General

Astronomy

  1. 1. Introduction to Astronomy
  2. Legacy Course

  3. Introduction to Astronomy
  4. History of Astronomy
  5. Fundamentals of Astronomy
  6. The Solar System
  7. The Moon and Planetary Science
  8. Stars and Stellar Evolution
  9. Galaxies and the Universe
  10. Cosmology and the Early Universe
  11. Observing the Sky
  12. Future of Astronomy
  13. Careers in Astronomy

The Sun

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Learning

The Sun is a medium-sized star located at the center of the Solar System. It is the primary source of energy for the Solar System, and is responsible for providing the light and heat that makes life on Earth possible. The Sun has a mass of about \(1.989\times10^{30}\) kilograms and a radius of about 695,800 kilometers, making it about 330,000 times more massive than the Earth.

File:Sun poster.svg

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The Sun is composed primarily of hydrogen and helium, with smaller amounts of heavier elements such as carbon, nitrogen, and oxygen. To illustrate this, the Sun's energy is produced through the process of nuclear fusion, which occurs in the core of the Sun. In this process, hydrogen atoms are combined to form helium, releasing vast amounts of energy in the process. The energy produced by the Sun is released into space in the form of electromagnetic radiation, including visible light, ultraviolet radiation, and infrared radiation.

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