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  • Star - Wikipedia
    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
  • Stars - NASA Science
    A star’s gas provides its fuel, and its mass determines how rapidly it runs through its supply, with lower-mass stars burning longer, dimmer, and cooler than very massive stars
  • Star | Definition, Light, Names, Facts | Britannica
    A star is any massive self-luminous celestial body of gas that shines by radiation derived from its internal energy sources Of the tens of billions of trillions of stars in the observable universe, only a very small percentage are visible to the naked eye
  • What Is a Star and How Does It Work? - ThoughtCo
    How does a star work? How do they form, live, and eventually die? Learn more about these distant objects and their major importance in the universe
  • Life Cycle of a Star: Stages, Facts, and Diagrams
    A star is a giant sphere of extremely hot, luminous gas (mostly hydrogen and helium) held together by gravity A few examples of well-known stars are Pollux, Sirius, Vega, Polaris, and our own Sun Stars are essentially the building blocks of galaxies and are the source of all the heavier elements
  • Types of Stars | Stellar Classification, Lifecycle, and Charts
    Here is some information about each type of known star in our universe Below, is a simple star color temperature chart that provides examples of some of the most well-known stars in the night sky, and their colors Protostar: A protostar is what you have before a star forms
  • Stars—facts and information | National Geographic
    These large, swelling stars are known as red giants But there are different ways a star’s life can end, and its fate depends on how massive the star is
  • Star Facts - Interesting Facts about Stars
    Star birth can take millions of years and create families of stars Astronomers see examples of star formation in nebulae throughout our own Milky Way Galaxy and in many other galaxies


















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