The solar system, which formed approximately 4.6 billion years ago, originated from a vast gas cloud. The collapse of the gas cloud's interior led to a gradual increase in density, ultimately resulting in the formation of the Sun. As gravity took effect, the material surrounding the Sun began to gather, giving rise to planetary systems and various celestial bodies.

The solar system consists of eight major planets, namely Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. These planets are arranged in order of their distance from the Sun.

In most cases, the rotation of these planets aligns with their revolution, except for Venus and Uranus. Venus rotates in the opposite direction to its revolution, while Uranus rotates at a unique 97° angle to its orbit.

At the center of the solar system lies the Sun, exerting its gravitational pull on all celestial bodies within its vicinity. Most celestial bodies near the Sun follow a similar orbital plane, while those located farther away deviate from this plane as they revolve around the Sun.

Apart from the planets, the solar system also harbors a fascinating region known as the "Kuiper Belt." This belt-like expanse extends beyond the orbit of Neptune and comprises numerous icy small bodies, comets, and other objects.

Scientists hypothesize that the Kuiper Belt might contain remnants from the early stages of planet formation within the solar system.

In addition to its internal components, the solar system interacts with other galaxies and interstellar space. For instance, gravitational interactions can propel comets out of the solar system and into interstellar space. Moreover, interstellar objects like dust clouds and gas clouds can make their way into the solar system, establishing further interactions.

Notably, each planet within the solar system possesses its own set of satellites. Jupiter, for instance, boasts a multitude of moons, with the four largest known as the Galilean moons, discovered by Galileo in the 17th century.

Saturn also possesses numerous moons, among which Titan garners considerable attention due to its potential icy oceans that may harbor liquid water.

The solar system has long served as a primary target for human space exploration. Throughout the 20th century, unmanned probes were successfully dispatched to various celestial bodies within the solar system to conduct exploration missions.

The renowned US Voyager and Pioneer missions, along with the recent New Horizons mission, have provided us with invaluable data and images of objects within our solar system.

Despite the growing body of knowledge we have acquired, numerous uncharted territories within the solar system beckon further exploration.

Are there undiscovered planets or dwarf planets lingering within our system? What other enigmatic icy objects reside in the Kuiper Belt? How can we gain a deeper understanding of the solar system's formation and evolution? These pressing questions continue to captivate scientists and drive the advancement of solar system exploration.

As our quest for knowledge persists, mankind remains committed to unraveling the mysteries of the solar system. With each new discovery, we inch closer to comprehending our cosmic neighborhood and expanding our understanding of the universe at large.