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The greater the distance, the longer is the orbital period and the slower the velocity.

"Kepler's Laws of Planetary Motion" contain mathematical details.

Further explanation is given by the work of Isaac newton and his theory of

gravitation.

For example, one version of Kepler's 3rd law is :

The square of the orbital period (in Earth years) equals the cube of the average distance from the Sun (in Astronomical Units).

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The second half of the question can be answered from the above formula.

For example, a planet at four times the distance of Earth from the Sun would go round the Sun in eight years.

The length of that orbit would be (almost exactly) four times as far as Earth's.

So, the planet would travel at half the speed of Earth.

In this example, and also generally, the orbital speed is inversely proportional to the square root of the average distance from the Sun.

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Q: How does the distance from the sun impact the orbital period and velocity of a planet?
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