Gas-Grain Simulation Facility: Fundamental studies of particle formation and interactions. Volume 2: Abstracts, candidate experiments and feasibility study

An overview of the Gas-Grain Simulation Facility (GGSF) project and its current status is provided. The proceedings of the Gas-Grain Simulation Facility Experiments Workshop are recorded. The goal of the workshop was to define experiments for the GGSF--a small particle microgravity research facility. The workshop addressed the opportunity for performing, in Earth orbit, a wide variety of experiments that involve single small particles (grains) or clouds of particles. Twenty experiments from the fields of exobiology, planetary science, astrophysics, atmospheric science, biology, physics, and chemistry were described at the workshop and are outlined in Volume 2. Each experiment description included specific scientific objectives, an outline of the experimental procedure, and the anticipated GGSF performance requirements. Since these experiments represent the types of studies that will ultimately be proposed for the facility, they will be used to define the general science requirements of the GGSF. Also included in the second volume is a physics feasibility study and abstracts of example Gas-Grain Simulation Facility experiments and related experiments in progress

Gas-Grain Simulation Facility: Fundamental studies of particle formation and interactions. Volume 1: Executive summary and overview

An overview of the Gas-Grain Simulation Facility (GGSF) project and its current status is provided. The proceedings of the Gas-Grain Simulation Facility Experiments Workshop are recorded. The goal of the workshop was to define experiments for the GGSF--a small particle microgravity research facility. The workshop addressed the opportunity for performing, in Earth orbit, a wide variety of experiments that involve single small particles (grains) or clouds of particles. The first volume includes the executive summary, overview, scientific justification, history, and planned development of the Facility

Space Station Gas-Grain Simulation Facility: Microgravity Particle Research

A wide variety of experiments significant to Exobiology, Planetary Science, Astrophysics, Atmospheric Science, and basic Chemistry and Physics involves the physical interactions of small particles (micrometer to centimeter in size). In many astro-geophysical systems (atmospheric clouds, interstellar clouds, planetary rings, Titan\u27s organic aerosols, Martian dust storms, lightning, etc.), processes involving small particles determine the overall behavior of the system. Condensation of particles from a gas, aggregation of small particles into larger ones, low velocity collisions, and charge accumulation are a few of the processes that influence particles in these systems. Examples of particles undergoing these processes include interstellar grains, protoplanetary particles, atmospheric aerosols, combustion products, and abiotic organic polymers. Although processes of the type described above span a wide range of disciplines, the study of these processes places common fundamental constraints on particle handling. Two common constraints are the need for long time periods during which the particles must be suspended and low relative velocities between particles. Experiments involving small particles generally require material be suspended for periods substantially longer than are practical in Earth\u27s 1 g gravitational field. However, one can investigate these processes with a general-purpose particle research facility (in particular, with the proposed Gas-Grain Simulation Facility) on the Space Station 1 \u273 . Because of the very low gravitational acceleration (microgravity) in the Earth orbital environment, many experiments deemed impractical or impossible to perform on Earth will become feasible. Such experiments are those in which gravity either interferes directly with the phenomenon under study (e.g., gravitational convection masks diffusional processes) or in which gravity precludes the establishment of the proper experimental conditions (e.g., in 1 g, gravity accelerates test objects to unacceptable velocities)

Gas-grain simulation facility: Aerosol and particle research in microgravity

This document reports on the proceedings of the Gas-Grain Simulation Facility (GGSF) Science Workshop which was co-hosted by NASA Ames Research Center and Desert Research Institute, University of Nevada System, and held in Las Vegas, Nevada, on May 4-6, 1992. The intent of the workshop was to bring together the science community of potential GGSF experimenters, Science Working Group and staff members, and the Phase A contractor to review the Phase A design with the science participants and to facilitate communication between the science community and the hardware developers. The purpose of this report is to document the information disseminated at the workshop, to record the participants' review of the Phase A GGSF design concept and the current science and technical requirements for the Facility, and to respond to any questions or concerns that were raised at the Workshop. Recommendations for the future based on numerous discussions with the participants are documented, as well as science presentations and poster sessions that were given at the Workshop and a summary of 21 candidate experiments

Resuspension of Particles by Aerodynamic Deagglomeration

A deagglomerator system was developed, characterized by laboratory tests, and flown under low-gravity (low-g) microgravity conditions. Requirements for a dry powder deagglomeration system were generated by university and National Aeronautics and Space Administration (NASA) scientists from diverse fields of interest including exobiology, planetary sciences, and atmospheric sciences. Existing deagglomeration methods and devices are reviewed. An aerosol generation method suitable for dry powders over a large rang of particle sizes and types at high concentrations with consistent deagglomeration efficiency are evaluated. Development of a pulsed-flow laboratory device and experimental approaches to meet the requirements without being g-dependent are described. Results of laboratory one-g quantitative characterization on one type of dry powder particle generator is discussed. Data from NASA low-g tests are summarized

Exobiology in Solar System Exploration

A symposium, 'Exobiology in Solar System Exploration,' was held on 24-26 Aug. 1988. The symposium provided an in-depth investigation of the role of Exobiology in solar system exploration. It is expected that the symposium will provide direction for future participation of the Exobiology community in solar system exploration and alert the Planetary community to the continued importance of an Exobiology Flight Program. Although the focus of the symposium was primarily on Exobiology in solar system exploration missions, several ground based and Earth-orbital projects such as the Search for Extraterrestrial Intelligence, Gas Grain Facility, and Cosmic Dust Collection Facility represent upcoming research opportunities planned to accommodate the goals and objectives of the Exobiology community as well. This report contains papers for all but one of the presentations given at the symposium