2013 · Q14
Variations in the length of daytime and nighttime from season to season are due to
- (a)the earth's rotation on its axis
- (b)the earth's revolution round the sun in an elliptical manner
- (c)latitudinal position of the place
- (d)revolution of the earth on a tilted axis
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The phenomenon has two necessary conditions acting together: the inclination of the earth's axis at about 23.5 degrees to the perpendicular to the plane of the ecliptic, and the earth's revolution around the sun. Because the axis maintains a fixed orientation in space through the orbit, a condition called parallelism, the circle of illumination cuts the parallels of latitude unequally at all positions except the equinoxes, and the proportion of each parallel lying in daylight therefore changes through the year.
- Option (d) captures both conditions and is correct.
- Option (a) is incorrect because rotation produces the alternation of day and night and fixes its twenty four hour period, but a rotating earth with an upright axis would give every place a twelve hour day throughout the year.
- Option (b) is incorrect because orbital eccentricity varies the earth's distance from the sun and therefore the intensity of insolation and the speed of orbital motion, which is why the seasons are of slightly unequal length, but it does not vary day length; a circular orbit with a tilted axis would still produce the full seasonal swing.
- Option (c) is incorrect because latitude explains why the seasonal variation in day length is negligible at the equator and extreme at the poles, that is, it explains the spatial pattern of the variation, but it cannot explain why the variation occurs at all at a single fixed place, which is what the question asks. The elimination route is to ask, of each option, whether removing that factor while keeping the others would abolish the phenomenon; only the tilt survives that test.
Easy · Static · Geography · Climatology and Atmospheric Processes