The American Museum of Natural History (AMNH), in collaboration with New York University's Institute for Education and Social Policy and the University of Southern Maine Center for Evaluation and Policy, will develop and evaluate a new teacher education program model to prepare science teachers through a partnership between a world class science museum and high need schools in metropolitan New York City (NYC). This innovative pilot residency model was approved by the New York State (NYS) Board of Regents as part of the state’s Race To The Top award. The program will prepare a total of 50 candidates in two cohorts (2012 and 2013) to earn a Board of Regents-awarded Masters of Arts in Teaching (MAT) degree with a specialization in Earth Science for grades 7-12. The program focuses on Earth Science both because it is one of the greatest areas of science teacher shortages in urban areas and because AMNH has the ability to leverage the required scientific and educational resources in Earth Science and allied disciplines, including paleontology and astrophysics.
The proposed 15-month, 36-credit residency program is followed by two additional years of mentoring for new teachers. In addition to a full academic year of residency in high-needs public schools, teacher candidates will undertake two AMNH-based clinical summer residencies; a Museum Teaching Residency prior to entering their host schools, and a Museum Science Residency prior to entering the teaching profession. All courses will be taught by teams of doctoral-level educators and scientists.
The project’s research and evaluation components will examine the factors and outcomes of a program offered through a science museum working with the formal teacher preparation system in high need schools. Formative and summative evaluations will document all aspects of the program. In light of the NYS requirement that the pilot program be implemented in high-need, low-performing schools, this project has the potential to engage, motivate and improve the Earth Science achievement and interest in STEM careers of thousands of students from traditionally underrepresented populations including English language learners, special education students, and racial minority groups. In addition, this project will gather meaningful data on the role science museums can play in preparing well-qualified Earth Science teachers. The research component will examine the impact of this new teacher preparation model on student achievement in metropolitan NYC schools. More specifically, this project asks, "How do Earth Science students taught by first year AMNH MAT Earth Science teachers perform academically in comparison with students taught by first year Earth Science teachers not prepared in the AMNH program?.”
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TEAM MEMBERS:
Maritza MacdonaldMeryle WeinsteinRosamond KinzlerMordecai-Mark Mac LowEdmond MathezDavid Silvernail
This award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5).
Scientists and researchers from fields as diverse as oceanography and ecology, astronomy and classical studies face a common challenge. As computer power and technology improve, the sizes of data sets available to us increase rapidly. The goal of this project is to develop a new methodology for using citizen science to unlock the knowledge discovery potential of modern, large data sets. For example, in a previous project Galaxy Zoo, citizen scientists have already made major contributions, lending their eyes, their pattern recognition skills and their brains to address research questions that need human input, and in so doing, have become part of the computing process. The current Galaxy Zoo project has recruited more than 200,000 participants who have provided more than 100 million classifications of galaxies from the Sloan Digital Sky Survey. This project builds upon early successes to develop a mode of citizen science participation which involves not only simple "clickwork" tasks, but also involves participants in more advanced modes of scientific thought. As part of the project, a symbiotic relationship with machine learning tools and algorithms will be developed, so that results from citizen scientists provide a rich training set for improving algorithms that in turn inform citizen science modes of participation. The first phase of the project will be to develop a portfolio of pilot projects from astrophysics, planetary science, zoology, and classical studies. The second phase of the project will be to develop a framework - called the Zooniverse - to facilitate citizen scientists. In particular, research and machine-learning communities will be engaged to identify suitable projects and data sets to integrate into Zooniverse.
The ultimate goal with the Zooniverse is to create a sustainable future for large-scale, internet-based citizen science as part of every researcher?s toolkit, exemplifying a new paradigm in computational thinking, tapping the mental resources of a community of lay people in an innovative and complex manner that promises a profound impact on our ability to generate new knowledge. The project will engage thousands of citizens in authentic science tasks leading to a better public understanding of science and also, by the engagement of students, leading to interest in scientific careers.
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TEAM MEMBERS:
Geza GyukPamela GayChristopher LintottMichael RaddickLucy FortsonJohn Wallin
The Space Science Institute is developing an astronomy educational social game for the Facebook platform. The game uses the "sporadic play" model popular with many Facebook games, in which players take only a few actions at a time, then return to explore the results. Here players will create their own stars and planetary systems that evolve over time at a rate of a million years a minute. Players set systems in motion, revisiting the game over days or weeks to make new choices and alter strategies. The game is in effect an end-to-end solar system simulation, following a star from birth to death. As a result it encompasses a wide variety of core concepts in astronomy, including galactic structure, stellar evolution and lifecycles, planetary formation and evolution, and habitability and "habitable zones." The accompanying research program will examine the effectiveness of this type of game in informal education, and the effects of the social network on meeting the education goals, including viral spread, cooperative play, and discussions about the game and its underlying content in associated online forums.
