📖 PART 1: Latitudes (Parallels)
Latitude is the angular distance of a point north or south of the Equator, measured in
degrees (°), minutes ('), and seconds ("). The Equator is 0° latitude. Lines joining places of the same
latitude are called parallels of latitude.
- Latitudes range from 0° (Equator) to 90°N (North Pole) and
90°S (South Pole).
- Total number of latitude lines: 181 (including the Equator).
- All parallels of latitude are circles (decrease in circumference from Equator to
poles). All parallels of latitude run east-west.
- Distance between any two adjacent parallels (1° apart) = approximately 111 km.
Important Latitudes and Their Names
| Latitude |
Name |
Significance |
| 0° |
Equator |
Divides Earth into N and S hemispheres; longest parallel; 12 hrs day/night all year |
| 23½°N |
Tropic of Cancer |
Sun is directly overhead on June 21 (Summer Solstice) — northernmost position of vertical Sun
|
| 23½°S |
Tropic of Capricorn |
Sun is directly overhead on December 22 (Winter Solstice) — southernmost position of vertical
Sun |
| 66½°N |
Arctic Circle |
24-hour daylight on June 21; 24-hour darkness on Dec 22 |
| 66½°S |
Antarctic Circle |
24-hour daylight on Dec 22; 24-hour darkness on June 21 |
| 90°N |
North Pole |
6 months day, 6 months night; all longitudes meet |
| 90°S |
South Pole |
6 months day, 6 months night; all longitudes meet |
Uses of Latitudes
- Used to locate the north-south position of a place on Earth.
- Determine climate zones: Torrid Zone (0°–23.5°), Temperate Zone (23.5°–66.5°), Frigid
Zone (66.5°–90°).
- Help in determining duration of day and night.
📖 PART 2: Longitudes (Meridians)
Longitude is the angular distance of a point east or west of the Prime Meridian (0°),
measured in degrees (0° to 180°). Lines joining places of the same longitude are called meridians of
longitude. All meridians are semi-circles and are of equal
length, running north-south.
- Total number of meridians: 360 (one every 1°). Each degree can be divided into 60 minutes and each
minute into 60 seconds.
- All meridians meet at the North and South Poles.
- The distance between two adjacent meridians decreases from the Equator (111 km apart) to zero at the
poles.
Important Longitudes
| Longitude |
Name |
Significance |
| 0° |
Prime Meridian (Greenwich Meridian) |
Passes through the Royal Observatory, Greenwich, London. Reference meridian for time
zones. |
| 180° |
International Date Line (IDL) |
Opposite of Prime Meridian; passes mainly through Pacific Ocean; when crossed, date changes |
| 82°30'E |
Standard Meridian of India (IST) |
India's standard time = GMT + 5:30 hours; passes through Mirzapur (UP) |
Uses of Longitudes
- Determine the east-west position of a place.
- Determining local time and time zones. Every 15° of longitude = 1 hour difference in
time (Earth rotates 360° in 24 hours → 15° per hour).
⏰ PART 3: Time – Local, Standard, and Time Zones
Local Time
- Local Time is time based on the position of the Sun at a specific meridian — it is 12
noon (Local Solar Time) when the Sun is at its highest point (overhead or due south).
- Local time changes by 4 minutes for every 1° of longitude (as Earth rotates 1° every 4 minutes).
- Places to the east have a later (ahead) time than places to the west.
💡 Time Calculation Formula
If a place is X°
east of Greenwich: IST = GMT + (X ÷ 15) hours
If a place is X°
west of Greenwich: local time = GMT − (X ÷ 15) hours
India (82°30'E): 82.5 ÷ 15 = 5.5 hours →
IST = GMT + 5:30 hours
Standard Time
- A country or region adopts a single time for the whole area, based on one standard
meridian, to avoid confusion from different local times across the country.
- India's standard time (IST) is based on the 82°30'E meridian (Mirzapur, UP) and is
5 hours 30 minutes ahead of GMT (UTC+5:30).
Greenwich Mean Time (GMT)
- The time at the Prime Meridian (0° longitude) — used as the world reference time. Also called
Universal Time Coordinated (UTC).
- All countries calculate their standard time as GMT + or − number of hours corresponding to their
standard meridian.
🗓️ PART 4: International Date Line (IDL)
- The International Date Line (IDL) lies broadly along the 180° meridian
in the Pacific Ocean.
- When you cross the IDL going eastward (Pacific to Americas): go back one
day (subtract 1 day).
- When you cross the IDL going westward (Americas to Pacific/Asia): go forward
one day (add 1 day).
- The IDL is not a straight line — it bends around island groups to avoid cutting a
single country or island group into two different dates. Deviates around Aleutian Islands (Alaska),
Fiji, Samoa.
- Why it is needed: Without the IDL, a person travelling west continuously would find
that their calendar is one day behind after circling the globe — IDL corrects for this.
🌐 PART 5: Eastern and Western Hemispheres
- Eastern Hemisphere: All land/area east of Prime Meridian (0°) up to 180° — includes
Europe, Asia, Africa, Australia.
- Western Hemisphere: All land/area west of Prime Meridian (0°) up to 180° — includes the
Americas.
- Great Circles: Any circle on the Earth's surface whose plane passes through the centre
of the Earth. The Equator is the only parallel that is a Great Circle. All meridian pairs (a meridian +
its opposite meridian) form Great Circles. Great Circle routes are the shortest distances between two
points on Earth — used by ships and aircraft.
📌 Chapter Summary
- Latitude: angular distance N/S of Equator (0°–90°). Key parallels: Equator (0°), Tropic of Cancer
(23.5°N), Tropic of Capricorn (23.5°S), Arctic Circle (66.5°N), Antarctic Circle (66.5°S). Uses:
climate zones, seasons, locating places.
- Longitude: angular distance E/W of Prime Meridian (0°–180°). All meridians equal length; meet at
poles. 15° = 1 hour time difference.
- GMT = reference time (0° meridian, Greenwich, London). IST = GMT + 5:30 (82.5°E meridian, Mirzapur).
- IDL = 180° meridian (with deviations); crossing eastward = lose a day; crossing westward = gain a
day.
- Great Circles: planes passing through Earth's centre; shortest route for navigation.