Unicorn Projects, Inc. is producing and distributing a project on the origins of life and its connections to the origin of the universe. The project will present the challenges facing scientists working to unlock universal mysteries and the often painstaking but ultimately rewarding process of the scientific endeavor. It will be designed to reach the lay audience by linking what seem to be abstract and complicated ideas -- like how the universe was born, or how stars evolve -- to issues at the heart of everyday life raised by such simple questions as "Where did we come from?" The components of the project will include: * Four, one-hour television programs for prime time broadcast * An informal science outreach component targeted to middle school-age children and families * Activity kits and training guides adaptable for both informal and formal education * A World Wide WEB site The Co-Executive Producers for the series will be Thomas Levenson and Larry Klein. Levenson has been on the staff of NOVA at WGBH and was producer for the NOVA program on Einstein. Klein has been the producer for numerous science films including "Matters of Life and Death" in the Science Odyssey series. The co-producer for the series and science editor for the project will be Alan Dressler, an astronomer and cosmologist whose principal area of research is the formation and evolution of galaxies. Advisors to the series include: Colleen Cavanaugh, Professor of Organismic and Evolutionary Biology at Harvard University; George V. Coyne, Director of the Vatican Observatory; Douglas Erwin, Research Paleobiologist and Curator at the National Museum of Natural History; Sandra Faber, Professor of Astronomy and University Professor at the UCO/Lick Observatory, UC, Santa Cruz; John P. Grotzinger, Professor at Massachusetts Institute of Technology; Matt Mountain, Director of the Gemini 8M Telescopes project; and Ethan J. Schreier, Astronomer and Associate Director for Operations at the Space Telescope Science Institute. Outreach material will be developed by staff at the Pacific Science Center and implementation will be handled by the AAAS.
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Thomas LevensonLarry KleinBarbara Flagg
The Astronomical Society of the Pacific requests $1,348,428 to enhance the dissemination of Project ASTRO in communities by building new capability into an existing network to serve the "whole family". Family ASTRO will consist of the following components: Six Family Astronomy Kits, in English and Spanish, each consisting of a suite of hands-on activities that can be done with simple materials that are available to a wide range of families. All families will have the capability to perform these activities. A Family Astronomy Events Manual to help partners and site leaders use star parties, Sun, Moon, and Shadows sessions, and other larger group astronomy events into the project. Training protocols and materials at three levels: to train the families in doing astronomy activities directly, to train the astronomy/teachers partners to work with families and to train regional site leaders on the best ways to work with their local partners to start their own Family ASTRO program. The project will have a strong focus on families of underserved populations in science by continuing the work of Project ASTRO sites in urban areas such as Chicago and San Francisco, and in rural areas like southern New Mexico.
The Ft. Worth Museum of Science and History will develop "Texas Dinosaurs: How Do We Know? -- Regional Dissemination of Science Inquiry Exhibits and Educational Programs on Paleontology." This will be a major permanent and portable exhibition project that will be accompanied by an array of educational programs for formal and informal audiences throughout Texas. The permanent 12,000 sq. ft. exhibit, "Texas Dinosaurs: How Do We Know?", will recreate field and laboratory processes of paleontological research in an inquiry approach to public learning in geology, biology, ecology and mathematics. Portable versions of the exhibit will be distributed to the Dinosaur Valley State Park in Glen Rose, the Texas Parks and Wildlife Headquarters, the Panhandle-Plains Historical Museum in Canyon, the Science Spectrum in Lubbock, the McAllen International Museum, and the El Paso Insights Science Museum -- all in Texas. Regional dissemination of "How Do We Know?" exhibits and educational programs and materials will reach at least 1.5 million people annually, including isolated rural communities in the large geographic region of Texas.
Midwestern Wild Weather is a traveling exhibition designed to reach the target audiences in the small/rural communities and the science centers and museums in the states of Illinois, Iowa, Indiana and Michigan. This is a three-year project to replicate five of a set of nine interactive exhibits on the topic of Wild Weather. This exhibition is being produced in collaboration with SPARC (Springfield, Peoria, Aurora, Rockford and Carbondale) which are cities located in the State of Illinois. The project represents a strong model for collaboration between museums, science centers and the formal educational system. An innovative feature of this project design is the use of "attractor" exhibits to entice persons to come to the museum and/or science center. "Many places have talked about doing this but few have tried it." Also, this project has the potential to fill the real need of making available quality exhibits to small museums and bringing informal education resources to small/rural communities. The Science and Technology Interactive Center's cost share for this project is 52.1 percent of the total budget.
