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Question: Discuss the Implications of these Auroral Observations particularly from the perspective of the Planetary Interior Structure. Given the Jovian nature of this planet, what other Observable Characteristics might you see? Answer: Planets in the Solar system are mainly classified into two types, namely the Jovian planets and the terrestrial planets. Beyond the frost line of our solar system, the region where volatile materials such as water, methane and ammonia begin to freeze, the Jovian planets such as Jupiter, Saturn, Uranus and Neptune reside (Heller Pudritz, 2015). These planets differ in characteristics, in size, composition and mass. The auroral observations that are seen, results from the structure and composition of these planets. These planets are primarily composed of gases such as hydrogen and helium. The remaining portions are occupied by heavy metallic elements and a molten core that is composed of rocky substances. These compositional differences, from the terrestrial planets, results in the development of the auroral activities of the Jovian planets (Heller Pudritz, 2015). These planets experience auroras near the northern and southern poles. This results from an intense radiation, the magnetic field of the planet, along with the abundance of materials from los volcanoes, which has a strong reaction with the ionosphere of the Jovian planet. These planets also experience violent weather patterns that increase the auroral activities (Mankovich et al., 2015). The storms form within hours and become thousands of kilometres in diameters overnight. These are some of the causes of the frequent auroral activiti es of the Jovian planets. The winds of the Saturn are the second fastest in the Solar system. The southern and the northern poles highlight the fact that the planet has been experiencing stormy weather. Thus, the weather conditions of the Jovian planets, along with the composition of the planets result in the auroral activities. References Heller, R., Pudritz, R. (2015). Water ice lines and the formation of giant moons around super-Jovian planets. The Astrophysical Journal, 806(2), 181. Mankovich, C., Fortney, J. J., Moore, K. L., Nettelmann, N. (2015). Helium Rain and the Thermal Evolution of the Jovian Planets. In AAS/Division for Planetary Sciences Meeting Abstracts (Vol. 47).