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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 Stars are the most fundamental building blocks of our universe. Stars form in large clouds of gas and dust called molecular clouds.
Many other stars are visible to the naked eye at night Stars are spherical balls of hot, ionized gas (plasma) held together by their own gravity Their immense distances from earth make them appear as fixed points of light
The most prominent stars have been categorised into constellations and asterisms, and many of the brightest stars have proper names.
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 a fundamental component in the universe and collectively form star clusters, galaxies and galaxy clusters Find out more about star names, star clusters to see with the naked eye, how to photograph stars and the science of stardust.
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. Stars are huge celestial bodies made mostly of hydrogen and helium that produce light and heat from the churning nuclear forges inside their cores.
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