Answer: The correct answer is Earth's orbital period and distance from the Sun.
Explanation: Rosalinda can use Kepler's Laws to determine the mass of the Earth. Third law of Kepler is the most convenient for this purpose.
Expression for Kepler's Third Law is:

Where,
P = orbital period determined in days
k = Gaussian Gravitational constant with value 0.01720209895
= Mass of the sun which is known to us which is 
= Mass of Earth which has to be determined
a = Semi major axis which is the distance of Earth from the sun.
Hence, Earth's orbital period and its distance from the sun is useful in determining the mass of Earth.