The goal of the study is to develop new concepts for in situ sample capture missions, where samples from the Venusian surface or lower atmosphere are delivered to an “airborne laboratory” for analysis. Study participants will identify approaches to in situ sample retrieval and analysis, analyze the feasibility of the approaches, and determine the technology needed and pathways to development.
This 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.
A goal of the KISS study is to explore fundamental questions in black hole physics, to review the science motivation for event horizon scale probes, to assess and explore techniques to connect observations to the underlying black hole physics, and to evaluate what ancillary science might be possible with future space-enhancements to Earth-based arrays like the EHT.
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.
The focus of the study is new approaches toward the search for intelligent life elsewhere in the Universe. We will explore the possible paths for a systematic exploration of observable parameter spaces derived from the modern sky surveys, using machine learning and other computational tools.
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 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.
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 study will bring together space scientists, technologists, and mission designers across two workshops to understand the current limitations faced by SmallSat science missions stemming from the communication bottleneck, and together craft novel technical approaches for optical data transfer that significantly enhances the quality and volume of data returned by these missions.
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.
The goal of this program is to formulate space applications and mission concepts enabled by optical frequency comb technology and to identify high priority technology challenges and gaps that need to be addressed to implement these missions.
This study will consider how three-dimensional (3D) additive construction using in-situ resources can vastly decrease the launch mass required to establish exploration infrastructure on other planetary surfaces.
This study will bring mission designers together with experts in these technologies, resulting in a better understanding of where we can best apply these ideas in space science, and leading toward development of the most promising concepts.
The aim of this study is to inform scientists of the capabilities of airship vehicles as instrumental platforms.
The principal goal of this study is to determine whether emerging technologies could enable crucial oceanographic and space science investigations.
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.
The technical objectives of this program is to identify the set of application areas in space communications and sensing that could benefit from novel quantum-enhanced techniques.
The goal of this study program is to investigate the system capabilities, software architectures and autonomy technologies that will provide the needed resilience for future missions.
The main objective of this study is to identify the technology challenges that must be overcome to advance SmallSat capabilities for revolutionary space science observations.
The aim of this program is to investigate the feasibility of finding, characterizing, robotically capturing, and returning an entire Near Earth Asteroid (NEA) to the vicinity of the Earth.
Our technical goal of this program is to develop a few realistic, benchmark problems on which the methods can be compared, keeping in mind computational resources and available architectures.
The goal of this study is to create a new paradigm in UV/Optical instrument design, detector technology, and optics to form the foundation for the next generation of UV/Optical missions.
The goal of the program is to bring together key technical experts from across the U.S. to advance the study of surface interactions and to deepen our understanding of key mission life-cycle processes. The results will be enabling for many future missions in our solar system.
The goal of this program is to formulate revolutionary technology breakthroughs that will enable the development of sample acquisition systems and relevant instruments capable of in-situ operation during NASA's missions to extremely cold environments.
The aim of this program is to to discuss perspectives regarding the use or improvement of remote sensing techniques to image and measure seismic waves from optical and SAR systems.
This study will significantly advance the capability to build single photon counting array detectors at submillimeter to ultraviolet wavelengths for astronomy, including optical single photon detectors for communications.
The aim of this study is to analyze the state of the art in optical and RF apertures and to make a lasting impact on the field of large space apertures.
The goal of this workshop is to explore new potential mission concepts for the exploration of high-risk planetary surfaces.