The Science Museum of Minnesota (SMM) in collaboration with the Illinois State Museum (ISM), the St. Louis Science Center (SLSC), and the National Center for Supercomputing Applications(NCSA) at the University of Illinois in Champaign, Illinois, will form a museum consortium to develop two virtual reality interactive displays (River Pilot Simulator and Digital River Basin) and other web-based activities that focus on the Mississippi River. This group will be known as the Mississippi River Web Museum Consortium. Each museum will end up with both software modules that will lead visitors to the story of the River. The river's local presence will serve as an entry point for the visitors at each museum. The NCSA will contribute their access to and knowledge of powerful computer simulation, scientific visualization, and collaborations technologies that are usually restricted to research settings and rarely available to a museum audience or the general public. The Consortium will also develop a shared site on the WWW that will invite users to engage in guided inquiry that will deepen their understanding of the large, complex, and integrated river system. The science content underlying the project will include river hydrology and geomorphology, life sciences, environmental studies employing geographic information systems, and the physics of motion. The activities will address a number of the National Science Education Standards. Complementary programming linking these activities with formal education include a RiverWeb(tm) Posting Board and a RiverWeb(tm) Classroom Resource Guide.
Design Technology in After School Programs is a collaboration between science centers and community-based programs to provide "hands on" activities for children age 6-10 in an informal setting. This project enables science centers and community-based organizations to use their expertise to conduct outreach for students and their parents using activities developed. The activities will consist of a variety of design projects that will challenge children to build working models of technological devices. The materials involved in the activities are common everyday items that are usually found around the home. The project will be scaled up each of the three years to reach six science centers and 25-30 after school programs in major areas of the eastern part of the United States. The PI will produce a manual for collaboration and a design technology guide for publication and national dissemination. The cost sharing for this project is 33% of the total project budget.
This Phase I SEPA proposal supports a consortium of science and education partners that will develop System Dynamics (SD) computer models to illustrate basic health science concepts. The consortium includes Oregon Health Sciences University (OHSU), Portland Public Schools (PPS), Saturday Academy, and the Portland VA Medical Center. SD is a computer modeling technique in which diagrams illustrate system structure and simulations illustrate system behavior. Desktop computers and commercial software packages allow SD to be applied with considerable success in K-12 education. NSF grants to Portland Public Schools have trained over 225 high school teachers in Portland and surrounding areas. Two magnet programs have been established with an emphasis on systems and at least five other schools offer significant systems curriculum. Major components of this project include (1) Annual summer research internships at OHSU for high school teachers and high school students, (2) Development of SD models relevant to each research project, (3) Ongoing interactions between high school science programs and OHSU research laboratories, (4) Development of curriculum materials to augment the use of the SD model in the high school classroom or laboratory setting, and (5) Development of video materials to support the classroom teacher. Content will focus on four fundamental models: linear input/exponential output, bi-molecular binding (association/dissociation), population dynamics, and homeostasis. Each of these models is very rich and may be extended to a broad variety of research problems. In addition these models may be combined, for example to illustrate the effect of drugs (binding model) on blood pressure (homeostasis model). System Dynamics is an exemplary tool for the development of materials consistent with National Science Education Standards. SD was specifically developed to emphasize interactions among system structure, organization, and behavior. Students use these material as part of inquiry-based science programs in which the teacher serves as a guide and facilitator rather than the primary source of all content information; technical writing by students is also encouraged. Finally, these SD materials will provide a coherent body of work to guide the ongoing professional development of the classroom science teacher.
Founded in 1999, the Silicon Valley Astronomy Lectures are non-technical illustrated public lectures, presented on six Wednesday evenings during each school year at Foothill College, in the heart of California's Silicon Valley. Speakers over the years have included a Nobel-prize winner, members of the National Academy of Sciences, the first woman in history to discover a planet, an astrophysicist who is an award-winning science fiction writer, and many other well-known scientists explaining astronomical developments in everyday language. The series is jointly sponsored by the Astronomical Society of the Pacific, the SETI Institute, NASA's Ames Research Center, and the Foothill College Astronomy Program. In-kind funding and staff time is contributed by the sponsoring organizations. The lectures are held and videotaped in the 950-seat Smithwick Theater in Los Altos Hills. Thanks to a generous grant from an anonymous local donor, each lecture is now video and audio taped, professionally edited, and made available free of charge on a number of web sites. Videotaped lectures include: * Frank Drake discussing his modern view of the Drake Equation, * Sandra Faber on how galaxies were "cooked" from the primordial soup, * Michael Brown explaining how his discovery of Eris led to the demotion of Pluto, * Alex Filippenko talking about the latest ideas and observations of black holes, * Natalie Batalha sharing the latest planet discoveries from the Kepler mission, * Anthony Aguirre discussing how it is possible to have multiple universes, and * Chris McKay updating the Cassini discoveries about Saturn's moon Titan.