About this document
Understanding the Sun: A Scientific Overview by denisardiansa49 is a document available to read on EtoBox.
The Sun is a G main sequence star at the center of the Solar System, composed mainly of hydrogen and helium, with a diameter of about 1.39 million km. It formed approximately 4.6 billion years ago and generates energy through nuclear fusion, fusing 620 million metric tons of hydrogen every second. The Sun orbits the Milky Way galaxy and significantly influences Earth
- Author
- denisardiansa49
- Language
- EN