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  1. en.wikipedia.org › wiki › StarStar - Wikipedia

    A star is a luminous spheroid of plasma held together by self-gravity. 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.

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  2. A simple chart for classifying the main star types using Harvard classification. In astronomy, stellar classification is the classification of stars based on their spectral characteristics.

  3. Astronomers think there is a very large number of stars in the Universe. The observable Universe contains more than 2 trillion (10 12) galaxies [2] and, overall, as many as an estimated 1 × 1024 stars [3] [4] (more stars than all the grains of sand on planet Earth ). [5]

  4. Nuclear fusion powers a star for most of its existence. Initially the energy is generated by the fusion of hydrogen atoms at the core of the main-sequence star. Later, as the preponderance of atoms at the core becomes helium, stars like the Sun begin to fuse hydrogen along a spherical shell surrounding the core.

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