Saturn's day is about 10 and one half hours. This rapid rotation makes the largest polar flattening among the planets.
No. All of the meridians merge in a single point at the poles.
The North and South poles
Answer:To a first-order approximation the Earth is round. Thisis due to gravity. Gravity pulls with equal strength in alldirections; therefore any variations from a sphericalshape will lead to gravitational forces thatbring the shape back into that of a sphere.This is without considering the rotation of the earth,however. The rotation of the earth adds centrifugaleffects, which cause the earth to bulge slightly atits equator and flatten slightly at its poles.(This is like twirling a rock on the end of a stringand then letting go--the rock flies away from thetwirler.) Because of these centrifugal effects, thedistance from the center of the earth to the surfaceof the earth is about 0.33% shorter at the polescompared to the equator.
That depends on your latitude. Near the equator, the days will hardly get longer or shorter; the nearer you get to the poles, the greater the difference will be.That depends on your latitude. Near the equator, the days will hardly get longer or shorter; the nearer you get to the poles, the greater the difference will be.That depends on your latitude. Near the equator, the days will hardly get longer or shorter; the nearer you get to the poles, the greater the difference will be.That depends on your latitude. Near the equator, the days will hardly get longer or shorter; the nearer you get to the poles, the greater the difference will be.
No, it slightly bulges at the equator, and is a bit flat on the North and South Poles.
Saturn has the greatest polar flattening of any planet in our solar system. Its oblateness, or polar flattening, is due to its rapid rotation, causing it to bulge at the equator and flatten at the poles.
Several planets are flattened at the poles. That just means the distance between the poles is less than diameter of the planet at the equator. Saturn is the most extreme example in our solar system, followed by Jupiter. Even the Earth is slightly flattened at the poles. Astronomers call this "oblateness".
The rapid rotation of Saturn flattens it at the poles by about 10%, making it the most oblate planet.
Jupiter is the planet with flattened poles due to its rapid rotation. This fast rotation causes the planet to bulge at its equator and flatten at the poles.
The planet that is known for its flat shape due to very fast rotation is Saturn. Its rapid rotation causes it to bulge at the equator and flatten at the poles, giving it a distinctive oblate spheroid shape.
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.
Yes, the Earth is approximately spherical in shape. It is not a perfect sphere due to its rotation, which causes it to bulge slightly at the equator and flatten at the poles.
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.
The spinning motion of the Earth causes it to flatten slightly at the poles and bulge at the equator. This flattening, known as oblateness, is a result of the centrifugal force counteracting the gravitational force at the equator. The shape of the Earth is an oblate spheroid due to this flattening.
Saturn is not perfectly spherical due to its fast rotation causing it to bulge at the equator. However, it is not shaped like a pear either. The overall shape of Saturn is best described as an oblate spheroid, where it is slightly flattened at the poles and bulging at the equator.
Yes and no. They are round, but not perfectly spherical. For example, the Earth has a slight bulge around the equator. Jupiter and Saturn have more obvious bulges. Saturn in particular is flattened at its poles compared with its equator. Also, of course, the surfaces of the planets are not perfectly smooth.
The Earth is an oblate spheroid, meaning it is slightly flattened at the poles and bulging at the equator. This bulging at the equator results in a greater equatorial distance compared to the polar distance. This is due to the centrifugal force generated by the Earth's rotation, which causes the equatorial regions to bulge outwards.