NCERT Solutions Curiosity Chapter 12 Interdisciplinary projects — Exploratory Projects

Book page 186 Updated on2026-09-05

Q1.
Repeat Activity 12.2 but replace the torch with an electric lamp. Then place the globe at different positions on a circle around the lamp while maintaining the tilt of the globe. (i) Note down your observations regarding how much of the Northern and Southern hemispheres of the globe are illuminated at different positions. (ii) Rotate the globe and take a note of the length of the day and night on different parts of the globe. (iii) Repeat (ii) for different positions of globe on the circle.
Answer

This project turns the whole chapter into one table-top model. The one rule that must never be broken: the globe's axis must keep pointing in the same direction — the same way, towards the same corner of the room — at every position on the circle. Do not turn the stand to face the lamp.

How to set it up

  1. Stand a bare electric lamp (no shade) in the middle of a table in a dark room. This is the Sun.
  2. Chalk a circle of radius about 60–75 cm around the lamp. Mark four positions on it: June, September, December, March.
  3. Carry the globe around the circle, keeping the axis tilted the same way throughout, and stop at each mark.

(i) How much of each hemisphere is lit

PositionNorthern HemisphereSouthern HemispherePoles
JuneMore than half of it is litLess than half of it is litNorth Pole fully lit; South Pole fully dark
SeptemberExactly halfExactly halfThe lit–dark line passes through both poles
DecemberLess than half of it is litMore than half of it is litNorth Pole fully dark; South Pole fully lit
MarchExactly halfExactly halfThe lit–dark line passes through both poles

(ii) and (iii) Length of day and night — at each position, spin the globe slowly and watch a sticker on Delhi, one on the equator and one on Australia. Count roughly what fraction of each turn the sticker spends in the light.

Place on the globeJune positionMarch / SeptemberDecember position
Delhi (Northern Hemisphere)Day longer than nightDay ≈ nightDay shorter than night
On the equatorDay ≈ nightDay ≈ nightDay ≈ night
Australia (Southern Hemisphere)Day shorter than nightDay ≈ nightDay longer than night
North Pole24 hours of dayOn the boundary24 hours of night
What the model proves: the lamp never changed and the distance never changed — only the direction of the tilt with respect to the lamp changed. That alone produced longer days, shorter days and midnight sun. This is the strongest possible demonstration that the seasons come from the tilt, not from the distance.
Tip: use a lamp without a shade so light spreads in all directions, and keep the room really dark. Take a photograph of the globe at each position — the four pictures side by side make an excellent chart for the class.
Q2.
The Earth goes around the Sun in an oval-shaped path. Draw two circles with the same centre, one with a radius of 14.7 cm, and another one with a radius of 15.2 cm. If 1 cm corresponds to 10 million km, the two circles represent the closest and farthest distances from the Sun. Note how small is the difference between these two distances.
Answer

Do the drawing on a full A4 sheet with a compass, marking the same centre for both circles.

Scale: 1 cm = 10 million km
Closest distance = 14.7 cm × 10 = 147 million km
Farthest distance = 15.2 cm × 10 = 152 million km
Difference on paper = 15.2 − 14.7 = 0.5 cm (5 mm)
Difference in reality = 152 − 147 = 5 million km
As a fraction = 0.5 ÷ 15.2 ≈ 0.033 = about 3%

What you will see: the two circles are so close together that from a step away they look like one thick line. Yet that 5 mm gap stands for five million kilometres.

What the drawing proves: the Earth's orbit is very nearly a circle. Textbook pictures of an "oval" orbit are exaggerated on purpose, and they mislead students into thinking that seasons come from the changing distance. A 3% change in distance cannot produce summer and winter — the tilt of the axis does that.
Add this to your poster: the Earth is at its closest to the Sun in January — the coldest month in North India. Write that under the two circles; it settles the argument at once.
Q3.
Suppose the tilt of the Earth's axis of rotation increases. Will it cause more extreme seasons? Find out if the tilt of Uranus is more than the Earth and about the seasons there. Write an interesting article for a newspaper or your school magazine about it.
Answer

Yes — a bigger tilt would make the seasons far more extreme, and Uranus is the spectacular proof of it.

EarthUranus
Tilt of the axisAbout 23.5°About 98° — it rolls on its side
Time for one revolutionAbout 1 yearAbout 84 Earth years
Length of one seasonAbout 3 monthsAbout 21 Earth years
At the polesSix months of day, six months of nightAbout 42 years of continuous day, then about 42 years of night

Sample article — you can adapt this in your own words:

Sample answer:
The Planet That Lies Down
On the Earth, a season lasts about three months, and we grumble when June is too hot or January too cold. Blame the tilt: our planet's axis leans by about 23.5°, so each hemisphere takes its turn to face the Sun.
Now imagine tipping that axis right over. That is Uranus. Its axis is tilted by about 98°, which means it does not spin like a top at all — it rolls around the Sun like a ball. For part of its orbit its north pole points almost straight at the Sun; half an orbit later its south pole does.
Uranus needs about 84 Earth years for one trip around the Sun, so each of its seasons drags on for roughly 21 years. At its poles the Sun does not set for about 42 years — and then does not rise for the next 42. A person born at the Uranian north pole would be middle-aged before seeing a single sunrise.
The lesson for us is simple. Seasons are not about how near a planet is to the Sun; they are about how it leans. Tilt a planet a little and you get spring and autumn. Tilt it right over and you get a world of endless summers and endless nights.
Why a bigger tilt means harsher seasons: a larger tilt makes the summer Sun climb higher (so its rays are concentrated on a still smaller area) and makes the summer day still longer, while the winter Sun stays lower for a still shorter day. Both effects grow together, so summers become hotter and winters colder.
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