(a) Explanation Given: R=422×10 3 km T 1 =1 .77 Earth days Formula Used: FromKepler’s third law of planetary motion: M J = 4 π 2 R 3 G . T 2 Where, R -Mean distance from Jupiter, T -periodof revolution. G=6 .67×10 11 Nm 2 /kg 2 (G is gravitational constant) T=(1 (b) To determine The mass of the Jupiter using the data of other three moons i.e. Europa, Ganymede and Calisto and find if all the resultants are consistent.

Physics: Principles and Applications -- Pearson e Text Instant Access (Pearson+)

7th Edition

ISBN: 9780137679065

Author: Douglas Giancoli

Publisher: PEARSON+

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Chapter 5, Problem 62P

(a)

To determine

The mass of the Jupiter using the given IO.

(b)

To determine

The mass of the Jupiter using the data of other three moons i.e. Europa, Ganymede and Calisto and find if all the resultants are consistent.

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Chapter 5, Problem 61P

Chapter 5, Problem 63P

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