Page 107 - text book form physics kssm 2020
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Chapter 3
                                                                                                  Gravitation
                    (a) Th  e radius of the orbit of planet Mars can be determined by comparing the orbit of Mars
                        with the orbit of the Earth. What information is needed to determine the radius of the
                        orbit of Mars?
                                                                  11
                    (b) Th  e radius of the orbit of the Earth is 1.50 × 10  m, orbital period of the Earth and Mars
                        is 1.00 year and 1.88 years respectively. Calculate the radius of the orbit of Mars.
                     Solution:

                    (a)  Radius of the orbit of the Earth, orbital period of the Earth and orbital period of Mars.
                    (b)                              Radius of orbit of the Earth, r  = 1.50 × 10  m
                                                                                          11
                         Step                                                  1
                                                     Radius of orbit of Mars = r
                         List the given information  14243 Orbital period of Mars, T  = 1.88 years
                                                                             2
                         in symbols.                 Orbital period of the Earth, T  = 1.00 years
                                                                               1
                                                                           2
                         Step                        T  2  r  3                    SMART
                                                                                   SMART
                         Identify and write down the   14243 T 1 2  =  r 1 3                 INFO
                         formula used.                2    2                             T  2  r  3
                                                                               The equation   1 2  =   1 3  involves
                                                     1.00 2  (1.50 × 10 )                T 2  r 2
                                                                     11 3
                                                          =                    the orbital period of a planet
                                                     1.88 2      r  3
                                                                  2            divided by the orbital period
                         Step                            (1.50 × 10 ) × 1.88 2  of another planet. The same
                                                                  11 3
                                                      3
                         Substitute numerical values   r  =     1.00 2         unit needs to be used for
                                                      2
                         into the formula and       14444244443                both periods.
                                                                   11 3
                         perform the calculations.    2                    2
                                                         3 (1.50 × 10 ) × 1.88
                                                     r  =
                                                                1.00 2
                                                      = 2.28 × 10  m
                                                                 11
                    Example 2
                    Figure 3.31 shows that a research satellite needs to orbit at a height of 380 km to capture clear
                    images of the surface of the Earth. What is the orbital period of the satellite?
                                                                        Moon


                                                                r
                                                                 2
                                                           Earth

                                                                  r
                                                   h               1
                                                    2
                                                                      Satellite 1
                                                           h
                                                            1



                                                       Earth at the centre

                                                         Figure 3.31
                                                            8
                    [Radius of the orbit of the Moon = 3.83 × 10  m, orbital period of the Moon = 655.2 hours]
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                   3.2.3                                                                            101
                   3.2.3
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