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๐Ÿ”† Sun

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๐Ÿ“Œ Type: G2V star, commonly called a yellow dwarf.
๐Ÿ“Œ Age: Approximately 4.6 billion years.
๐Ÿ“Œ Diameter: Approximately 1.39 million kilometres.
๐Ÿ“Œ Mass: Approximately 333,000 times the mass of Earth.
๐Ÿ“Œ Distance from Earth: Approximately 150 million kilometres.
๐Ÿ“Œ Temperature at visible surface: Approximately 5,500ยฐC.
๐Ÿ“Œ Core temperature: Approximately 15 millionยฐC.
๐Ÿ“Œ Composition: Primarily hydrogen (about 73% by mass) and helium (about 25%), with small amounts of heavier elements.
๐Ÿ“Œ Gravity: Approximately 28 times Earthโ€™s surface gravity.
๐Ÿ‘‰ Remarkable fact: More than 1.3 million Earths could fit inside the Sun by volume!

The Sun produces energy through a process called nuclear fusion.

๐Ÿ“Œ Its enormous gravitational pressure compresses hydrogen in its core.
๐Ÿ“Œ Hydrogen nuclei combine to form helium.
๐Ÿ“Œ A small amount of mass is converted into enormous amounts of energy.
๐Ÿ“Œ This energy eventually escapes into space as light and other electromagnetic radiation.
๐Ÿ“Œ That energy travels approximately 150 million kilometres to reach Earth in just over 8 minutes.
๐Ÿ‘‰ Remarkable fact: The Sun converts approximately 600 million tonnes of hydrogen into helium every second. Around 4 million tonnes of mass are converted into energy every second.