The Adler Planetarium, Johns Hopkins University, and Southern Illinois University-Edwardsville are investigating the potential of online citizen science projects to broaden the pool of volunteers who participate in analysis and investigation of digital data and to deepen volunteers' engagement in scientific inquiry. The Investigating Audience Engagement with Citizen Science project is administering surveys and conducting case studies to identify factors that lead volunteers to engage in the astronomy-focused Galaxy Zoo project and its Zooniverse extensions. The project is (1) identifying volunteers' motivations for joining and staying involved, (2) determining factors that influence volunteers' movement from lower to higher levels of involvement, and (3) designing features that influence volunteer involvement. The project's research findings will help informal science educators and scientists refine existing citizen science programs and develop new ones that maximize volunteer engagement, improve the user experience, and build a more scientifically literate public.
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TEAM MEMBERS:
Karen CarneyMichael RaddickPamela Gay
The Liz Lerman Dance Exchange, in partnership with several universities and a science advisory committee of distinguished international researchers in physics and astronomy, is producing "The Matter of Origins," a two-part experimental program that engages the public in explorations of the nature of beginnings and the physics of the origin of matter. Act I takes place in a theater where audiences will experience a dance performance illuminated by video and a vivid soundscape. Act II takes place in an adjacent space where audiences, who will be seated with scientists, historians, philosophers, and religious leaders, can participate in facilitated dialogue about the nature of origins in an immersive environment that incorporates dance, projected images, and provocative questions. The program will be implemented around the country, initially at four universities, with possible expansion to additional venues. The goals of this EAGER project are (1) to develop an innovative model for using dance, digital media, and structured dialogue to attract and engage public audiences in science content and processes and (2) to explore how artistic practices may have broader applications with respect to science learning and research. The intention is to explore how science can be represented in the art and in the experience and not simply interpreted into abstract choreographic expression with a program note. The program elements and outcomes will be evaluated by researchers from Michigan State University who will study impacts on the public and on participating professionals - dancers, scientists, etc. Dissemination of results will be to professional communities in the sciences, arts and informal science education.
The Rochester Institute of Technology's National Technical Institute for the Deaf (NTID) and Center for Computational Relativity and Gravitation (CCRG) will collaborate on a CRPA project designed to develop a dance-based performance to educate deaf and hard of hearing students on astrophysics concepts. This project seeks to address the following goals: 1) provide all audience members with access to scientific information in an inherently engaging and stimulating manner; 2) facilitate the acquisition of scientific knowledge in all audience members, including deaf and hard-of-hearing individuals, with special reference to general information and basic concepts from the fields of gravitational physics and astrophysics; and 3) stimulate general interest in STEM fields within all audience members. An extensive team of physicists, arts faculty, computer scientists, performance experts, and evaluators have assembled to translate original research on gravity-based astrophysics, including collision events between black-holes and neutron-stars, entire galaxies, and the central black-hole engine that powers active galactic nuclei, into novel educational presentations. The original science to be presented was generated in part by the scientists at the Center for Computational Relativity and Gravitation. Project deliverables include live performances and a project website with educational materials and a virtual tour of the recorded performance. The live performances will include dance and computer generated visualizations of space phenomena, supplemented with discussion and interactive components to engage audiences both before and after the presentation. The mixed-method evaluation will provide insights into how the medium of dance can be used to engage audiences in STEM fields and increase the understanding of STEM content areas which have had little previous investigation, but may be highly relevant to the engagement of underserved audiences. Performances are planned for select sites in New York, Ohio, Connecticut, Rhode Island, Washington, DC, Pennsylvania and Maryland. It is estimated that the project will directly impact 7,000 individuals, approximately half of whom will be deaf or hard or hearing. Deaf and hard of hearing populations are greatly underserved in science education. This project is an effort to bridge that gap by providing creative models for communicating to the public on contemporary science concepts. Learning outcomes for the target audience include increasing awareness and interest in STEM, acquisition of information and basic concepts from the fields of gravitational physics and astrophysics, and enhancing awareness of relationships among science and the arts. Project activities will be disseminated through the website hosted by the Rochester Institute of Technology, as well as social networking sites including Facebook, Twitter, and Google+. The project will also be promoted through science festivals and media events.
