Stars are not unchanging objects – they don’t last for ever. They are born, evolve and die.

What determines the life cycle of a star?

A star’s life cycle is determined by its mass. The larger its mass, the shorter its life cycle.

More massive stars have a stronger gravitational force acting inwards so their core gets hotter. The higher temperatures mean that the nuclear reactions occur at a much greater rate in massive stars. They thus use up their fuel much quicker than lower mass stars.

Must read: Cepheids – Definition , Use and Classes

What determines the mass of a star?

A star’s mass is determined by the amount of matter that is available in its nebula.

What is nebula?

Nebula is a giant cloud of gas and dust from which a star is born.

Protostar

A star is born from a giant cloud of gas and dust known as nebula. Over time, the hydrogen gas in the nebula is pulled together by gravity and it begins to spin. As the gas spins faster, it heats up and becomes a protostar.

Main Sequence Star

Eventually the temperature reaches 15,000,000 degrees and nuclear fusion occurs in the cloud’s core. The cloud begins to glow brightly, contracts a little, and becomes stable. It is now a main sequence star and will remain in this stage, shining for millions to billions of years to come.

Thus, a star that is fusing hydrogen to helium in its core is known as a main sequence star. Main sequence stars make up around 90% of the universe’s stellar population. This is the stage our Sun is at right now.

Red Giant Phase

As the main sequence star glows, hydrogen in its core is converted into helium by nuclear fusion. When the hydrogen supply in the core begins to run out, and the star is no longer generating heat by nuclear fusion, the core becomes unstable and contracts.

The outer shell of the star, which is still mostly hydrogen, starts to expand. As it expands, it cools and glows red. The star has now reached the red giant phase.

It is red because it is cooler than it was in the main sequence star stage and it is a giant because the outer shell has expanded outward. In the core of the red giant, helium fuses into carbon.

All stars evolve the same way up to the red giant phase. The amount of mass a star has determines which of the following life cycle paths it will take from there.

For low-mass stars like our Sun, after the helium has fused into carbon, the core collapses again. As the core collapses, the outer layers of the star are expelled. A planetary nebula is formed by the outer layers. The core remains as a white dwarf and eventually cools to become a black dwarf.

Like low-mass stars, high-mass stars are born in nebulae and evolve and live in the Main Sequence. However, their life cycles start to differ after the red giant phase. A massive star will undergo a supernova explosion.

If the remnant of the explosion is 1.4 to about 3 times as massive as our Sun, it will become a neutron star.

Pulsars are a type of rapidly rotating neutron star. Bright X-ray hot spots form on the surfaces of these objects. As they rotate, the spots spin in and out of view like the beams of a lighthouse. Some pulsars spin faster than blender blades.

The core of a massive star that has more than roughly 3 times the mass of our Sun after the explosion will do something quite different. The force of gravity overcomes the nuclear forces which keep protons and neutrons from combining. The core is thus swallowed by its own gravity. It has now become a black hole which readily attracts any matter and energy that comes near it.

Why supernova explosion occurs in high mass stars?

Once stars that are 5 times or more massive than our Sun reach the red giant phase, their core temperature increases as carbon atoms are formed from the fusion of helium atoms. Gravity continues to pull carbon atoms together as the temperature increases and additional fusion processes proceed, forming oxygen, nitrogen, and eventually iron.

When the core contains essentially just iron, fusion in the core ceases. This is because iron is the most compact and stable of all the elements. It takes more energy to break up the iron nucleus than that of any other element. Creating heavier elements through fusing of iron thus requires an input of energy rather than the release of energy.

Since energy is no longer being radiated from the core, in less than a second, the star begins the final phase of gravitational collapse. The core temperature rises to over 100 billion degrees as the iron atoms are crushed together. The repulsive force between the nuclei overcomes the force of gravity, and the core recoils out from the heart of the star in a shock wave, which we see as a supernova explosion.

What is supernova remnant?

As the shock encounters material in the star’s outer layers, the material is heated, fusing to form new elements and radioactive isotopes.

While many of the more common elements are made through nuclear fusion in the cores of stars, it takes the unstable conditions of the supernova explosion to form many of the heavier elements. The shock wave propels this material out into space. The material that is exploded away from the star is now known as a supernova remnant.

The hot material, the radioactive isotopes, as well as the leftover core of the exploded star, produce X-rays and gamma-rays.

For furthur information: External link: https://en.wikipedia.org/wiki/Stellar_evolution

PRACTICE QUESTIONS

QUES . Consider the following statements: UPSC 2024

Statement-I:

Giant stars live much longer than dwarf stars.

Statement-II:

Compared to dwarf stars, giant stars have a greater rate of nuclear reactions.

Which one of the following is correct in respect of the above statements?

(a) Both Statement-I and Statement-II are correct and Statement-II explains Statement-I

(b) Both Statement-I and Statement-II are correct, but Statement-II does not explain Statement-I

(c) Statement-I is correct, but Statement-II is incorrect

(d) Statement-I is incorrect, but Statement-II is correct

Show Answer