The third Kepler’s law of planetary motion states that the square of the orbital period of a planet is proportional to the cube of the semi-major axis (mean distance) of its orbit:
here, "P_M=32\\ years" is the orbital period of Morana, "P_N" is the orbital period of Noveria, "a_M=17\\ AU" is the mean distance of Morana from Pax and "a_N=3.5\\ AU" is the mean distance of Noveria from Pax.
Then, from this equation we can find the length of the Noveria year (or its orbital period):
Answer:
(d) "P_N=2.99\\ years."
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