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Pili, Unofre B.; Violanda, Renante R. – Physics Education, 2020
The oscillating atmospheric CO[subscript 2] concentrations at Mauna Loa, on the island of Hawaii, Hawaii, United States of America, are Fourier transformed in order to extract the period of oscillations. Also well-known as the Keeling curve, CO[subscript 2] concentrations (in time series) at Mauna Loa oscillate in direct association with seasonal…
Descriptors: Computer Software, Physics, Science Instruction, Astronomy
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Spathopoulos, Vassilios McInnes – Physics Education, 2020
The ancient Greek astronomers devised ingenious methods for measuring the size and distances of the Earth, Moon and Sun. The concepts were beautifully simple and although in most cases could only yield approximate results, they have the advantage that they can be understood by anyone with a basic mathematical background. The emergence of…
Descriptors: Greek Civilization, Computer Simulation, Astronomy, Computer Software
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Kaltcheva, Nadia; Nenkova, Maia – Physics Education, 2021
Many introductory astronomy courses include concepts related to basic stellar properties. In general, these are concepts that originate from the human perception of starlight. This observational aspect is not easy to incorporate in the classroom. We explore if these concepts could be developed using the built-in data in a planetarium software.…
Descriptors: Teaching Methods, Introductory Courses, Astronomy, Computer Software
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Körber, C.; Hammer, I.; Wynen, J.-L.; Heuer, J.; Müller, C.; Hanhart, C. – Physics Education, 2018
Numerical simulations are playing an increasingly important role in modern science. In this work it is suggested to use a numerical study of the famous perihelion motion of the planet Mercury (one of the prime observables supporting Einsteins general relativity) as a test case to teach numerical simulations to high school students. The paper…
Descriptors: Motion, Physics, Science Instruction, Simulation
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Persson, J. R.; Eriksson, U. – Physics Education, 2016
Students often find astronomy and astrophysics to be most interesting and exciting, but the Universe is difficult to access using only one's eyes or simple equipment available at different educational settings. To open up the Universe and enhance learning astronomy and astrophysics different planetarium software can be used. In this article we…
Descriptors: Science Instruction, Astronomy, Physics, Teaching Methods
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Zinzi, Angelo; Pittori, Carlotta; Tagliamonte, Rosa; Nichelli, Elisa – Physics Education, 2021
Since 2017 the Italian Space Agency (ASI) participates to so-called 'Alternanza Scuola-Lavoro' (i.e. 'school-work synergy') outreach projects promoted by the Italian government, and the ASI Space Science Data Center (SSDC) actively contributes to them, with the primary aim of bringing students closer to space-related activities before choosing…
Descriptors: Physics, Science Instruction, High School Students, Space Sciences
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Vollmer, Michael; Möllmann, Klaus-Peter – Physics Education, 2018
Video analysis with a 30 Hz frame rate is the standard tool in physics education. The development of affordable high-speed-cameras has extended the capabilities of the tool for much smaller time scales to the 1 ms range, using frame rates of typically up to 1000 frames s[superscript -1], allowing us to study transient physics phenomena happening…
Descriptors: Physics, Science Education, Motion, Time
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George, Samuel J. – Physics Education, 2011
The field of extrasolar planets is still, in comparison with other astrophysical topics, in its infancy. There have been about 300 or so extrasolar planets detected and their detection has been accomplished by various different techniques. Here we present a simple laboratory experiment to show how planets are detected using the transit technique.…
Descriptors: Laboratory Experiments, Science Instruction, Astronomy, Science Experiments
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de Moraes, I. G.; Pereira, J. A. M. – Physics Education, 2009
The motion of the four Galilean moons of Jupiter is studied in this work. The moons had their positions with respect to the centre of the planet measured during one week of observation by means of telescopic charge coupled device images. It is shown that their movement can be well described as a simple harmonic motion. The revolution period and…
Descriptors: Astronomy, Motion, Science Activities, Science Education
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Meyn, Jan-Peter – Physics Education, 2008
A digital SLR camera with a standard lens (50 mm focal length, f/1.4) on a fixed tripod is used to obtain photographs of the sky which contain stars up to 8[superscript m] apparent magnitude. The angle of view is large enough to ensure visual identification of the photograph with a large sky region in a stellar map. The resolution is sufficient to…
Descriptors: Photography, Motion, Astronomy, Science Instruction
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Bridges, Richard – Physics Education, 1995
Describes how to fit binocular observations of the planets to a theoretical model of circular orbits using a modern computer spreadsheet, from which fundamental data about the solar system may be deduced. (AIM)
Descriptors: Astronomy, Computer Software, Earth Science, Physics
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Bridges, Richard – Physics Education, 1995
Describes how a spreadsheet is used to fit a circular orbit model to observations of Jupiter's moons made with a small telescope. Kepler's Third Law and the inverse square law of gravity are observed. (AIM)
Descriptors: Astronomy, Computer Software, Earth Science, Physics
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Grafton, Teresa; Suggett, Martin – Physics Education, 1991
Resources that are available for teachers presenting astronomy in the National Curriculum are listed. Included are societies and organizations, resource centers and places to visit, planetaria, telescopes and binoculars, planispheres, star charts, night sky diaries, equipment, audiovisual materials, computer software, books, and magazines. (KR)
Descriptors: Astronomy, Audiovisual Aids, Books, British National Curriculum