Modeling/Theory | Bill Farrell | Marc Neveu, Jen Eigenbrode, Amanda Hendrix, Lynnae Quick, Catherine Elder, James Roberts, Conor Nixon, Cesare Grava | ||||||||||||||
55 | ca006@email.uark.edu | The Need for a Facility to Understand Volatile Ice Rheology | Caitlin Ahrens | Orkan Umurhan | ||||||||||||||
56 | reggie.hudson@nasa.gov | Lab research supporting Ocean Worlds exploration | Reggie Hudson | Jen Eigenbrode, Vishaal Singh, Marc Neveu, Zach Ulibarri, Conor Nixon, Julie Castillo, Ellen Czaplinski, Tim Livengood, Kurt Retherford, Michael Poston | ||||||||||||||
57 | 5/27/2020 17:20 | jennifer.c.stern@nasa.gov | Building Consensus and Capability for Ocean Worlds Field Science | Jen Stern | Heather Graham, Margaret Weng, Marc Neveu, Jeff Bowman, Lynnae Quick, Pablo Sabron | Yes | Yes | Field Work | Contact me for a copy! | |||||||||
58 | conor.a.nixon@nasa.gov; stefanie.n.milam@nasa.gov | Ocean 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.edu | New Frontiers Titan Orbiter | Jason Barnes | Shannon 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 Dong | No distinction between coauthors and cosigners/endorsers | Yes | http://barnesos.net/publications/NF_Titan_Orbiter_whitepaper.pdf | |||||||||||
61 | arh@psi.edu | Need for an Ocean Worlds Program | POC: Amanda Hendrix | Catherine 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.gov | Astrobiology as a lens into solar system exploration | Kevin Hand | Cynthia Phillips, Richard Mathies, Anna Butterworth, Heather Graham | ||||||||||||||
63 | trspilker@yahoo.com | Technologies for Outer Solar System exploration in the decade 2023-2032 | Tom Spilker | E. Venkatapathy, J. Zakrajsek, R. Reeve, V. Singh, R Frampton, R Schindhelm, Heather Graham, Tim Livengood | ||||||||||||||
64 | slee@dmns.org | Advanced Developments for In Situ Ocean Worlds Exploration | Steve Lee | Julie Castillo, Tim Livengood | ||||||||||||||
65 | matt@seti.org | Saturn Ring Skimmer | Matt Tiscareno | Matt Hedman, Mar Vaquero, Carol Paty, Frank Crary, Rebecca Schindhelm, the Saturn Ring Skimmer Team | Yes | Yes | TBD | Outer Solar System Exploration | Saturn, Rings, Magnetospheres, Atmospheres, Interiors | TBD | ||||||||
66 | sbrooks@jpl.nasa.gov | Future of Planetary Rings Exploration | POC: Shawn Brooks | Tracy Becker, Matt Hedman | Yes | Yes | ||||||||||||
67 | Glenn.S.Orton@jpl.nasa.gov | Science from Atmospheric Entry Probes in the Outer Solar System | POC: Tom Spilker Lead: Glenn Orton | Shawn Brueshaber, Michael H. Wong, Tim Livengood, Kunio Sayanagi, Dave Atkinson | ||||||||||||||
68 | Shannon.MacKenzie@jhuapl.edu | Titan 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.edu | Gas Giant Atmospheres | Mike Wong | Erika Barth, Shawn Brueshaber, Conor Nixon, Michael H. Wong, Amy Simon, Tim Livengood, Dave Atkinson | ||||||||||||||
70 | Noam.Izenberg@jhuapl.edu | Hopper Missions to Triton and Pluto using a Vehicle with In-Situ Refueling | Noam 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.gov | Planetary Ice Shells as a Science Destination | Sam Howell | Julie Castillo | ||||||||||||||
72 | Morgan.L.Cable@jpl.nasa.gov | Distinguishing Biotic from Abiotic Signatures in Ocean Worlds | POC: Morgan Cable | Marc Neveu, Zach Ulibarri, Conor Nixon, Cindy Young, Jeff Bowman | ||||||||||||||
73 | terry.a.hurford@nasa.gov | Callisto | Terry Hurford | Alex Patthoff, Sierra Ferguson, Richard Cartwright, Amanda Hendrix, Catherine Walker, Tim Livengood, Wes Patterson, Jessica Noviello, Alyssa Mills | ||||||||||||||
74 | krista@ig.utexas.edu | Ice Giant Interiors | POC: Krista Soderlund | Shawn Brueshaber | Yes | Yes | ||||||||||||
75 | schenk@lpi.usra.edu | Chronology (specific to the Outer Solar System) | POC: Paul Schenk | |||||||||||||||
76 | Giant planet migration and the influence of solar system architecture | Timothy Holt | ||||||||||||||||
