Belts and Zones
Atmospheric flows are forced into belts and zones
Jupiter's rapid rotation affects the planet by making it wider at the equator than at the poles. It also affects it by giving the planet its cloud bands.
The relatively pronounced bulge is due to, Jupiter's rapid rotation rate of 9 hrs 56 mins, and Saturns 10hrs 32. As the planets are made of gas this high speed rotation pushes out the gas at the equator.
C) a large impact early in Earth's development.
Saturn's rotation causes its oblate shape. During rotation, Saturn is flattened at the poles and bulges in the middle. Saturn is the sixth planet from the sun and the second largest in the solar system.
The belts and zones of Jupiter result from the planet's convetion and it's rapid differential rotation.
Atmospheric flows are forced into belts and zones
Jupiter's rapid rotation affects the planet by making it wider at the equator than at the poles. It also affects it by giving the planet its cloud bands.
The rapid rotation of Saturn flattens it at the poles by about 10%, making it the most oblate planet.
The relatively pronounced bulge is due to, Jupiter's rapid rotation rate of 9 hrs 56 mins, and Saturns 10hrs 32. As the planets are made of gas this high speed rotation pushes out the gas at the equator.
A whole buttload of hot metal moving fast in the core of the planet. ****************************************************************** Here's a better answer: - Rapid rotation, and liquid conducting interior- electric charges move about= Strong magnetic field --You are welcome! - Hershey
It has a rapid rotation of 10.6 hours.
No. Like most other planets Saturn is what is called an oblate spheroid, meaning it is slightly wider across the equator than it is from pole to pole. This is due to its rotation. Because of its low density and rapid rotation Saturn is the most oblate planet in the solar system.
rapid rotation
It has a rapid rotation of 10.6 hours.
rapid rotation. A.K.A penis jerkin.
Jupiter's rapid rotation rate causes its equator to bulge out and its poles to be flattened. It looks a bit like a squashed ball; the planet is seven percent larger at the equator than at the poles.