The Earth orbits the sun due to gravitational forces and the conservation of angular momentum from the solar system's formation. If the Earth were stationary, it would eventually fall into the sun due to gravity, but its tangential velocity allows it to maintain a stable orbit. The Earth is constantly accelerating toward the sun, yet its sideways motion keeps it from colliding with it. Over extremely long timescales, gravitational interactions with other celestial bodies could potentially alter Earth's orbit, but current models suggest stability for billions of years. Understanding these dynamics helps clarify why the Earth does not simply remain in one place.