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To find the mass of Earth using Kepler's laws or Newton's universal law of gravitation, Rosalinda should consider Earth's distance from the Sun and the moon's orbital period.
Earth's distance from the Sun and the moon's orbital period would allow Rosalinda to find the mass of Earth through Kepler's laws or Newton's universal law of gravitation. This is because the square of the period is proportional to the cube of the distance between Earth and the Moon, a key relationship in these calculations.
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