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resource project Exhibitions
Chabot Space and Science Center is developing and organizing a major traveling exhibit called "Dragon Skies: Astronomical Instruments of Imperial China." The exhibit will consist of nine Chinese astronomical instruments, dating between 1439 and 1744, as well as 25 smaller artifacts. In addition, a variety of interpretive materials and activities will be developed to enhance the exhibit. The PI, Michael Reynolds, has visited the Ancient Beijing Observatory and begun initial conversations with the staff there, resulting in tentative collaboration agreements. Subsequent to that visit, the Ancient Beijing Observatory has already determined which original instruments will be able to travel, has replicated several exhibits, and has compiled a collection of additional artifacts that will enhance the exhibit. The planning phase will be carried out by staff from Chabot, the Beijing Ancient Observatory, the Chinese Astronomical Society, and a team of advisors. Planning activities will include: Decide which aspects of exhibit development will be taken on by each partner; Determine what ancillary materials will need to be developed; Establish what interactive activities, such as hands-on activities or computer kiosks, will enhance the project; Determine what multimedia programs, such as an audio tour or planetarium shows, will increase the impact of the exhibit; Determine the translation needs for the exhibit and for the supplemental materials and programs; Arrange the logistics for the traveling exhibit; Establish criteria for venues that might display the exhibit and identify potential sites.
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TEAM MEMBERS: Michael Reynolds
resource project Exhibitions
The Buffalo Bill Historical Center will develop the "Greater Yellowstone Adventure project," encompassing 1,719 square meters of exhibits in the Center's newly constructed Draper Museum of Natural History. The exhibits and associated programming constitute a major cultural and educational resource for underserved residents of rural, northwestern Wyoming and approximately 500,000 annual visitors to the region. The goal of Greater Yellowstone Adventure is to promote understanding of the relationships binding humans and nature and the use of science in exploring those relationships. The exhibits are orgainized into three galleries: Expedition Trailhead, Braided Paths and Tangled Destinies, and Seasons of Discovery.
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TEAM MEMBERS: Charles Preston Maryanne Adrus Eugene Reber Robert Pickering Marcia Britton
resource project Exhibitions
The Lawrence Hall of Science (LHS) proposes to develop a permanent, one-acre, outdoor exhibition overlooking the San Francisco Bay called called "The Forces That Shape the San Francisco Bay." The exhibition will focus on the geologic and hydrologic forces and the human impacts that have shaped the San Francisco Bay and its environs. The exhibition's interactive components and related programs will involve visitors in learning about erosion, river sediment and deposition, mountain building, folding of strata and thrusting, faulting and seismicity.
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TEAM MEMBERS: Ian S. Carmichael
resource project Public Programs
The Independence Seaport Museum will create "Boat Building: Art and Science," a 3,000-square foot permanent exhibit that is designed to educate visitors about the science of boat building and design. Concepts such as buoyancy, water displacement, turbulence and drag will be explored through interactives, maritime artifacts, models and oral histories of tradesmen. By using the principles identified by the Family Science Learning Research Project of the Philadelphia/Camden Informal Science Education Collaborative (PISEC), the exhibit will be user-friendly for families with young children. Visitor workstation topics may include boat building, floating, buoyancy, sails, wind and boat shape. Visitors will use science processes while learning through open-ended play and exploration. Creative programs for families and school groups, as well as curriculum materials will support the exhibit. A website and technical training manual will also be produced. Four phases of evaluation are planned, and include front-end analysis which will incorporate focus groups with children ages 7-12, and formative evaluation using prototypes of interactives. Remedial evaluation will be carried out once the exhibit opens, and summative evaluation will use tracking and exit interviews to assess learning and understanding. The estimated annual audience of over 130,000 visitors will be expanded by replicating and traveling various components to other maritime museums in partnership with the Association of Science and Technology Centers. Evaluation of traveling components will also be undertaken to determine if they present an appropriate model for maritime-based exhibits.
