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 mass of the Sun
is the mass of 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.