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ee Figure 3 for an illustration of choosing the appropriate locations to measure for determining e period (indicated by red circles for Ganymede). As an example we will measure the period I lo. From the figure we determine there are 23 days between selected times (shown with white uares). There are 13 orbits (periods) executed during this time so 23 days/13 orbits gives 1.77 ays per orbit, or a period of 1.77 days. Convert this to seconds, and put your answer here: period (P) = seconds

ee Figure 3 for an illustration of choosing the appropriate locations to measure for determining e period (indicated by red circles for Ganymede). As an example we will measure the period I lo. From the figure we determine there are 23 days between selected times (shown with white uares). There are 13 orbits (periods) executed during this time so 23 days/13 orbits gives 1.77 ays per orbit, or a period of 1.77 days. Convert this to seconds, and put your answer here: period (P) = seconds

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Ganymede (red circle). Also shown are some of the beginning and ending of orbits for lo (whit Figure 3. Image shows some of the locations to measure the beginning or ending of an orbit for Ca G C July 1 21 WEST EAST 3. 8. to 10 Europa 11 Ganymede 12 13 14 15 16 Callisto 17 18 19 20 21 22 23 24 25 26 or square).
Transcribed Image Text:Ganymede (red circle). Also shown are some of the beginning and ending of orbits for lo (whit Figure 3. Image shows some of the locations to measure the beginning or ending of an orbit for Ca G C July 1 21 WEST EAST 3. 8. to 10 Europa 11 Ganymede 12 13 14 15 16 Callisto 17 18 19 20 21 22 23 24 25 26 or square).
See Figure 3 for an illustration of choosing the appropriate locations to measure for determining the period (indicated by red circles for Ganymede). As an example we will measure the periou or lo. From the figure we determine there are 23 days between selected times (shown with white squares). There are 13 orbits (periods) executed during this time so 23 days/13 orbits gives I.7! days per orbit, or a period of 1.77 days. 7. Convert this to seconds, and put your answer here: period (P) = %3D seconds Now we can apply Kepler's third law to determine the mass of Jupiter (M) 47 R3 (1) %3D GP2 Use this formula, find the mass of Jupiter (M), and write your answer here: (MJupiler) = kg Using the same method, astronomers have determined the mass of the Earth to be 5.95 x your 9. 1024 kg. How many times more massive is Jupiter than the Earth, according to calculations? 01 10. Jupiter's mass is really about 318 times that of Earth. What are some possible sources of error in your measurement? zelRƏ vaW yilliM orli lo ezsM sdT 8.
Transcribed Image Text:See Figure 3 for an illustration of choosing the appropriate locations to measure for determining the period (indicated by red circles for Ganymede). As an example we will measure the periou or lo. From the figure we determine there are 23 days between selected times (shown with white squares). There are 13 orbits (periods) executed during this time so 23 days/13 orbits gives I.7! days per orbit, or a period of 1.77 days. 7. Convert this to seconds, and put your answer here: period (P) = %3D seconds Now we can apply Kepler's third law to determine the mass of Jupiter (M) 47 R3 (1) %3D GP2 Use this formula, find the mass of Jupiter (M), and write your answer here: (MJupiler) = kg Using the same method, astronomers have determined the mass of the Earth to be 5.95 x your 9. 1024 kg. How many times more massive is Jupiter than the Earth, according to calculations? 01 10. Jupiter's mass is really about 318 times that of Earth. What are some possible sources of error in your measurement? zelRƏ vaW yilliM orli lo ezsM sdT 8.
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