This MCQ module is based on: Sun, Earth, Time, Day and Year
Sun, Earth, Time, Day and Year
Probe and Ponder
Close your eyes and picture yesterday morning. How did you know it was morning and not midnight? Most likely the Sun was already up, warm light pouring through the window, birds calling. But suppose you had no clock, no phone, no watch — how would you tell that three hours had passed? Or that it was almost time for lunch?
- Why does the Sun rise in the east and set in the west every single day, without fail?
- How did people, thousands of years before clocks were invented, know the time of day?
- Why is one "year" exactly 365 days — and where do the extra "leap day" hours come from?
- Have you heard the shadow of a person getting shorter by noon and longer again in the evening? What makes it behave so?
In this chapter we step outside and look at the sky — the oldest clock and calendar ever invented. The Sun, the Moon and the stars have been ticking above our heads since long before humans existed, and ancient Indian observers learnt to read them with astonishing precision.
11.1 The Earth Spins — and a Day is Born
Stand still in your school ground at sunrise. In a few minutes you will see the Sun climb a little higher. By noon it is overhead. By evening it slides down to the west and disappears. For most of history people believed the Sun was moving around the Earth — a reasonable guess, because that is exactly what our eyes show us.
We now know the truth is the opposite. The Earth rotates on its own axis — an imaginary line running from the North Pole to the South Pole — completing one full turn in about 24 hours. As our part of the Earth swings round to face the Sun, we call it day. When it swings away, we call it night. The Sun has barely moved; it is we who are turning.
Why Does the Sun Appear to Move from East to West?
The Earth spins from west to east, so the edge of our view slides eastwards. Whatever is in the sky — Sun, Moon, stars — therefore seems to drift in the opposite direction, from east to west. The rising Sun always appears in the east; the setting Sun always in the west. Many Indian languages even capture this: Pūrva (east) comes from "in front", where the day begins.
11.2 The Sundial — The First Clock
Long before mechanical clocks, ancient people noticed that the shadow of a stick in the ground changed direction and length as the Sun moved across the sky. A pointed stick stuck upright in level earth could, with a little marking, be turned into a clock. This simple device is called a sundial.
At sunrise the shadow is long and points westwards. As the morning advances, the shadow swings towards the north (in the Indian subcontinent) and shortens, reaching its shortest length near noon. By afternoon it grows again and points eastwards, lengthening until sunset. Markings drawn on the ground turn these changes into readable "hours".
Jantar Mantar — India's Giant Open-Air Clocks
In the early 18th century, Maharaja Sawai Jai Singh II of Jaipur built a series of stone observatories called Jantar Mantar at Delhi, Jaipur, Ujjain, Varanasi and Mathura. Each houses giant sundials — stone triangles and circles built so large that they can measure time to within a few seconds. The Samrat Yantra ("Supreme Instrument") at Jaipur is the tallest sundial on Earth.
11.3 The Earth Revolves — and a Year is Born
While Earth spins on its axis, it also travels along a wide oval path around the Sun. This orbital journey is called revolution. One complete trip around the Sun takes approximately 365 days and 6 hours.
The Problem of the Quarter Day — and the Leap Year
If a year were exactly 365 days, everything would be simple. But it is 365 days plus roughly 6 hours. If we ignored those 6 hours every year, after 4 years the calendar would be 24 hours behind the Sun — our summer would start shifting into spring. Within a century, seasons and months would fall completely out of step!
The clever solution: ignore the 6 extra hours for three ordinary years, then add all the saved hours (6 × 4 = 24 = one full day) as a single extra day in the fourth year. That extra day is February 29, and such a year is called a leap year.
Example: 2020 ✓, 2024 ✓, 2028 ✓. But 2023 ✗, 2025 ✗.
Small fine-print for century years: a century year (like 1900 or 2100) is a leap year only if it is also divisible by 400. So 2000 was a leap year, but 1900 was not.
The Saur Maas — India's Solar Month
Ancient Indian astronomers divided the Sun's yearly path through the sky into 12 equal parts, one for each zodiac sign (rashi). The time the Sun takes to travel through one zodiac sign is the Saur Maas — the solar month — and it lasts about 30 days. The day the Sun crosses from one sign into the next is called a Sankranti. Makar Sankranti, celebrated in January, is the day the Sun enters Makara (Capricorn).
| Unit of Time | Based on | Approximate length |
|---|---|---|
| Day | One rotation of the Earth | 24 hours |
| Saur Maas (solar month) | Sun passing through one zodiac sign | ≈ 30 days |
| Year | One revolution of the Earth around the Sun | ≈ 365.25 days |
| Leap Year | Every 4th year (with century fine print) | 366 days |
11.4 The Sun Across the Year
Because Earth's axis is tilted by about 23.5°, the Sun does not rise at exactly the same point on the eastern horizon every day. In summer it rises a little to the north of due east; in winter a little to the south. Ancient observers who watched sunrise from a fixed spot over many months could track the year almost as precisely as a modern calendar.
This is also why days are longer in summer and shorter in winter: the tilt means the Sun's path through the summer sky is high and long, while in winter it is low and short. The two special days when day and night are exactly equal — the equinoxes — occur around 21 March and 23 September each year.
You will need: a level patch of ground in sunlight, a straight stick about 30 cm long, small stones or chalk, and a watch.
- Stick the rod firmly upright in the ground so it stands perfectly vertical. This is your gnomon.
- On a sunny morning, starting at 8 a.m., go outside every hour and place a small stone (or chalk mark) at the tip of the shadow.
- Write the time (9, 10, 11, 12 …) neatly beside each mark.
- Continue until sunset. Join the marks with a gentle curve.
Shortest shadow: near 12 noon (local solar noon), pointing due north (in most of India). This is when the Sun is highest in the sky.
Direction change: the shadow starts in the west at sunrise and ends in the east at sunset — opposite to the Sun.
Spacing: the marks are not evenly spaced. Near noon they cluster close together; near sunrise and sunset they spread far apart. This is because the angle the Sun sweeps per hour looks different depending on where it is in the sky.
Now you can read the time on any sunny day — just check which stone the shadow tip is near!
11.5 What We Owe to the Sun
🎯 Competency-Based Questions
Q1. L1 Remember Name the approximate time taken by the Earth for (i) one rotation and (ii) one revolution.
Q2. L2 Understand Explain why the shadow of Aarav's rod is shortest around noon.
Q3. L3 Apply Aarav's cousin claims: "If a year were exactly 365 days, we would not need leap years." Is he correct? Justify.
Q4. L4 Analyse Why do the hour marks drawn on Aarav's grandmother's sundial become closer together near noon and farther apart near sunrise and sunset?
Q5. L5 Evaluate A friend says that the Jantar Mantar of Jaipur is "just a big tourist attraction with no scientific value". Evaluate this claim.
🔗 Assertion–Reason Questions
Assertion (A): The Sun appears to move from east to west across the sky every day.
Reason (R): The Earth rotates on its axis from west to east, so objects in the sky appear to move in the opposite direction.
Assertion (A): One year on Earth is taken to be 365 days.
Reason (R): Earth completes exactly 365 rotations during one revolution around the Sun.
Assertion (A): A vertical stick's shadow is shortest at local noon.
Reason (R): At local noon the Sun is at its highest point in the sky for that day.