This KISS study program aims to define and develop the ability to simulate a proposed mission concept synthetically ahead of time, where the simulation includes the fundamental physical processes of interest, the characteristics of proposed observations (both intrinsic to any given instrument and how the measurement technique interacts with the physical environment), and finally the ConOps for the mission (e.g., acquisition strategy, orbital parameters, viewing geometry, mission duration, etc.).
This study will evaluate the science case for, and feasibility of, returning samples from the surface, atmosphere, and/or plumes of planetary bodies all across the Solar System, from Mercury to Kuiper Belt Objects beyond Pluto’s orbit.
This study program will bring together theorists, observers, experimentalists, and mission architects to draft an innovative yet practical plan for determining the interior structure of Uranus.
This study will develop a new framework for biological validation for future missions with science driving the instrument development.
This study will leverage previous results from that 2018 KISS study, especially in the realm of science traceability, instrumentation, and concept of operations. This study will dive directly into the mission lifecycle changes required to explore an ISO and LPC and will dive deeper into “rapid response”, develop strategies and identify technologies to enable the up-close exploration of the next ISO or LPC discovered.
This KISS study will examine and advance 1) non-destructive instrumentation to detect biosignatures (agnostic and Earth inspired); 2) sampling techniques to collect and preserve microhabitats while retaining the spatial context; and 3) culturing of acquired microorganisms.
This KISS study will investigate a system architecture with the potential to provide solar-powered transportation to the outer planets and solar power in orbit at the destination.
This KISS study will identify the transformative science that would be enabled by next-generation geodesy at Mars, Venus, and Ocean Worlds and discover the new technologies and mission architectures needed to achieve these scientific advances.
The goal of this study is to explore approaches to the next-generation planetary radar capable of providing compelling science and complementing and motivating NASA science missions as well as potentially providing NASA mission assurance by being able to track spacecraft.
The main goals for this study are to identify the most important measurements related to Decadal survey science questions; to conceive the mission architecture to access the Martian surface (entry-descent-landing; EDL) and conduct efficient operations of multiple Mars assets; and to identify how/if emerging commercial lunar capabilities can be leveraged to break the mass-cost dependency for Mars surface missions.
The goals of this study program are to identify new science missions enabled by a nebula; to quantify benefit to traditional, existing, and planned science missions; to identify candidate mission architectures and demonstration milestones for follow on proposal development for all participants.
This KISS study will emphasize the Jovian system, and Io in particular, as the best laboratory for understanding the fundamental processes of tidal heating.
This KISS study will investigate the best strategies for exploring planetary objects with very long periods such as ‘Oumuamua, the first interstellar visitor ever observed, and comets coming from the Oort cloud.
This study is the incubator for determining science questions, key technologies, collaborations, strategies, and mission proposals that will make deep and wide Mars subsurface access a feasible and affordable reality beyond Mars 2020.
This KISS study is devoted to the question of accessing the subsurface oceans of icy worlds in order to explore these water oceans and to discover the presence of alien extant life. The goal is to review the different technologies that have been developed and to define the technologies that are still required.
This study will establish a core group of researchers and technologists that will be likely to propose a future mission to the Martian polar regions. We will also identify future opportunities to leverage existing facilities for the study of Mars ice analog samples, and testing hardware for future missions
This study will evaluate a comet’s nucleus interior based on the new results from the Rosetta mission and determine the science impact tradeoffs for a series of temperature ranges for a cryogenic comet nucleus sample return mission. It will also determine the technology needs and technology readiness levels (TRLs) for the various temperature ranges narrowed down in the first goal.
The aim of this workshop will be a critical review of a potentially new space exploration strategic approach: field scientific research on planetary surfaces conducted by astronaut/scientists using robotic surrogates when the distance from the scientists to the robots is so short as to provide the illusion of being part of the surface environment without requiring humans to be physically at the site.
This Keck Institute Space Science study will examine the photoelectrochemical production of fuel (such as carbon monoxide) and oxygen from carbon dioxide on the Mars surface. The main technical goals will be to identify specific photoelectrochemical pathways that are well suited for carbon dioxide reduction in the unique Mars environment, as well as viable designs for scalable Mars oxygen and fuel production devices.
This study will investigate whether life could originate in hydrocarbon fluids using Titan as an exemplar of a low temperature exoplanetary surface. It will also investigate other fluids such as liquid and supercritical CO2 suggested to be present on exoplanets.
We will investigate and explore the best route for solving the profound puzzles arising from the recent ground-truth detection of methane on Mars by the Tunable Laser Spectrometer (TLS) onboard Curiosity.
The goal of the study is to devise methods to determine the level of current seismic activity and constrain the global structure that would work in the severe environment of Venus.
The goals of this study program are to develop the science that can be teased out of spaceborne gazing, specific types of targets and applications, the resolution and spectral bands needed to achieve the science, and possible instrument configurations for future missions.
This study will develop innovative, low-cost mission concepts for detecting and mapping polar ice deposits on the Moon.
The goal of this study is to develop new methods to test the radically new understanding of solar system formation that has recently emerged, and to identify innovative instrumentation targeted to this purpose.
This program is conducted to investigate the feasibility of finding, characterizing, robotically capturing, and returning an entire Near Earth Asteroid (NEA) to the vicinity of the Earth.
This study will bring together key technical experts from across the U.S. to advance the study of such surface interactions, deepening our understanding of key mission life-cycle processes: formulation trades, design, mission operations, and in-situ science context and integration.
This program focuses on the potential to developing innovative ideas for future space missions based on the strategy of including a unique cross-fertilization of key experts from multi-institutional backgrounds.
The aim of this program is to take a fresh look at exoplanet characterization science from the point of view of new instruments that could do breakthrough science or that could pave the way for the next generation of space missions.
The goal of this study is to bring together scientists and engineers to discuss the planetary structure and seismological approaches. The outcome of the program will be a critical assessment of whether there are new directions to develop, or existing directions in need of technological impetus.
The aim of this program is to analyze the findings from the recent exploration of the surface of Mars.
The goal of this workshop is to explore new potential mission concepts for the exploration of high-risk planetary surfaces.