Exploring Extraterrestrial Life: Perspectives from the Realm of Astrobiology [Telugu]

By Neha Chatterjee

Oceans of stars, galaxies dancing, the birth and death of stars - A visit to the universe

The universe is a wondrous place. It is filled with oceans of stars, galaxies dancing with each other, and stars being born and dying. We are constantly learning new things to try to understand this world and find our place in it.

Oceans of stars

There are billions of trillions of stars in the universe. They come in all shapes and sizes, but they are all made of the same basic materials: hydrogen and helium.

Stars are born in large clouds of hydrogen and helium gas. This gas gradually collapses inward under the force of gravity. In the center, the gas becomes very hot and dense, which triggers the nuclear fusion process.

Nuclear fusion is the process of two or more hydrogen atoms fusing together to form a helium atom. This process releases a tremendous amount of energy, which powers the stars.

Stars go through different stages in their lives. The first stage of their life is called the main sequence. In this stage, stars continue to convert hydrogen into helium.

After the main sequence ends, stars enter their final stages of life. These stages can be classified as supernovae, red dwarfs, or black holes.

Galaxies dancing

Galaxies are large collections of stars, gas, and dust. They are held together by gravity. There are billions of galaxies in the universe.

Galaxies come in all shapes and sizes. The Milky Way galaxy is a spiral galaxy. It is home to our solar system.

Galaxies are constantly moving and interacting with each other. They can collide, merge, or even form new galaxies.

The birth of stars

Stars are born in large clouds of gas and dust. These clouds are called nebulae. Nebulae are often very beautiful and colorful.

The process of star formation begins when a cloud of gas and dust begins to collapse under the force of gravity. As the cloud collapses, it becomes hotter and denser.

At the center of the cloud, the temperature and pressure become so high that nuclear fusion begins. This is the process that powers stars.

The death of stars

Stars eventually die. The way a star dies depends on its mass.

Low-mass stars, like our Sun, will eventually become red dwarfs. Red dwarfs are very dim and cool stars that will eventually fade away.

• Format: Paperback
• Language: Telugu
• ISBN: B0CRPLNLCY
• ISBN13: 9798869079824
• Release Date: December 2023
• Publisher: Sunshine
• Length: 82 Pages
• Weight: 0.27 lbs.
• Dimensions: 0.2" x 6.0" x 9.0"