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Chemistry, 13.11.2019 06:31 QueenNerdy889
The following equation, derived from newton's version of kepler's third law, allows us to calculate the mass (m) of a central object, in solar masses, from an orbiting object's period (p) in years and semimajor axis (a) in astronomical units: m=a3p2 using this formula with the values you found in parts c and d, what is the approximate mass of the central object? view available hint(s)
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The following equation, derived from newton's version of kepler's third law, allows us to calculate...
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