A star is a luminous spheroid of plasma held together by self-gravity. [1] The nearest star to Earth is the Sun. Many other stars are visible to the naked eye at night; 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. Astronomers have ...

Star, any massive self-luminous celestial body of gas that shines by radiation derived from its internal energy sources. 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.

Variable stars, such as Cepheid variables, change in brightness over time due to internal pulsations or interactions with companion stars. These stars have been vital for measuring cosmic distances and understanding the expansion of the universe. Fascinating Star Facts The Sun makes up 99.8% of the mass in our solar system.

Explore seven major types of stars — from tiny red dwarfs to massive blue supergiants — and learn their defining traits, lifecycles, sizes, temperatures, and common examples. This hub summarizes key…

Stars 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. According to NASA, astronomers estimate there could be as many as one septillion stars in the universe, which is a one with 24 zeros after it. Within our galaxy ...