NCERT Class 4 EVS • New NEP 2020 / NCF 2023

Chapter 10: Our Sky

The Solar System, Earth's Rotation & Revolution, Moon Phases & Constellations | CBSE Session 2026–27

Core Pedagogical Competencies & Concepts
  • The celestial sphere: Sun, Moon, stars, constellations, and artificial observation satellites.
  • Day and Night mechanics: Earth's 24-hour rotation from West to East around its tilted axis.
  • The changing phases of the Moon: 29.5-day synodic cycle from New Moon (Amavasya) to Full Moon (Purnima).
  • Finding directions using the night sky: Saptarshi (Big Dipper) and Dhruva Tara (Pole Star).
Our Sky — Earth's Rotation & Saptarshi Constellation SUN ☀️ DAY NIGHT सप्तर्षि (Saptarshi) Earth rotates West to East in 24 hours: The side facing the Sun has Day, the side in shadow has Night.

All Textbook Exercises & In-Text Tasks (14 Questions)

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Q1 Astronomy & Planetary Science
Why do day and night occur on Earth? Why does the Moon appear to change its shape every night throughout the month?
[4 Marks]
✅ Step-by-Step Solution & Working
1. Why Day and Night occur:
The Earth is a spherical planet that rotates on its tilted axis from West to East once every 24 hours. As it rotates, only one half of the Earth faces the Sun at any given time, experiencing Day. The opposite half faces away into shadow, experiencing Night. As the Earth keeps spinning continuously, day and night follow each other smoothly.

2. Why the Moon's shape appears to change (Phases of the Moon):
The Moon does not produce any light of its own; it reflects sunlight like a mirror. As the Moon orbits around the Earth once every 29.5 days, the angle between the Sun, Earth, and Moon changes constantly. From Earth, we can only see that portion of the sunlit half of the Moon that faces us. When none of the sunlit side faces Earth, it is a New Moon (Amavasya); when the entire illuminated side faces us, it is a Full Moon (Purnima).
CBSE Step-by-Step Marking Scheme
Scientific explanation of Earth's 24-hour rotation causing day/night 2.0 M
Explanation of Moon reflecting sunlight and orbital angle phases 2.0 M
Q2 Sky Observation • Constellations
What is a 'constellation'? Describe the Saptarshi (Ursa Major) constellation and explain how it helps locate the Pole Star.
[3 Marks]
✅ Step-by-Step Solution & Working
1. Constellation:
A constellation is a recognizable pattern or group of bright stars in the night sky that people historically associated with mythological figures, animals, or objects.

2. Saptarshi & Locating the Pole Star:
• Saptarshi (Big Dipper / Ursa Major): Consists of seven prominent bright stars arranged in the shape of a large ladle or dipper (four stars forming the cup and three stars forming the curved handle).
• Locating Dhruva Tara (Pole Star): The two front stars of the cup are called Pointer Stars. If an imaginary straight line is extended upward through these two pointer stars by about five times the distance between them, it points directly to the Pole Star (North Star), which always marks true geographic North.
CBSE Step-by-Step Marking Scheme
Definition of constellation 1.0 M
Description of Saptarshi's seven stars and pointer line to Pole Star 2.0 M
Q3 Solar Motion • Shadows & Time
How does the length and direction of a tree's shadow change from morning to evening? How did people use sundials in ancient times?
[3 Marks]
✅ Step-by-Step Solution & Working
1. Daily Shadow Patterns:
• Early Morning: The Sun is low in the eastern sky, creating very long shadows pointing West.
• Noon (Midday): The Sun reaches its highest point directly overhead, casting the shortest shadow of the day.
• Late Evening: The Sun sinks low in the western sky, casting long shadows pointing East.

