Volume increases with the Cube of the radius, so an easy way to compute the volume of the giant planet is to simply take the ratio of the radius Giant Planet: Earth and raise it to the 3rd power.
Since these planets are the same shape (Spherical) this ratio is accurate enough for our purposes. In the case of an object that is oblate (like Saturn or Jupiter), one can still calculate the volume accurately by taking the Equatorial Radius squared and multiplying it by the Polar Radius.
In this given case the volume of Giant Planet = 14 x 14 x 14, or 2,744x that of Earth.
Since Mass = 681x that of Earth, Density = 681/2744 = 0.248 of Earth's (just a little under one quarter).
You could go one step further to calculate the density of this object by multiplying the density ratio by Earth's density (5.515x water) - so Giant Planet's density = 1.369 grams/cm3.
Saturn:)Saturn is the least dense of the gas giants, even out of all of the planets in our solar system. Its average density is around 0.7 g/cc (less than water)
The average density of Jovian (gas giant) planets like Jupiter and Saturn is low compared to terrestrial planets like Earth. Their densities are around 1-2 grams per cubic centimeter due to being primarily composed of hydrogen and helium gases with small rocky cores.
The density of water in terrestrial depends on many different factors. The density can only be determined based on the planet's history, they may have "water", but there could be other things inside. Also the gravity of the planet play a role of the density of the water.
It is said that if you could find an ocean on Earth large enough to accommodate it, Saturn would float. That is, Saturn's average density is less than the density of water. Turns out it's the only planet with an average density less than 1.000, that is, less than the density of water.
The planet density chart provides information about the relative densities of different planets in our solar system. By comparing the densities of the planets, we can understand their composition and internal structure. Planets with higher densities are likely to have more solid materials, while planets with lower densities may have more gases or lighter materials. This information can help scientists learn more about the formation and evolution of planets.
No. Terrestrial planets are much denser than Jovian planets.
The Earth has the greatest average density, of all the planets.
The density of a planet depends basically on the density of the materials that make the planet up. It is a weighted average of those densities.
Mars is the least dense of the rocky planets.
Average density of the planet
Earth's average density is about 5.52 grams per cubic centimeter. This density is determined by the distribution of material in Earth's layers, with the denser iron-nickel core contributing to the overall value. Earth's density is higher than that of most other planets in our solar system.
Saturn, with an average density of 0.7 g/cc.
Saturn:)Saturn is the least dense of the gas giants, even out of all of the planets in our solar system. Its average density is around 0.7 g/cc (less than water)
Mercury is the smallest of the four inner planets and closest to the sun. It is also the smallest of all eight planets.
The average density of Jovian (gas giant) planets like Jupiter and Saturn is low compared to terrestrial planets like Earth. Their densities are around 1-2 grams per cubic centimeter due to being primarily composed of hydrogen and helium gases with small rocky cores.
Neptune is the outermost planet, and is farthest from Earth's orbit.
The density of water in terrestrial depends on many different factors. The density can only be determined based on the planet's history, they may have "water", but there could be other things inside. Also the gravity of the planet play a role of the density of the water.