I used Newton's version of Kepler's third law to calculate Saturn's mass from orbital characteristics of its moon Titan?

Answer 1

Yes, the equation p2 = a3, where p is a planet's orbital period in years and a is the planet's average distance from the Sun in AU. This equation allows us to calculate the mass of a distance object if we can observe another object orbiting it and measure the orbiting object's orbital period and distance.

Answer 2

Great job! Using Kepler's third law, you can determine Saturn's mass by analyzing the orbital characteristics of its moon Titan. This is a common method in astrophysics to estimate the mass of celestial bodies. Keep up the good work with your astrophysical calculations!