The Solar System, our cosmic home, is a fascinating tapestry woven by gravity's threads. At its heart, the Sun, a luminous G-type main-sequence star, burns with the fire of nuclear fusion. Born from the collapse of a dense molecular cloud some 4.6 billion years ago, the Sun and its protoplanetary disk gave rise to the diverse worlds that dance to its tune. The Sun's core is a crucible where hydrogen transmutes into helium, while its photosphere radiates this energy outward.