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TEAM MEMBERS:
Manuela CampanelliHans-Peter BischofJacob Noel-Storr
StarTalk Radio will develop a highly innovative new genre of science radio that bridges the intersection between popular culture and science education. Host of the show and project PI is Dr. Neil deGrasse Tyson, renowned scientist, astrophysicist, popular science author and director of the Hayden Planetarium in New York City. The radio programs will combine comedy, references to pop culture, and public fascination with space science to reach an untapped audience for the informal science field--those who listen to commercial talk radio call-in shows. The STEM content will include astronomy, astrophysics, astrobiology, space exploration, earth system science, and associated technologies. Goals and intended outcomes of the project include increasing knowledge and interest of space science topics, and motivating audiences to pursue additional learning acitivities as the result of listening to the programs. This project builds on a previous SGER grant (#0852400) which produced 13 pilot programs and was evaluated by Multimedia Research. Project deliverables include 39 one-hour live call-in shows a year for a total of 117 shows over three years, a website, and a business strategy that projects making the radio programs self-sustaining. Dr. Tyson will be the host, and each program will include a celebrity guest who has a strong interest in science. The target audience for the show is the "blue collar intellectual" audience segment who listens to commercial talk radio, has a high school education or less and is in the 25-44 year old range. It is estimated that there will be one million listeners per week by the end of the project. People with disabilities (deaf and visually impaired) will have access to the products through captioning and other features on the website. Project partners include CBS Radio, CBS/AOL, and Discover Magazine. Formative evaluation of these new shows and website will be conducted by Multimedia Research. The Goodman Research Group (GRG) will conduct the summative evluation to assess the extent to which the project accomplishes the goals and specifically will gather and analyze data on the previously untappped and underserved audiences. The evaluation will examine the differences in impact on Science Novices and Science Enthusiasts, asking questions about how the programs increase awareness of scientific issues, and their effects on society and culture, as well as factual knowledge. Methods include multi-level, quasi-experimental, and longitudinal episode assessments. Potential impacts on the field of informal science education include opening up a new commercial radio audience for informal science learning, increasing knowledge about effective approaches to combining humor and science, and demonstrating an effective business model that results in a self-supporting show about science on commercial radio.
The 2009 International Year of Astronomy coincides with the dimming and brightening of a variable star that can be seen with the naked eye. The American Association of Variable Star Observers and the Adler Planetarium and Astronomy Museum are organizing a new citizen program called STARS (Science Through Astronomical Research) that engages 8,000 amateur astronomers and non-astronomers in measuring brightness changes in the star Epsilon Aurigae, analyzing their observational data, and developing and testing their own explanatory hypotheses. The goals of the project are to increase public understanding of science by involving citizens in active research on an accessible, yet enigmatic astronomical phenomenon, and disseminate lessons learned to other citizen science programs. A mixed methods evaluation study is monitoring the implementation and impact of the program. The project should (1) increase the number of non-astronomers who take up astronomy as a hobby, (2) increase the number of amateur astronomers who participate in other citizen science-related astronomical activities (for example, sky surveys), and (3) increase the number of non-science oriented citizens who become more interested in science. A research study is investigating how a large-scale informal citizen science project changes public understanding of scientific inquiry.
The Astronomical Society of the Pacific, in collaboration with the Institute for Learning Innovation, will implement "Sharing the Universe." This research and implementation project is designed to include both a comprehensive, two-phased research component, as well as a large-scale national dissemination. The intended impacts are to improve the quality and effectiveness of informal science education activities provided by amateur astronomers; increase the frequency of public engagements in astronomy; and broaden the variety of events and diversity of the outreach to include underserved and underrepresented audiences. The project will create a community of practice using club leaders to improve astronomy clubs nationwide through research tools, training and outreach skills. Project deliverables include Phase I research which is designed to gain an understanding of how outreach-orientated clubs function and identify strategies that make successful clubs effective. Phase II will examine a core group of 20 clubs in detail to further understand the outreach culture while using interventions developed from the Phase I results such as a training DVD, Online Resource Library, Outreach Toolkit and a robust community of practice. The final deliverable will be the dissemination of proven strategies and best practices revealed by the research to 200 diverse astronomy clubs across the country. Strategic impact will be realized in increased outreach capacity among amateur astronomers and a strong model for astronomy clubs with proven best practices and resources. It is anticipated this project will reach more than 4,400 amateur astronomers and indirectly impact more than one million Americans in astronomy clubs in four years. Inverness Research will conduct the summative evaluation of the project.
