Report - La Tierra en el Universo: Leyes de Kepler - PiCasaTeniendo en cuenta la tercera ley de Kepler: T2 R3 = K (1a˜noterrestre )2 R3 = T2 J (5,2 ·R)3 ⇒ 1 R3 = 2 J (5,2 ·R)3 simplificando

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