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  1. science.nasa.gov › universe › starsStars - NASA Science

    Stars are giant balls of hot gas – mostly hydrogen, with some helium and small amounts of other elements. Every star has its own life cycle, ranging from a few million to trillions of years, and its properties change as it ages.

  2. 12 de abr. de 2024 · star, 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 composing the observable universe, only a very small percentage are visible to the naked eye. Many stars occur in pairs, multiple systems, or star clusters.

  3. 20 de mar. de 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.

  4. Únete al programa de lealtad PlayStation Stars y empieza a ganar puntos para canjearlos por coleccionables digitales exclusivos de PlayStation, crédito de PS Store y mucho más. Escanéalo para unirte a PlayStation Stars o inicia sesión en PlayStation App.

  5. Discover the wonders of the night sky with NASA's interactive skymap. Learn about stars, planets, constellations and more with a click of your mouse.

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

    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.

  7. 15 de jul. de 2014 · A star is a luminous ball of gas, mostly hydrogen and helium, held together by its own gravity. Nuclear fusion reactions in its core support the star against gravity and produce photons and heat, as well as small amounts of heavier elements. The Sun is the closest star to Earth.

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