MadSci Network: Astronomy |
Indeed Jupiter's colors are flesh-toned to red in color, reflecting the chemical compositions of the atmospheric layers. However, the disk of Jupiter also shows bands of white, blue, and yellow clouds, also reflecting the various chemical compounds formed there. The alternating strips of light and dark regions that run parallel to the equator are called zones and belts. Infrared (IR) observations show that the zones have lower temperatures than the belts, and the differences in temperature imply that the zones mark the tops of rising regions of high pressure, while the belts mark the descending regions of low pressure. The temperature variations also have some influence over the colors we see. Lightning does occur on Jupiter and the photons (hv)[hv - h times nu is the energy of the photon] that result do influence chemical reactions. Some examples are as follows: Making water (H2O): O + hv -> O+ +e- O+ + H2 -> OH+ + H OH+ + H2 -> H2O+ + H H2O+ + H2 -> H3O+ + H and recombination causes H3O+ + e- -> H2O + H Making ammonia (NH3): N + hv -> N+ + e- N+ + H2 -> NH+ + H NH+ + H2 -> NH2+ + H NH2+ + H2 -> NH3+ + H NH3+ + H2 -> NH4+ + H and recombinatins causes NH4+ + e- -> NH3 + H Methane (CH4) can be made in much the same way, starting with C + hv -> C+ + e- IR analyses show that the atmosphere consists of methane, ammonia, molecular hydrogen (H2), and helium (He). Acetylene, ethane, phosphine, water, and germane have also been detected. By mass, Jupiter's atmosphere contains 78% hydrogen, 20% helium, and 2% all other elements, essentially the composition of the Sun. The Red Spot is a few degrees cooler than the surrounding zone and a rising region of high pressure. Its color probably results from chemical reactions of major and trace molecules, with photoionization (hv) and dissociation driving the reactions to make hydrocarbons that provide the coloration. Reference: Astronomy and Astrophysics (Zeilik and Gregory, 199) and notes from RPI's Origins of Life Course.
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