Page 173 - NCERT Science Class 10 English Medium
P. 173

10.5   ATMOSPHERIC REFRACTION

                                            You might have observed the apparent random wavering or
                                            flickering of objects seen through a turbulent stream of hot air
                                            rising above a fire or a radiator. The air just above the fire becomes
                                            hotter than the air further up. The hotter air is lighter (less dense)
                                            than the cooler air above it, and has a refractive index slightly
                                            less than that of the cooler air. Since the physical conditions of
                                            the refracting medium (air) are not stationary, the apparent
                                            position of the object, as seen through the hot air, fluctuates.
                                            This wavering is thus an effect of atmospheric refraction (refraction
                                            of light by the earth’s atmosphere) on a small scale in our local
              Figure
              Figure  10.9
              Figure 10.910.9
              Figure 10.9
              Figure 10.9
              Apparent star position        environment. The twinkling of stars is a similar phenomenon on
                                            a much larger scale. Let us see how we can explain it.
              due to atmospheric
              refraction
                                     Twinkling of stars
                                     The twinkling of a star is due to atmospheric refraction of starlight. The
                                     starlight, on entering the earth’s atmosphere, undergoes refraction
                                     continuously before it reaches the earth. The atmospheric refraction
                                     occurs in a medium of gradually changing refractive index. Since the
                                     atmosphere bends starlight towards the normal, the apparent position
                                     of the star is slightly different from its actual position. The star appears
                                     slightly higher (above) than its actual position when viewed near the
                                     horizon (Fig. 10.9). Further, this apparent position of the star is not
                                     stationary, but keeps on changing slightly, since the physical conditions
                                     of the earth’s atmosphere are not stationary, as was the case in the
                                     previous paragraph. Since the stars are very distant, they approximate
                                     point-sized sources of light. As the path of rays of light coming from
                                     the star goes on varying slightly, the apparent position of the star
                                     fluctuates and the amount of starlight entering the eye flickers – the
                                     star sometimes appears brighter, and at some other time, fainter, which
                                     is the twinkling effect.
                                                        Why don’t the planets twinkle? The planets are much
                                                    closer to the earth, and are thus seen as extended sources.
                                                    If we consider a planet as a collection of a large number
                                                    of point-sized sources of light, the total variation in the
                                                    amount of light entering our eye from all the individual
                                                    point-sized sources will average out to zero, thereby
                                                    nullifying the twinkling effect.

                                                    Advance sunrise and delayed sunset
                                                    The Sun is visible to us about 2 minutes before the actual
                                                    sunrise, and about 2 minutes after the actual sunset
                                                    because of atmospheric refraction. By actual sunrise, we
                                                    mean the actual crossing of the horizon by the Sun. Fig.
                                                    10.10 shows the actual and apparent positions of the
              Figure
              Figure 10.10
                     10.10
              Figure 10.1010.10                     Sun with respect to the horizon. The time difference
              Figure
              Figure 10.10
              Atmospheric refraction                between actual sunset and the apparent sunset is about
              effects at sunrise and                2 minutes. The apparent flattening of the Sun’s disc at
              sunset
                                                    sunrise and sunset is also due to the same phenomenon.
               168                                                                                   Science

                                                           2024-25
   168   169   170   171   172   173   174   175   176   177   178