The primary factor that prevents the Sun's gravity from pulling the planets directly towards it is **the planets' speed**.
As planets orbit the Sun, they have a tangential velocity due to their orbit. This means that instead of falling directly into the Sun, they continuously move forward while being pulled by the Sun's gravitational force. The balance between the gravitational pull of the Sun and the inertia of the planets (their speed) results in stable orbits. If a planet's speed were to decrease significantly, it could spiral in towards the Sun, but under normal conditions, the combination of speed and gravitational attraction allows for stable orbits.
The other options, while they may play a role in the dynamics of the solar system, are not the primary reason for the stability of planetary orbits. The Sun’s gravity is strong enough to keep the planets in orbit, and the large distances between the planets and the Sun, while influencing gravitational interactions, do not significantly counteract the effects of gravity itself.