Johannes Kepler: TheLaws of Planetary Motion
Observe the motion of Jupiter’s moons over several days (movie) Estimate the orbiting period (T) of Moon I or II . T = Estimate the mean radius (r) of the moon’s orbit by comparing it to the diameter of Jupiter (142984 km) r = Solve for the mass of Jupiter using Kepler’s 3rd law (use consistent units!) ................
................
To fulfill the demand for quickly locating and searching documents.
It is intelligent file search solution for home and business.