- Moon Lo Date And Time Of Eastern Elongation 10 24 13 4 00 00 10 25 13 19 00 00 Europa Ganymede 10 23 13 20 00 00 Callist 1 (32.81 KiB) Viewed 38 times
- Moon Lo Date And Time Of Eastern Elongation 10 24 13 4 00 00 10 25 13 19 00 00 Europa Ganymede 10 23 13 20 00 00 Callist 2 (92.33 KiB) Viewed 38 times
- Moon Lo Date And Time Of Eastern Elongation 10 24 13 4 00 00 10 25 13 19 00 00 Europa Ganymede 10 23 13 20 00 00 Callist 3 (55.46 KiB) Viewed 38 times
Moon lo Europa Ganymede Callisto Largest angular separation in decimal degrees 0.0327 0.052 0.07805 Part 4- The Mass of Jupiter 36. In Parts 2 and 3, you determined the values for the Orbital Period and Orbital Radius of the moons of Jupiter. Now we will solve for the mass of Jupiter. 0.483 7² = (2) 37. The value of 4²/G is 5.915 x 10" kgs-/m². Substituting this value and rearranging the equation will provide Moon M = (5.915 x 10¹¹ kgs /m²) = 38. What is the mass of Jupiter using the values from lo's orbit? (Show all steps of your calculation) lo Semi-major axis in meters 39. From the answer in 38, calculate the percent error in our result for Jupiter's mass. The accepted value of Jupter is 1.9 x 10 kg (Show all steps of your calculation % Error = 40 Complete the table for the remaining moons. Mass of Jupiter in kg Europa 4.17 10'8 6.62*10^8 9.94*10^8 6.15*10^9 Ganymede M-19x10x100 19x10 kg % Error
2 4π 3 = (GM),²³ r of 4² / G is 5.915 x 10¹1 kgs²/m³. Substitut anging the equation will provide 2 M = (5.915 x 10¹1¹kgs²/m³) T² e mass of Jupiter using the values from lo's of your calculation) % Error = answer in 38, calculate the percent error in mass. The accepted value of Jupter is 1.9 x of your calculation) M - 1.9 x 10²7 kg 3 r (kg) 27 1.9 x 10 kg x 100