2. Ancient Sundials:
Ancient astronomers (like Maharaja Jai Singh at Jantar Mantar) built large triangular ramps called gnomons that cast shadows on calibrated curved marble scales. As the Sun traversed the sky, the moving shadow position accurately indicated the exact hour and minute of the day.
CBSE Step-by-Step Marking Scheme
Clear daily progression of shadow length and direction 1.5 M
Principle of sundial timekeeping explained 1.5 M
Q4 Safety in Astronomy • Solar Observation
Why must you NEVER look directly at the Sun with naked eyes or through ordinary binoculars, even during a solar eclipse?
[2 Marks]
✅ Step-by-Step Solution & Working
Danger of Direct Solar Viewing:
The Sun emits intense, focused ultraviolet (UV) and infrared rays. Staring directly at the Sun—or focusing its light through magnifying binoculars or telescopes—burns the light-sensitive retinal cells at the back of the eye (solar retinopathy) in a matter of seconds without causing pain. This can lead to permanent blind spots or complete, incurable blindness. One must only use certified ISO 12312-2 solar filter glasses or pinhole projection methods.
CBSE Step-by-Step Marking Scheme
Scientific explanation of retinal burn / UV damage and safe viewing methods 2.0 M
Q5 Celestial Mechanics • Day and Night
How are day and night formed on Earth? Explain with a simple globe and torch experiment.
[3 Marks]
✅ Step-by-Step Solution & Working
Day and Night Formation:
Earth is a sphere that rotates continuously on its tilted axis from West to East once every 24 hours.
• Experiment: Shine a torch (representing the Sun) on a globe (representing Earth) in a dark room. The half facing the torch receives light and experiences Day. The opposite half in shadow experiences Night. As the globe turns, day and night alternate.
CBSE Step-by-Step Marking Scheme
Rotation of Earth every 24 hours cited 1.5 M
Globe and torch experiment described 1.5 M
Q6 Lunar Phases • Moon Cycle
Why does the shape of the Moon appear to change every night? Name four distinct phases of the Moon.
[4 Marks]
✅ Step-by-Step Solution & Working
Phases of the Moon:
The Moon does not produce its own light; it reflects sunlight. As the Moon orbits around Earth, we see differing amounts of its sunlit half from Earth.
Four Phases:
1. New Moon (Amavasya): Moon is between Earth and Sun; dark side faces Earth.
2. Crescent Moon: A tiny curved sliver of light.
3. Half Moon (First/Last Quarter): Half the lit face is visible.
4. Full Moon (Purnima): Entire round sunlit face shines brightly.
CBSE Step-by-Step Marking Scheme
Reflected sunlight and orbit explained 2 M
Four lunar phases correctly named 2 M
Q7 Solar Energy • The Sun
Why is the Sun called the ultimate source of light and energy for all life on planet Earth?
[3 Marks]
✅ Step-by-Step Solution & Working
The Sun as Ultimate Source:
1. Photosynthesis: Green plants use sunlight to produce food and oxygen, supporting all herbivores and carnivores.
2. Weather & Water Cycle: Solar heat evaporates water to form rain clouds and drives wind currents.
3. Warmth: Without solar heat, Earth would freeze into an uninhabitable ice planet.
CBSE Step-by-Step Marking Scheme
Photosynthesis role explained 1 M
Water cycle / weather driver 1 M
Thermal life support 1 M
Q8 Constellations • Saptarshi (Big Dipper)
What is a constellation? Describe the Saptarshi (Ursa Major / Great Bear) constellation.
[3 Marks]
✅ Step-by-Step Solution & Working
Constellations:
• Constellation: A recognizable pattern or group of bright stars in the night sky forming imaginary shapes of animals, mythological heroes, or objects.
• Saptarshi: A group of seven prominent stars resembling a giant saucepan or dipper (four stars form the bowl and three form the curved handle).
CBSE Step-by-Step Marking Scheme
Scientific definition of constellation 1.5 M
Saptarshi seven stars and saucepan shape 1.5 M
Q9 Direction Finding • Pole Star (Dhruva Tara)
