Mathematics, 04.11.2020 17:50 ashtonlauber95

De acuerdo con la tercera ley de movimiento planetario de Kepler, la masa de un planeta es directamente proporcional al cubo de la distancia promedio entre él y un satélite en órbita, pero inversamente proporcional al cuadrado del período orbital del satélite. La Tierra tiene una masa de 75.97×10^24 kg y está a una distancia promedio de 3.84×10^5 km de la Luna, la cual completa una órbita en 27.3 días. Si la Tierra orbita al Sol en 365.3 días y está a una distancia promedio de 1.496×10^8 km, ¿cuál es la masa del Sol?

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De acuerdo con la tercera ley de movimiento planetario de Kepler, la masa de un planeta es directame...