Page 35 - Geography for Secondary Schools Student’s Book Form One
P. 35

Geography for Secondary Schools
                                                                          Student’s Book Form One

            Exercise 3.4

            1.     Discuss the effects of the earth’s revolution in your area.
            2.     Explain the common economic activities carried out in your area in different
                 seasons of the year.

           FOR ONLINE READING ONLY
                  Activity 3.6
             1.     Think of your community at home town or village, and relate the seasons of the
                  year with their daily activities. Use the following questions for guidance:
                     (a)   What activities do they conduct in each season?
                     (b)   Why do you think they do such activities in that particular season?

             2.     Write short essay on the activities done in relation to the seasons of the year.


            (iv)    Aphelion and Perihelion
            The Earth revolves around the sun in an elliptical orbit. Due to the elliptical shape of
            the earth’s orbit, the Sun is closer to the Earth at one point of the year than at the other
            (Figure 3.7). The furthest position from the sun in the orbit of the earth is called aphelion.
            Normally, the Earth is at aphelion each year on 4  July when it is 152 million kilometres
                                                          th
            away from the Sun. Perihelion occurs when the Earth is nearest to the Sun about 147
            million kilometres away from the Sun. The Earth is at perihelion each year on the 3
                                                                                              rd
            of January. Aphelion and perihelion affect the amount of solar radiation received by
            the Earth, though their influence on the seasons is much smaller than the axial tilt. The
            slight variation in solar radiation due to Earth’s changing distance from the Sun during
            its orbit is not sufficient to cause significant climate change or shifts in seasons.




























                                    Figure 3.7: Perihelion and aphelion


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