Indian Geography (Unit 1-Topic 1) Latitudes and Longitudes

byBright Zoom •May 18, 2018

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Indian Geography (Unit 1-Topic 1)

Latitudes and Longitudes are imaginary lines used to determine the location of a place on earth.
The shape of the earth is ‘Geoid’. And the location of a place on the earth can be mentioned in terms of latitudes and longitudes.
Example: The location of New Delhi is 28° N, 77° E.

Latitude is the angular distance of a point on the earth’s surface, measured in degrees from the center of the earth.
As the earth is slightly flattened at the poles, the linear distance of a degree of latitude at the pole is a little longer than that at the equator.
For example at the equator (0°) it is 68.704 miles, at 45° it is 69.054 miles and at the poles it is 69.407 miles. The average is taken as 69 miles (111km).
1 mile = 1.607 km.

Besides the equator (0°), the north pole (90°N) and the south pole (90° S), there are four important parallels of latitudes–
Tropic of Cancer (23½° N) in the northern hemisphere.
Tropic of Capricorn (23½° S) in the southern hemisphere.
Arctic circle at 66½° north of the equator.
Antarctic circle at 66½° south of the equator.

The mid-day sun is exactly overhead at least once a year on all latitudes in between the Tropic of Cancer and the Tropic of Capricorn. This area, therefore, receives the maximum heat and is called the torrid zone.
The mid-day sun never shines overhead on any latitude beyond the Tropic of Cancer and the Tropic of Capricorn. The angle of the sun’s rays goes on decreasing towards the poles. As such, the areas bounded by the Tropic of Cancer and the Arctic circle in the northern hemisphere, and the Tropic of Capricorn and the Antarctic circle in the southern hemisphere, have moderate temperatures. These are, therefore, called temperate zones.
Areas lying between the Arctic circle and the north pole in the northern hemisphere and the Antarctic circle and the south pole in the southern hemisphere, are very cold. It is because here the sun does not raise much above the horizon. Therefore, its rays are always slanting. These are, therefore, called frigid zones.

Longitude is an angular distance, measured in degrees along the equator east or west of the Prime (or First) Meridian.
On the globe longitude is shown as a series of semi-circles that run from pole to pole passing through the equator. Such lines are also called
Unlike the equator which is centrally placed between the poles, any meridian could have been taken to begin the numbering of longitude. It was finally decided in 1884, by international agreement, to choose as the zero meridian the one which passes through the Royal Astronomical Observatory at Greenwich, near London.
This is the Prime Meridian (0°) from which all other meridians radiate eastwards and westwards up to 180°.
As the parallels of latitude become shorter poleward, so the meridians of longitude, which converge at the poles, enclose a narrower space.
They have one very important function, they determine local time in relation to G.M.T. or Greenwich Mean Time, which is sometimes referred to as World Time.

Since the earth makes one complete revolution of 360° in one day or 24 hours, it passes through 15° in one hour or 1° in 4 minutes.
The earth rotates from west to east, so every 15° we go eastwards, local time is advanced by 1 hour. Conversely, if we go westwards, local time is retarded by 1 hour.
We may thus conclude that places east of Greenwich see the sun earlier and gain time, whereas places west of Greenwich see the sun later and lose time.
If we know G.M.T., to find local time, we merely have to add or subtract the difference in the number of hours from the given longitude.