dc.contributorUniversidade Estadual Paulista (UNESP)
dc.creatorLewin, Walter
dc.date2016-10-26T18:04:40Z
dc.date2016-10-26T18:04:40Z
dc.date.accessioned2017-04-06T12:48:19Z
dc.date.available2017-04-06T12:48:19Z
dc.identifierhttp://acervodigital.unesp.br/handle/unesp/368953
dc.identifierhttp://objetoseducacionais2.mec.gov.br/handle/mec/14111
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/965235
dc.descriptionConservation of mechanical energy, circular motion
dc.descriptionEducação Superior::Ciências Exatas e da Terra::Física
dc.descriptionKepler's three Laws summarize the motion of the planets in our solar system. Following Newton's law of universal gravitation, the conservation of angular momentum and mechanical energy allow us to calculate the semimajor axis of the elliptical orbits, the orbital period and other orbital parameters. All we have to know is one position and the associated velocity of a planet and the entire orbit follows
dc.publisherMIT OpenCourseWare – Massachussetts Institute of Technology
dc.relation22.WMV
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dc.subjectEducação Superior::Ciências Exatas e da Terra::Física::Física Geral
dc.subjectElliptical orbits
dc.subjectKepler’s laws
dc.titleKepler’s law, elliptical orbits, satellites, change of orbits, ham sandwich
dc.typeVideos


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