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resource project Media and Technology
First Light is a one-hour documentary to be shown nationally on WGBH-TV's NOVA science series. It tells the extraordinary story behind the building of the Hale Telescope on Palomar Mountain in southern California. The film also documents a research effort at the frontiers of astronomy that has pushed the Hale beyond anything its builders had imagined: The attempt to find and map the edge of the known universe. It follows astronomers Maarten Schmidt, James Gunn and Don Schneider as they search for distant quasars. This team recently detected a quasar that is by far the most distant object yet found in the universe; its discovery may challenge our current understanding of cosmic evolution. The documentary is based on the award winning book First Light: The Search for the Edge of the Universe by Richard Preston. After broadcast, the program will have wide educational distribution in secondary schools and colleges.
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TEAM MEMBERS: Kathleen White
resource project Media and Technology
Eclipse| is a one-hour program within the prime-time series NOVA, to be broadcast nationally during the 1991-92 season on the Public Broadcasting Service (PBS). The program will document the total eclipse of the sun that takes place on July 11, 1991, and the research performed at the observatories located atop Mauna Kea on the Big Island of Hawaii. The program will trace three narrative lines. The first will be that of the eclipse itself and its importance for ongoing scientific investigation of the solar corona and solar physics. The second will be that of ongoing problems in understanding the sun, especially the issue of solar variability. The third will place this eclipse within the history of eclipse science. The passage of an eclipse over a major observatory complex is a unique occurrence -- it has never happened before, and will not happen again for several generations. The four minutes of totality will allow solar astronomers to turn deep space instruments on the sun for the first time. At the same moment, however, this eclipse marks what many observers feel is the end of a 130 year research program. Eclipse| will provide its audience with a portrait of a spectacular natural phenomenon and of scientists attempting in real-time to tease new knowledge out of the sun. In addition to its broadcast, Eclipse| will be seen in an estimated 70-90,000 classrooms over a seven year period.
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TEAM MEMBERS: Paula Apsell Thomas Levenson
resource project Media and Technology
The excitement of astrophysical research and discovery is brought into the high school science and mathematics classes through a flexible set of student activities and projects on variable stars. The project includes a computerized database, of 400,000 measurements of brightness of 150 variable stars in five constellations over 25 years, from which students can deduce properties, processes, and evolution of these stars. Students can make additional measurements and discoveries from carefully selected time sequences of 125 35mm slides or from actual measurements from the night sky. A comprehensive student manual and instructional videos make the materials self-contained and easy to use. The teacher manual enables the instructor to adapt the materials to skills, objectives and local curricula. The material can be used in a variety of contexts: traditional mathematics and science classes at both the high school and college level, independent projects, summer institutes, and community science clubs. The material will be field tested in classes and refined through workshops with teachers. A newsletter and a video about amateur astronomers is planned.
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TEAM MEMBERS: Janet Mattei John Percy
resource project Media and Technology
The Challenger Center for Space Science Education located in Alexandria, Virginia, a nonprofit organization with a mission to increase the number of youth interested in science and space, is requesting $303,170 over two years from the National Science Foundation (NSF) to develop a new scenario for its Challenger Learning Centers. Located in science centers. museums and schools around the country. Learning Centers house equipment and educational programming for hands-on training during a simulated mission. Scenarios use mathematics, science and problem-solving skills to provide participants with simulated experiences of working in a space laboratory and a "Mission control" laboratory. Challenger Center requests assistance and partnership from NSF to develop, field test, implement and evaluate a new scenario on the environment, "Mission to Planet Earth" scenario. This project will involve collaboration of expert scientists, educators, Challenger staff, and science museum professionals. Annually more than 180,000 students and between 10,000 and 15,000 adults will participate in the scenario at Learning Centers, using space as a format for learning about environmental issues. Challenger is working on the preliminary planning stage between June and December 1991. Two years of funding are requested from NSF beginning in January 1992.
