Answer:
Lesser
Step-by-step explanation:
The gravitational pull between a planet orbiting the Sun and the Sun is equal to the centripetal force keeping the planet in circular motion:

where
 is the gravitational constant
 is the gravitational constant
 is the mass of the Sun
 is the mass of the Sun
 is the mass of the planet
 is the mass of the planet
 is the distance between the Sun and the planet
 is the distance between the Sun and the planet
v is the orbital velocity of the planet
We can re-arrange the formula to solve for v, the orbital velocity of the planet:

We see that the velocity is inversely proportional to the square root of the distance, r: therefore, the farther the planet from the Sun, the lesser the orbital velocity of the planet.