The condensation sequence cannot explain the composition of the terrestrial and Jovian planets.

Question

Quizplus · Accepted Answer

The condensation sequence is responsible for the composition of the terrestrial and Jovian planets. As the solar nebula cooled, different materials condensed into solid particles at different distances from the Sun. At the inner edge, only the most refractory materials, such as metals and silicates, condensed into solid particles, which eventually formed the rocky, terrestrial planets. On the outer edge, volatile materials such as water, ammonia, and methane also condensed into solid particles, which eventually formed the Jovian planets.

The Condensation Sequence Cannot Explain the Composition of the Terrestrial