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TEAM MEMBERS: Richard Methia
resource project Exhibitions
Lowell Observatory astronomers will collaborate with educators, museum specialists, and planetarium professional to design and implement a unique series of interactive science education exhibits entitled Tools of the Astronomer. The exhibits will capitalize on widespread interest in astronomy to illustrate the research process, demonstrate the theory and function of basic astronomical instruments, and encourage visitors to discover how measurements made with these instruments reveal the properties of celestial objects. Exhibit concepts developed by the Lowell staff will be evaluated by a National Exhibit Advisory Board (NEAB). The original concepts will then be modified to reflect the Board's recommendations, and prototype exhibits will be built. The prototypes will be extensively tested for durability and effectiveness in achieving the educational goals. Students and teachers from Arizona (including those from nearby Navajo and Hopi Indian Reservations), plus members of the general public, will participate in the testing. The NEAB will then review the completed prototypes and test results, and recommend any further modification or testing needed prior to selection of a professional exhibit fabricator to build the final exhibits. The completed exhibits will be installed and further evaluated in a new educational facility to be opened at Lowell Observatory in spring of 1994. There, the exhibits will be experienced by tens of thousands of people who visit Lowell Observatory each year. A significant fraction of these visitors will be school children who will participate in instructional programs designed around the exhibits. The exhibits also will ultimately be used in teacher workshops. To achieve maximum impact, all software, exhibit designs, teacher's guides, and other material developed in this project will be marketed to schools, science centers, planetaria, observatories, and other educational entities at the cost of reproduction.
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TEAM MEMBERS: Robert Millis William Buckingham
resource project Exhibitions
Ohio's Center of Science and Industry (COSI) in Columbus, Ohio, in association with the Pacific Science Center in Seattle, WA. and the Battelle Memorial Institute will create and circulate a 4,000 square foot traveling exhibition, "Mission to Mars." Interactive exhibit units will be organized into a spacecraft mission simulator. Visitors in teams will run a scientific mission to the planet Mars. Exhibits and simulation activities will cover basic and applied science and mathematics topics appropriate for middle to high school students and family audiences. Educational materials for school use will accompany the exhibition. COSI has a strong reputation for interactive science exhibitions. Their widely acclaimed "Science of Sports" exhibition will be seen in more than 15 cities. The Pacific Science Center has a similar reputation for educational exhibitions and related materials development. Their educational materials on dinosaurs have been widely used by other museums. The Battelle Memorial Institute is a world- renowned research and applied science organization. "Mission to Mars" is supported by commitments from thirteen of America's leading science museums and a major award from Apple Computer Company. The project team will deliver a timely exhibition that will be both engaging and challenging, rich with scientific detail while still appealing to family audiences. "Mission to Mars" will travel to 13 cities on a three year tour, reaching an estimated three to five million people. NSF's 43% of the project cost will be leveraged by more than $878,000 in contributions from the originating institutions, from the displaying museums and from Apple.
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TEAM MEMBERS: Charles O'Connor Joseph Wisne Michael Stanley
resource project Public Programs
The Thames Science Center collaborative with the resources of the Smithsonian Astrophysical Observatory, Wesleyan University and the National Air and Space Museum will design and develop the project, "Shoot For the Moon." This science education project will capitalize on the attraction, familiarity and proximity of the moon using it as a basis to enrich and supplement the eight and ninth grade physical science curriculum. Ten classroom units, complimentary experiments and demonstrations will be developed. "Moonwatch" software and audio visual materials, including an instructional videotape and a multi.image presentation will accompany the units. Sixteen teachers and museum educators will participate in the training, evaluation and testing as the project is integratedinto the curriculum of twelve schools and four museums. The project is designed to be replicated in schools and science centers in different geographical locations nationally. The site for development and testing will be the Thames Science Center, a regional science museum in eastern Connecticut. The science center offers formal science enrichment programs and tours for students and teacher professional development programs throughout the region.
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TEAM MEMBERS: Jane Holdsworth William Gill