Nearly all the oxygen present is combined chemically with hydrogen to form water (H 2O). Uranus and Neptune were less efficient at attracting hydrogen and helium gas, so they have much smaller atmospheres in proportion to their cores.Ĭhemically, each giant planet is dominated by hydrogen and its many compounds. Uranus and Neptune are much smaller than Jupiter and Saturn, but each also has a core of rock, metal, and ice. We must infer the existence of the denser core inside these planets from studies of each planet’s gravity. In fact, when we look down from above, all we see is the atmosphere with its swirling clouds (Figure 1). Both Jupiter and Saturn, therefore, have cores composed of heavier rock, metal, and ice, but we cannot see these regions directly. Under the force of gravity, the heavier elements sink toward the inner parts of a liquid or gaseous planet. (credit: modification of work by NASA/JPL/University of Arizona) This true-color image of Jupiter was taken from the Cassini spacecraft in 2000. Because the bulk of both planets consists of compressed, liquefied hydrogen, we should really call them liquid planets.įigure 1: Jupiter. Jupiter and Saturn are so large that the gas is compressed in their interior until the hydrogen becomes a liquid.
On Earth, both hydrogen and helium are gases, so Jupiter and Saturn are sometimes called gas planets. The two largest planets, Jupiter and Saturn, have nearly the same chemical makeup as the Sun they are composed primarily of the two elements hydrogen and helium, with 75% of their mass being hydrogen and 25% helium. Certainly their compositions are dominated by different elements. The fact that there are two distinct kinds of planets-the rocky terrestrial planets and the gas-rich jovian planets-leads us to believe that they formed under different conditions. Explain why there is geological activity on some planets and not on others.Explain what influences the temperature of a planet’s surface.
Describe the characteristics of the giant planets, terrestrial planets, and small bodies in the solar system.By the end of this section, you will be able to:
0 kommentar(er)