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TEAM MEMBERS: David Beard Roberta Cooks
resource project Exhibitions
The Great Lakes Story is a 3,000 sq. ft. interactive traveling exhibit based on the highly successful and unique permanent exhibition at the Great Lakes Science Center. Its focus is devoted to highlighting the natural history of the Great Lakes ecosystem. The traveling exhibit will allow even more visitors around the country to understand the beauty, majesty and restoration efforts of this important national resource. Through a planned six-year tour, it is estimated "The Great Lakes Story" will be experienced by as many as three million people. There will be several components, including hands-on exhibits, organized with a centerpiece of a walk-around model of the Great Lakes region, and other interactive components. The four major areas of the exhibit are physical characteristics of the Lakes, the natural cycles and processes which shaped them over time, changes and threats to the Lakes (especially human-induced), and finally, restoration efforts to bring the Lakes back to being the rich and productive ecosystem they should be. Along with these exhibit areas, other project components are educational and marketing materials to ensure that host science centers are able to provide a complete learning experience to their youth, family, and adult audiences around the country.
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TEAM MEMBERS: Valence Davillier Andrew McDowell
resource project Exhibitions
The California Science Center Foundation will develop the California Science Center's Air and Space Gallery, a 12,000-square foot exhibit space. The California Science Center will reopen Aerospace Hall (closed in 1998) with new and re-designed exhibits and offer a full complement of learning experiences. Funding from NSF will support design, fabrication and core program development of the Air and Space Gallery. The Gallery will feature four themed areas that explore the depth and breadth of aeronautics and space exploration: Air and Aircraft; Humans and Their Spacecraft; Mission to the Planets; and Stars and Telescopes. Also featured will be a Discovery Room for young learners and their parents, a changing exhibit gallery and educational programs for the public and for schools.
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TEAM MEMBERS: Kenneth Phillips
resource project Exhibitions
COSI Columbus will develop "Speed," a traveling exhibition. "Speed" is a 6,000-square-foot, interactive traveling exhibition introducing visitors to the science of speed. Visitors experience extreme and slow speeds through a variety of interactives. The exhibition emphasizes the role of speed -- that is, the physical phenomenon of changing motion over time -- in governing biological, geological and electronic processes as well as the central role of mathematics as the language of physical science.
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TEAM MEMBERS: Joseph Wisne Wanda Foor
resource project Professional Development, Conferences, and Networks
A regional system of collaborative geoscience interpretation for the Finger Lakes region of New York State will be undertaken. The Museum of the Earth (MOTE) will be the interpretive hub and partnerships with six Finger Lakes State Parks, Cornell University and the Paleontological Institute are in place to provide field sites and geology content information. The integrated interpretive system of signage and related exhibits will be assessed as to reaching the needs of the target audience by way of extensive front end evaluation. The development of the geoscience content and prototyping of the signage will continue throughout the planning period.
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TEAM MEMBERS: Karen Wizevich
resource project Exhibitions
How do we know the distance to a star? How do we know what a star is made of? How do we know how fast an object is moving? These questions are addressed in this 1,488 square foot permanent exhibit which emphasizes astronomical spectroscopy - the detailed analysis of light from astronomical objects. This interactive, bilingual (English/Spanish) exhibit will demonstrate different applications of spectroscopy that provide insight into the universe, and will provide opportunities for students, teachers, parents, and the general public to learn about the universe. Bilingual ancillary materials will be produced: pre- and post-visit materials for school visitors; a "Life at an Observatory" ten-minute orientation/information video to be shown at the visitor center. Target audiences are students in grades K-12, and general visitors.
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TEAM MEMBERS: Sandra Preston
resource project Exhibitions
The Space Science Institute is developing a 5,000 s.f. hands-on traveling exhibitions called MarsQuest that will be the centerpiece of a wide-ranging planetary science education program. The exhibition will feature engaging, aesthetically designed, hands-on displays that offer experiences with science concepts relevant to Mars exploration, and will address the common misconceptions about Mars and its relationship to Earth. The most exciting aspect of the exhibition is its up-to-date connection to the progress and discoveries of 8-10 spacecraft that will be launched by NASA from 1996-2005. The exhibition will be supported by educational programs, including comprehensive teacher workshops, public programs on Mars themes, a 30-minute planetarium show emphasizing exploration and discovery, visits to schools and the dissemination of comprehensive field- tested educational materials developed by Arizona State University, the Planetary Society, NASA, the Pacific Science Center, and others. All educational materials will be aligned with the National Science Education Standards and will be available on the World Wide Web.
