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Sun, Earth, Time, Day and Year

🎓 Class 8 Science CBSE Theory Ch 11 — Friction ⏱ ~32 min
🌐 Language: [gtranslate]

This MCQ module is based on: Sun, Earth, Time, Day and Year

[myaischool_lt_science_assessment grade_level="class_8" science_domain="physics" difficulty="basic"]

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.

Fig 11.1 — Earth's Rotation: Day and Night Sun N (axis) Day Night Rotation (24 h) The Earth turns from west to east; the Sun only appears to move.
Fig 11.1 — One full rotation of the Earth = one day = 24 hours.
1 Day = 24 Hours: the average time Earth takes to complete one rotation with respect to the Sun. This is the very first unit of time that humans learnt to use.

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".

Fig 11.2 — How a Sundial Tells Time Gnomon (Shanku) Morning shadow Noon (shortest) Evening shadow W E (Ground marked with hour lines)
Fig 11.2 — The shadow of the gnomon swings across the dial as the Sun crosses the sky.

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.

🏛️
Delhi Jantar Mantar
Built 1724. The first of the five. Close to Connaught Place; houses the Samrat, Jai Prakash and Ram Yantras.
🏰
Jaipur Jantar Mantar
Built 1734. The largest. UNESCO World Heritage Site. Contains the 27-metre Samrat Yantra.
🕉️
Ujjain Observatory
Ujjain is historically the prime meridian of Indian astronomy — the "Greenwich" of ancient India.
📐
Shanku Yantra
A simple vertical rod used for centuries before Jantar Mantar to measure time and solar declination.

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.

Fig 11.3 — Earth's Revolution around the Sun Sun Spring Summer Autumn Winter One full orbit = 1 year
Fig 11.3 — Earth goes once round the Sun in about 365.25 days. That journey is the year.
1 Year ≈ 365.25 Days: the time Earth takes for one complete revolution around the Sun.

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.

Leap Year Rule (simple form): If a year is divisible by 4, it is 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 TimeBased onApproximate length
DayOne rotation of the Earth24 hours
Saur Maas (solar month)Sun passing through one zodiac sign≈ 30 days
YearOne revolution of the Earth around the Sun≈ 365.25 days
Leap YearEvery 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.

🌞 Activity 11.1 — Build Your Own Sundial

You will need: a level patch of ground in sunlight, a straight stick about 30 cm long, small stones or chalk, and a watch.

  1. Stick the rod firmly upright in the ground so it stands perfectly vertical. This is your gnomon.
  2. 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.
  3. Write the time (9, 10, 11, 12 …) neatly beside each mark.
  4. Continue until sunset. Join the marks with a gentle curve.
🔍 Predict: At what time of day will the shadow be shortest? In which direction will it point then? Will your hour-marks be evenly spaced?

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

🌅
The Day
One rotation of Earth = 24 hours. Sunrise, noon and sunset mark its natural beats.
🗓️
The Year
One revolution of Earth = 365.25 days. It gives us seasons, monsoons and harvests.
🕰️
Sundials
The first clock ever built — no moving parts, powered entirely by sunlight.
📆
Solar Calendar
Months defined by the Sun's passage through the 12 zodiac signs: the Saur Maas.

🎯 Competency-Based Questions

Aarav is on a summer vacation at his grandmother's village. There are no clocks in the courtyard, but his grandmother has fixed a tall vertical rod in the centre with stone markers arranged around it. "This is how we told time when I was your age," she says. Every hour she points to a new stone, and the family knows exactly when to eat lunch.

Q1. L1 Remember Name the approximate time taken by the Earth for (i) one rotation and (ii) one revolution.

Answer: (i) One rotation = 24 hours (one day). (ii) One revolution around the Sun = about 365 days and 6 hours (one year).

Q2. L2 Understand Explain why the shadow of Aarav's rod is shortest around noon.

Answer: Near noon, the Sun is at its highest point in the sky for the day. A high Sun shines almost straight down, so the shadow of a vertical rod becomes very short. As the Sun moves lower towards the horizon in the morning or evening, the same rod casts a long slanting shadow.

Q3. L3 Apply Aarav's cousin claims: "If a year were exactly 365 days, we would not need leap years." Is he correct? Justify.

Answer: The cousin is right in principle. Leap years exist only because Earth takes about 365.25 days to complete one revolution. The extra 6 hours every year would slowly push the calendar out of step with the seasons. To correct this, we add one extra day every 4 years — the leap day, 29 February. If the year had been exactly 365 days, no such correction would ever be needed.

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?

Answer: Near sunrise and sunset the Sun is low, so even a small change in its angle throws the tip of the shadow a long way across the ground. Near noon the Sun is almost overhead, so the same angular motion moves the shadow tip only a tiny distance. As a result, equal intervals of time map to unequal spacings on the dial — wide apart at the edges, cramped near noon.

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.

Answer: The claim is incorrect. The Jantar Mantar instruments are precision astronomical tools. The Samrat Yantra at Jaipur can tell local time to within about 2 seconds — remarkable accuracy for a stone instrument with no moving parts. Astronomers of the 18th century used them to track the Sun, forecast eclipses and build star catalogues. They are simultaneously a heritage site and working scientific instruments, which is why Jaipur's Jantar Mantar is recognised as a UNESCO World Heritage Site.

🔗 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.

  • A. Both A and R are true, and R correctly explains A.
  • B. Both A and R are true, but R does not explain A.
  • C. A is true, R is false.
  • D. A is false, R is true.
Answer: A. Earth's west-to-east spin produces an apparent east-to-west drift of the Sun, Moon and stars — a direct cause-and-effect relationship.

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.

  • A. Both A and R are true, and R correctly explains A.
  • B. Both A and R are true, but R does not explain A.
  • C. A is true, R is false.
  • D. A is false, R is true.
Answer: C. A is true as a convenient whole-number value. R is false — Earth actually completes about 365.25 rotations per revolution, which is why every 4th year is made a leap year of 366 days.

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.

  • A. Both A and R are true, and R correctly explains A.
  • B. Both A and R are true, but R does not explain A.
  • C. A is true, R is false.
  • D. A is false, R is true.
Answer: A. A high Sun produces a near-vertical light beam, so a vertical stick casts very little shadow. At sunrise/sunset the Sun is low, giving long slanting shadows.
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Science Class 8 — Curiosity
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