How can you find the North direction on a clear night using the pointer stars of Saptarshi?
[3 Marks]
✅ Step-by-Step Solution & Working
Locating the Pole Star:
Look at the two stars forming the outer front wall of the Saptarshi's bowl (Pointer Stars). Imagine a straight line drawn through them and extended five times their distance upwards. This imaginary line leads directly to the Pole Star (Dhruva Tara), which always indicates true North.
CBSE Step-by-Step Marking Scheme
Pointer stars identified 1.5 M
Line projection to Pole Star (North) 1.5 M
Q10 Solar Safety • Viewing Eclipses
Why should we never look directly at the Sun or during a solar eclipse with naked eyes?
[2 Marks]
✅ Step-by-Step Solution & Working
Solar Eye Safety:
Intense solar ultraviolet (UV) and infrared radiation can permanently burn the sensitive retinal cells of our eyes, causing irreversible blindness. We must only use certified solar eclipse safety glasses or pinhole projection.
CBSE Step-by-Step Marking Scheme
Retinal burn / UV damage explained 1 M
Certified solar filters stated 1 M
Q11 Astronomy • Planets vs Stars
State two differences between a star and a planet that can be observed in the night sky.
[2 Marks]
✅ Step-by-Step Solution & Working
Stars vs Planets:
• Stars: Massive balls of burning gas that emit their own light; they appear to twinkle due to atmospheric refraction.
• Planets: Solid or gaseous bodies that reflect sunlight; they shine with steady, non-twinkling light.
CBSE Step-by-Step Marking Scheme
Own light vs reflected light 1 M
Twinkling vs steady light 1 M
Q12 Atmosphere • Blue Sky
Why does the daytime sky appear blue to our eyes on a clear sunny day?
[2 Marks]
✅ Step-by-Step Solution & Working
Why Sky is Blue:
White sunlight contains all rainbow colors. As light passes through Earth's atmosphere, tiny gas molecules scatter the shorter, blue light waves much more strongly in all directions than other colors.
CBSE Step-by-Step Marking Scheme
Atmospheric scattering of short blue wavelengths 2 M
Q13 Atmospheric Phenomenon • Rainbow
When and where does a rainbow appear in the sky? What causes its seven colors?
[2 Marks]
✅ Step-by-Step Solution & Working
Rainbow Formation:
A rainbow appears when sunlight shines while rain is falling, always in the sky opposite to the Sun. Tiny suspended raindrops act like microscopic glass prisms that refract, reflect, and disperse white sunlight into its seven constituent colors (VIBGYOR).
CBSE Step-by-Step Marking Scheme
Opposite to Sun condition 1 M
Raindrop dispersion of light into VIBGYOR 1 M
Q14 Space Exploration • Satellites
What is an artificial satellite? Mention two ways satellites help people in their everyday lives.
[3 Marks]
✅ Step-by-Step Solution & Working
Artificial Satellites:
Human-made spacecraft launched by rockets that orbit Earth.
Everyday Uses:
1. Weather Forecasting: Tracking cyclones and storms to issue early disaster warnings.
2. Communication & GPS: Enabling television broadcasts, mobile phone networks, and vehicle navigation maps.
CBSE Step-by-Step Marking Scheme
Definition of artificial satellite 1 M
Weather warnings and GPS navigation uses 2 M
🌟 NEP 2020 Competency-Based Case Study

Night Sky Navigation Using the Pole Star

Ancient sailors and desert travelers had no compass or GPS. On dark clear nights, they never got lost.

Analytical Task: How did travelers locate true North in the night sky using the Saptarshi (Big Dipper) constellation?
Evaluation & Model Answer:
Travelers located the seven bright stars of Saptarshi (Ursa Major). The two stars forming the outer front wall of the 'dipper cup' are called the Pointer Stars. Drawing an imaginary straight line through these two pointer stars and extending it five times upward leads directly to a bright, steady star called the Pole Star (Dhruva Tara), which always points to true geographic North.
Rubric: 1.5 Marks for identifying Saptarshi and Pointer Stars; 1.5 Marks for projecting line to Pole Star (North).