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.
The Anchorage Museum of History and Art will develop "Lifting the Fog: Russian Exploration in the North Pacific, 1728-1867." This exhibition will reveal the world of the naturalists, oceanographers, astronomers, cartographers, ethnographers and artists who first described the west coast of America and the northern Pacific Ocean to the world. Approximately 200,000 visitors to the museum will view the 5,300-sq. ft. exhibition. Public programs will complement the exhibition, including a family day, lecture series by marine biologists, living history programs, weekend workshops, and an international symposium. An illustrated catalog with interpretive essays and a school curriculum and teachers' guide will accompany the exhibition. The exhibition will travel to three additional venues in the United States.
The Astronomical Society of the Pacific requests $1,317,701 over three years to implement its California pilot project to six sites around the country. Each site will establish local, self- sustaining coalitions linking science centers, astronomical institutions, school districts, and community groups. These coalitions will, with training and support from the national Project ASTRO staff, identify, link, and support the astronomer/teacher partners in their area to use the excitement of astronomy to improve the teaching and learning of science in elementary and middle school. A second strand of the project will use the Project ASTRO materials and techniques to train astronomers and teachers at national meetings outside the six sites to set up individual ASTRO partnerships on their own. Materials to be produced include a: Project ASTRO Coalition Manual; Training Manual; update to the Resource Notebook for the Teaching of Astronomy. Target audiences are students in grades 4-9.
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.