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Autor/inOostra, Benjamin
TitelIntroducing the Moon's Orbital Eccentricity
QuelleIn: Physics Teacher, 52 (2014) 8, S.460-463 (4 Seiten)Infoseite zur Zeitschrift
PDF als Volltext Verfügbarkeit 
Spracheenglisch
Dokumenttypgedruckt; online; Zeitschriftenaufsatz
ISSN0031-921X
DOI10.1119/1.4897579
SchlagwörterAstronomy; Science Instruction; Secondary School Science; High Schools; College Science; Algebra; Trigonometry; Physics; Motion; Introductory Courses; Teaching Methods
AbstractI present a novel way to introduce the lunar orbital eccentricity in introductory astronomy courses. The Moon is perhaps the clearest illustration of the general orbital elements such as inclination, ascending node, eccentricity, perigee, and so on. Furthermore, I like the students to discover astronomical phenomena for themselves, by means of a guided exercise, rather than just telling them the facts. The inclination and nodes may be found by direct observation, monitoring carefully the position of the Moon among the stars. Even the regression of the nodes may be discovered in this way. To find the eccentricity from students' observations is also possible, but that requires considerable time and effort. if a whole class should discover it in a short time, here is a method more suitable for a one-day class or home assignment. The level I aim at is, more or less, advanced high school or first-year college students. I assume them to be acquainted with celestial coordinates and the lunar phases, and to be able to use algebra and trigonometry. (As Provided).
AnmerkungenAmerican Association of Physics Teachers. One Physics Ellipse, College Park, MD 20740. Tel: 301-209-3300; Fax: 301-209-0845; e-mail: pubs@aapt.org; Web site: http://scitation.aip.org/tpt
Erfasst vonERIC (Education Resources Information Center), Washington, DC
Update2017/4/10
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