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Every star has its own life cycle, ranging from a few million to trillions of years, and its properties change as it ages Some types change into others very quickly, while others stay relatively unchanged over trillions of years. Stars form in large clouds of gas and dust called molecular clouds.

Historically, stars have been important to civilizations throughout the world The universe’s stars range in brightness, size, color, and behavior They have been part of religious practices, divination rituals, mythology, used for celestial navigation and orientation, to mark the passage of seasons, and to define calendars.

This article describes the properties and evolution of individual stars

Included in the discussion are the sizes, energetics, temperatures, masses, and chemical compositions of stars. Stars are huge celestial bodies made mostly of hydrogen and helium that produce light and heat from the churning nuclear forges inside their cores. Stars are spherical balls of hot, ionized gas (plasma) held together by their own gravity Stars are the most fundamental building blocks of our universe.

A star is a massive, luminous sphere of plasma held together by gravity The nearest star to earth is the sun, which is the source of most of the energy on the planet. Stars are massive, luminous spheres of gas, mainly composed of hydrogen, with smaller amounts of helium and other elements The lifespan of a star varies widely, generally ranging from several million to several trillion years.

Below are lists of the largest stars currently known, ordered by radius and separated into categories by galaxy

The unit of measurement used is the radius of the sun (approximately 695,700 km [1] the sun, the orbit of earth, jupiter, and neptune, compared to four stars (pistol star, rho cassiopeiae, betelgeuse, and vy canis majoris)

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