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TEAM MEMBERS: Paul Dusenbery
resource project Exhibitions
The Chabot Observatory and Science Center (COSC) in Oakland California will develop and present Bringing the Universe Down to Earth: Demystifying the Process that shapes the Solar System. This exhibition will utilize thirteen interactive works by Ned Kahn, a nationally recognized artist. The exhibition will consist of twenty-six exhibits: two per theme, one for Chabot, and one for the traveling component. The exhibition will be incorporated into the structure and network of COSC. It will invite visitors to draw on their general knowledge of this world by focusing on familiar earthly phenomena, such as volcanoes, whirlwinds, wind storms, avalanches, and to consider them in a broader context. Also, the project will take advantage of Chabot's well developed, online connection with schools and community groups in the area to create new opportunities for individualized inquiry. A direct product of this work will be a series of curricular outlines designed to help teachers make full use of the exhibition. This effort can be used to foster a strong collaboration between the informal and formal science education programs. An important feature of this exhibition is that it will travel to nine sites around the country under the auspices of the Association of Science and Technology Centers (ASTC). It is projected that over one million people at the nine sites will see this traveling exhibition. Educational and marketing materials, as well as workshops materials prepared for the COSC exhibition will accompany the traveling exhibit.
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TEAM MEMBERS: Michael Reynolds Margaret Hauben Ned Kahn
resource project Exhibitions
The Adler Planetarium & Astronomy Museum proposes to develop a 10,395 square foot permanent exhibition. Five major exhibit areas - The Milky Way; Billions and Billions; The Life Cycle of Stars; Properties of Stars; and The Dynamic Galaxy -will orient visitors to the Milky Way, and explore in detail the fascinating objects found within. Each gallery will represent different content areas, but there are several underlying connecting themes. 1. Science does not distract from the appreciation, beauty, and mystery of the Universe, but rather deepens it; 2. The universe is a vast, dynamic, evolving, and fascinating place, where we are always learning about new things; 3. We can organize our picture of the Universe in ways that help us understand its structure, and our place in it; 4. We can begin to understand the Universe through observation and interpretation; 5. Based on the fundamental laws of nature, there are some concepts that will help us to explain the phenomenons of the universe. The Adler's new exhibits and programs will reflect the principles and pedagogy articulated in the new National Science Education Standards. It will also be reflected in the national and local reform efforts such as the Urban Systemic Initiative. The Adler staff will collaborate with the Chicago Systemic Initiative of the Chicago Public Schools. The CSI teachers, parents, and students will be involved the program development and evaluation process through focus groups, working teams, and pilot testing activities on-site at the museum The project Principal Investigator (PI) Dr. Evalyn L. Gates received her Doctorate in Physics from Case Western Reserve University in 1990. Currently, she serves as Chair of the Astronomy Department at the Adler Planetarium and Astronomy Museum. Dr. Gates is a Research Scientist on the faculty in the Department of Astronomy and Astrophysics at The University of Chicago in Chicago, Illinois. In addition to the project team, a broad-based advisory comm ittee will serve as counsel to the project. Serving on the project advisory committee are: Minda Borun; Director of Research and Evaluation, The Franklin Institute Science Museum; Richard G. Kron, Ph.D., Director, Yerkes Observatory and on the faculty at The University of Chicago; Catherine A. Pilachowski, Ph.D., Kitt Peak National Observatory; Phillip M. Sadler, Ed.D. Harvard- Smithsonian Center for Astrophysics; James W. Thuran, Ph. D., The University of Chicago ; Melanie Wojtulewicz, M.A., the Chicago Public Schools; and Fahrad Y. Zadeh, Ph.D. Northwestern University.
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TEAM MEMBERS: Evalyn Gates