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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 In astronomy, we measure the brightness of stars in different ways. Stars form in large clouds of gas and dust called molecular clouds.
Many other stars are visible to the naked eye at night After forming, they go through several stages which we call the life cycle of a star 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 huge celestial bodies made mostly of hydrogen and helium that produce light and heat from the churning nuclear forges inside their cores. 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. 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 spherical balls of hot, ionized gas (plasma) held together by their own gravity
Stars are the most fundamental building blocks of our universe.
Stars are huge balls of hot, glowing gas that make light and heat through fusion Stars come in different sizes and colors, and each one has a life cycle like our sun As stars die, they spread elements in space that help make new stars, planets, and life. Stars shine for many millions of years, but do not last for ever
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