2.0 Moons of Jupiter 1.0 Moons of Saturm 05 04 06 0.8 1.0 12 1.4 1.6 The diagram shows two graphs of R'against T; one is for the moons of Jupiter and the other is for the moons of Saturn. R is the mean distance of a moon from a planet's centre and Tis its period. The orbits are assumed to be circular. The mass of Jupiter is 1.90 x 10" kg. (a) Why are the lines straight? (b) Find a value for the mass of Saturn

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Chapter1: Units, Trigonometry. And Vectors
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2.0
Moons of Jupiter
E 1.5
E 1.0
Moons of Satum
05
0.2
0.4
0.6
0.8
1.0
1.2
1.4
1.6
T10"s
The diagram shows two graphs of R' against
T; one is for the moons of Jupiter and the
other is for the moons of Saturn. R is the
mean distance of a moon from a planet's
centre and Tis its period.
The orbits are assumed to be circular.
The mass of Jupiter is 1.90 x 102" kg.
(a) Why are the lines straight?
(b) Find a value for the mass of Saturn.
(c) Find a value for the universal gravita-
tional constant G.
[L*)
Transcribed Image Text:2.0 Moons of Jupiter E 1.5 E 1.0 Moons of Satum 05 0.2 0.4 0.6 0.8 1.0 1.2 1.4 1.6 T10"s The diagram shows two graphs of R' against T; one is for the moons of Jupiter and the other is for the moons of Saturn. R is the mean distance of a moon from a planet's centre and Tis its period. The orbits are assumed to be circular. The mass of Jupiter is 1.90 x 102" kg. (a) Why are the lines straight? (b) Find a value for the mass of Saturn. (c) Find a value for the universal gravita- tional constant G. [L*)
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