77 | terry.a.hurford@nasa.gov | Small sats and cube sats for outer solar system science | POC: Terry Hurford | K.-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.edu | Expanding 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 Runyon | yes | Outer 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 Centaurs | Lead TBD | many - original at link at the right, will be updated for submission to Decadal | Yes | Outer Solar System exploration | Uranus, Neptune, KBO, Centaurs | https://arxiv.org/abs/1807.08769 | ||||||||||
80 | stuart@boulder.swri.edu | A White Paper on Pluto Follow On Missions: Background, Rationale, and New Mission Recommendations | Stuart robbins | (see link at right) | Yes | see link at right | Pluto System | Pluto, KBO, Outer Solar System, Water World | https://arxiv.org/abs/1808.07446 | |||||||||
81 | sean.hsu@lasp.colorado.edu | Jupiter System Dynamics Observatory at Sun-Jupiter Lagrangian Point One | Sean Hsu | Frak Crary, Tim Livengood | yes | yes | ||||||||||||
82 | nenon@berkeley.edu | The in-situ exploration of Jupiter's radiation belts | Quentin Nénon | Q. Nénon, I. Jun, P. Kollmann, E. Roussos and everyone else interested; George Clark; Ian Cohen | ||||||||||||||
83 | strappolee@gmail.com | Ice Giant ballistic escape after satellite tour to #SBAG target worlds | Steven Rappolee | |||||||||||||||
84 | strappolee@gmail.com | Neptune Triton B-plane for a retrograde brake on helioscentric access speeds for a sunword trajectory to Chiron | Steven Rappolee | |||||||||||||||
85 | morgan.l.cable@jpl.nasa.gov | Astrobiology Investigations via Plume Flythroughs: 'Impact' of Hypervelocity Sampling on Assessment of Biosignatures and Implications for Enceladus, Europa and Beyond | Morgan Cable | Yes | Yes | Enceladus, Europa, Triton, comets | ||||||||||||
86 | cindy.l.young@nasa.gov | Science that can be accomplished with a space telescope dedicated to planetary science | Cindy Young | |||||||||||||||
87 | cynthia.b.phillips@jpl.nasa.gov | Europa Lander mission concept | Kevin Hand, Cynthia Phillips | Europa Lander mission concept team | ||||||||||||||
88 | conor.a.nixon@nasa.gov | Titan Orbiter With Probes - Mission Concept | Conor 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 | N | Y | https://docs.google.com/document/d/1y6AHKDM1JYGaL0mL6jh6b3c0leBkAQ0d8HFZwkbAbEc/edit?usp=sharing | ||||||||||||
89 | shuvo.mustafi@nasa.gov | Cryogenic Propulsion for Planetary Missions | Shuvo Mustafi | Conor Nixon, Lloyd Purves, Alber Douglawi, Steven Simpson, Ali Hedayat | ||||||||||||||
90 | bethany.p.theiling@nasa.gov | Non-Robotic Science Autonomy Development | Bethany Theiling | Brian Powell, Heather Graham, Lu Chou, Eric Lyness, Jamie Cook, Jennifer Stern, Alex Pavlov, Will Brinckerhoff, Jennifer Eigenbrode, Andrej Grubisic, James McKinnon, Barbara Thompson | yes | yes | machine learning, artificial intelligence, outer solar system exploration | machine learning, Europa, Enceladus, Titan, Mars | https://docs.google.com/document/d/1mGqljtgHVZ5qKz9SXSodg5I347R6nmMkKTn0Pev28Ms/edit?ts=5e30d837 | |||||||||
91 | marc.f.neveu@nasa.gov | Returning Samples from Enceladus for Life Detection | Marc Neveu | Ariel Anbar, Alfonso Davila, Daniel Glavin, Shannon MacKenzie, Charity Phillips-Lander, Brent Sherwood, Yoshinori Takano, Peter Williams, Hajime Yano | Yes | Yes | See link ---> | astrobiology, sample return, ocean world plumes | Enceladus, life detection, sample return | https://docs.google.com/document/d/18OMyf2QMV85ISKKtz6enc6bFJxGXiFe1W5K1f46yvRg/edit?usp=sharing | ||||||||
92 | mark.s.marley@nasa.gov | Overcoming barriers to exoplanet/planetary collaborative science | Mark Marley | |||||||||||||||
93 | giada.n.arney@nasa.gov | Exoplanets in our Backyard: A report from an interdisciplinary community workshop and a call to combined action | Giada Arney, Noam Izenberg | see google doc | yes | yes | ||||||||||||
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