Stars and the Sun

A free interactive lesson on stars for Class 5 — the Sun is our nearest star, 109 Earths across, powered by nuclear fusion, 8 light-minutes away. Learn why star colour tells us temperature, and the life cycle from blue giant to white dwarf. Based on NCERT Class 5 Space. Includes quiz.

Class 5 ScienceClass 5 / Grade 5Ages 7–10
Lesson
Stars and the Sun
Our Sun is a star — and there are billions more.The SunOther stars (much, much farther away)

On a clear night you can see about two thousand stars with the naked eye. Every single one of them is a sun — a giant ball of glowing gas powered by nuclear reactions. Our own Sun is just the closest one. It looks so much bigger than the others only because it's a hundred and fifty million kilometres away, while the next nearest star is forty trillion kilometres.

The Sun — our nearest star

The Sun is a star — the same as every glittering point of light in the night sky, just unimaginably closer. The Sun is about 150 million km from Earth; the next nearest star (Proxima Centauri) is about 40 trillion km away — roughly 270,000 times further.

The Sun's diameter is about 1.4 million km — you could fit 109 Earths side by side across it. Its mass is 330,000 times Earth's mass, containing 99.8% of all the mass in the solar system.

How the Sun produces energy — nuclear fusion

The Sun's core reaches 15 million °C — so hot that hydrogen atoms are stripped of their electrons and forced together with enough pressure that they fuse into helium atoms. This process, nuclear fusion, releases an enormous amount of energy. Every second, the Sun converts about 600 million tonnes of hydrogen into helium — with 4 million tonnes converted directly into energy (following E=mc²).

The Sun has been burning for 4.6 billion years and has enough hydrogen to continue for another 5 billion years. It is currently in the main sequence phase of its life — a stable, middle-aged star.

Light travel time

Light travels at 300,000 km per second — the fastest anything can travel. At this speed, light takes about 8 minutes 20 seconds to travel from the Sun to Earth. This means when you look at the Sun (never directly — it will damage your eyes), you're seeing it as it was 8 minutes ago. When you look at the Moon, you're seeing it as it was 1.3 seconds ago. The nearest star beyond the Sun is 4.2 light-years away — its light left 4.2 years ago.

Types of stars

Stars come in different sizes, temperatures, and colours — and a star's colour tells us directly how hot it is:

  • Blue/blue-white stars — the hottest (surface temperature above 10,000°C) and most massive. They burn through their fuel quickly and live only millions of years (vs billions for smaller stars).
  • Yellow stars (like our Sun) — medium temperature (~5,500°C surface) and size. Main sequence stars that live for billions of years.
  • Orange and red stars — cooler (3,000–5,000°C), but red giants are very old, swollen stars that have exhausted their core hydrogen.
  • White dwarfs — the remnant core of a dead star like our Sun. Very dense (a teaspoon weighs tonnes) and slowly cooling over billions of years.

Frequently asked questions

What is the Sun made of?

The Sun is about 74% hydrogen and 25% helium by mass, with traces of heavier elements. Its core converts hydrogen into helium through nuclear fusion, releasing the energy that lights and warms our solar system.

How far is the Sun from Earth?

About 150 million km. Light takes 8 minutes 20 seconds to travel from the Sun to Earth at 300,000 km/second. This distance is called 1 Astronomical Unit (AU).

What does a star's colour tell us?

A star's colour indicates its surface temperature. Blue and blue-white stars are the hottest (above 10,000°C). Yellow stars like the Sun are medium temperature (~5,500°C). Red stars are the coolest (about 3,000°C). The hotter the star, the bluer its light.

What is nuclear fusion?

Nuclear fusion is the process that powers stars — hydrogen atoms are forced together under extreme heat and pressure (15 million °C in the Sun's core) to form helium atoms. The reaction releases enormous energy. Unlike nuclear fission (used in power plants), fusion produces no long-lived radioactive waste.

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