Researchers at the American Association of Variable Star Observers, the Living Laboratory at the Boston Museum of Science, and the Adler Planetarium are studying stereoscopic (three-dimensional or 3D) visualizations so that this emerging viewing technology has an empirical basis upon which educators can build more effective informal learning experiences that promote learning and interest in science by the public. The project's research questions are: How do viewers perceive 3D visualizations compared to 2D visualizations? What do viewers learn about highly spatial scientific concepts embedded in 3D compared to 2D visualizations? How are viewers\' perceptions and learning associated with individual characteristics such as age, gender, and spatial cognition ability? Project personnel are conducting randomized, experimental mixed-methods research studies on 400 children and 1,000 adults in museum settings to compare their cognitive processing and learning after viewing two-dimensional and three-dimensional static and dynamic images of astronomical objects such as colliding galaxies. An independent evaluator is (1) collecting data on museum workers' and visitors' perceived value of 3D viewing technology within museums and planetariums and (2) establishing a preliminary collection of best practices for using 3D viewing technology based on input from museum staff and visitors, and technology creators. Spatial thinking is important for learning many domains of science. The findings produced by the Two Eyes, 3D project will researchers' understanding about the advantages and disadvantages of using stereoscopic technology to promote learning of highly spatial science concepts. The findings will help educators teach science in stereoscopic ways that mitigate problems associated with using traditional 2D materials for teaching spatial concepts and processes in a variety of educational settings and science content areas, including astronomy.
The National Science Festival Network project, also operating as the Science Festival Alliance, is designed to create a sustainable national network of science festivals that engages all facets of the general public in science learning. Science Festivals, clearly distinct from "science fairs", are community-wide activities engaging professional scientists and informal and K-12 educators targeting underrepresented segments of local communities historically underserved by formal or informal STEM educational activities. The initiative builds on previous work in other parts of the world (e.g. Europe, Australasia) and on recent efforts in the U.S. to create science festivals. The target audiences are families, children and youth ages 5-18, adults, professional scientists and educators in K-12 and informal science institutions, and underserved and underrepresented communities. Project partners include the MIT Museum in Cambridge, UC San Diego, UC San Francisco, and the Franklin Institute in Philadelphia. The deliverables include annual science festivals in these four cities supported by year-round related activities for K-12 and informal audiences, a partnership network, a web portal, and two national conferences. Ten science festivals will be convened in total over the 3 years of the project, each reaching 15,000 to 60,000 participants per year. STEM content includes earth and space science, oceanography, biological/biomedical science, bioinformatics, and computer, behavioral, aeronautical, nanotechnology, environmental, and nuclear science. An independent evaluator will systematically assess audience participation and perceptions, level/types of science interest stimulated in target groups, growth of partnering support at individual sites, and increasing interactions between ISE and formal K-12 education. A variety of qualitative and quantitative assessments will be designed and utilized. The project has the potential to transform public communication and understanding of science and increase the numbers of youth interested in pursuing science.
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TEAM MEMBERS:
Loren ThompsonJeremy BabendureBen Wiehe
The Space Science Institute, in collaboration with the Catawba Science Center (North Carolina), the New Mexico Museum of Natural History and Science, the American Library Association, and the Astronomical Society of the Pacific propose to develop a multi-pronged project on the topic of asteroids. Content areas will include: Asteroids ? Up-close and Personal; Deep Impact; and Planetary Protection. Deliverables will include a 2,500 square-foot traveling exhibit for small to mid-sized museums; four, 300 square-foot "small exhibit components" (SECs) for libraries, community centers, etc.; Web 2.0 sites for the project developers and for the public; public education programs; professional development programs for informal STEM professionals; and a study of how Web 2.0 can be used to improve the evaluation of Web sites. The project team will be experimenting with virtual prototyping of exhibit modules as a way to improve exhibit development, especially with team members who are around the country. Teens from around the country will be enlisted to help inform the project on its deliverables. The Association of Science-Technology Centers will manage the exhibit tour. The Institute for Learning Innovation will conduct the evaluation activities, including the study of Web 2.0 and virtual prototyping tasks.