LOM v1.0atomicLOM v1.01URLhttp://portal.discoverthecosmos.eu/node/192360enStudents use a series of 31 images of Jupiter’s 4 Galilean moons to find their orbit periods and orbit radii. They compare their results with known data for those moons. Finally they test various mathematical expressions to find a “constant” relationship between orbit period (T) and orbit radius (R) to arrive at Kepler ’s 3rd Law.jupiter moonsorbit keplerLOM v1.0final1.0LOM v1.0author2013-04-02University of California at BerkeleyLOM v1.0publisher2013-04-02Rosa DoranenLOM v1.0LOM v1.0creator2013-04-02Rosa DoranLOM v1.0validatorLOM v1.0browserLOM v1.0anyLOM v1.0osLOM v1.0anytext/htmlhttp://portal.discoverthecosmos.eu/node/192360LOM v1.0noLOM v1.0noLOM v1.0activeLOM v1.0mediumLOM v1.0very easyLOM v1.0Guided ResearchLOM v1.02 didactic hours12-1515-18LOM v1.0DisciplineScienceAstronomy: PlanetsAstronomy: Rotation curve