G2V star
The Sun holds 99.86% of the Solar System’s mass.
Its core reaches about 15 million degrees Celsius, where hydrogen fuses into helium, powering its energy output.
Its light takes about 8 minutes and 20 seconds to reach Earth from 150 million kilometers away.
It is about 4.6 billion years old and roughly halfway through its life - in about 5 billion years it will swell into a red giant.
Its visible surface (photosphere) is around 5,500°C, while the outer atmosphere, the corona, is paradoxically far hotter, reaching millions of degrees.
Its activity follows a roughly 11-year cycle, reflected in the number of sunspots and space-weather events.
Its chemical composition is about 74% hydrogen and 24% helium, with trace amounts of heavier elements.
Its diameter is about 1.39 million km, roughly 109 times Earth's, with a volume that could hold about 1.3 million Earths.
It holds 99.86% of the Solar System's total mass; the planets, moons and everything else make up only the remaining fraction.
Its solar flares and coronal mass ejections can disrupt satellites and power grids on Earth.
It rotates once roughly every 25-35 days, with the rate varying by latitude (differential rotation).
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