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  1. en.wikipedia.org › wiki › Star_systemStar system - Wikipedia

    A star system or stellar system is a small number of stars that orbit each other, [1] bound by gravitational attraction. A large group of stars bound by gravitation is generally called a star cluster or galaxy, although, broadly speaking, they are also star systems.

  2. 3 Οκτ 2024 · 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.

  3. science.nasa.gov › universe › starsStars - Science@NASA

    Astronomers estimate that the universe could contain up to one septillion stars – that’s a one followed by 24 zeros. Our Milky Way alone contains more than 100 billion, including our most well-studied star, the Sun. Stars are giant balls of hot gas – mostly hydrogen, with some helium and small amounts of other elements.

  4. 20 Μαρ 2019 · Stars are huge celestial bodies made mostly of hydrogen and helium that produce light and heat from the churning nuclear forges inside their cores. Aside from our sun, the dots of light we see in...

  5. A star system is a group of stars held together by gravity. These systems can have from 2 stars to many stars. The most common type is a binary star system, where two stars move around each other. Physical double stars are another name for binary systems that are truly connected by gravity.

  6. en.wikipedia.org › wiki › StarStar - 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.

  7. Stars are classified by color and temperature: O (blue), B (bluish white), A (white), F (yellowish white), G (yellow), K (orange), and M (red), from hottest to coolest. Stars form from nebulas. Gravity causes stars to collapse until nuclear fusion begins. Stars spend most of their lives on the main sequence, fusing hydrogen into helium.

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