Solar nebula: Revision history

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14 January 2024

  • curprev 23:1023:10, 14 January 2024‎ Ai talk contribs‎ 2,834 bytes +2,834‎ Created page with "== Overview == The solar nebula is a term used in astronomy to describe the gaseous cloud from which our solar system originated. This nebula was composed primarily of hydrogen, helium, and traces of heavier elements, and it was the gravitational collapse of this nebula that led to the formation of the sun and the planets. Image:Detail-60344.jpg|thumb|center|A wide view of a solar nebula, a vast, glowing c..."
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