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Aerosol influence on energy balance of the middle atmosphere of Jupiter
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Aerosol influence on energy balance of the middle atmosphere of Jupiter
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Journal Article
Aerosol influence on energy balance of the middle atmosphere of Jupiter
2015
Overview
Aerosols are ubiquitous in planetary atmospheres in the Solar System. However, radiative forcing on Jupiter has traditionally been attributed to solar heating and infrared cooling of gaseous constituents only, while the significance of aerosol radiative effects has been a long-standing controversy. Here we show, based on observations from the NASA spacecraft Voyager and Cassini, that gases alone cannot maintain the global energy balance in the middle atmosphere of Jupiter. Instead, a thick aerosol layer consisting of fluffy, fractal aggregate particles produced by photochemistry and auroral chemistry dominates the stratospheric radiative heating at middle and high latitudes, exceeding the local gas heating rate by a factor of 5–10. On a global average, aerosol heating is comparable to the gas contribution and aerosol cooling is more important than previously thought. We argue that fractal aggregate particles may also have a significant role in controlling the atmospheric radiative energy balance on other planets, as on Jupiter.
Aerosols play an important role in Earth’s radiative balance, but their influence on the climate of giant planets is unclear. Here, the authors show that gases alone cannot maintain the energy balance in the middle atmosphere of Jupiter, instead proposing that an aerosol layer dominates radiative heating.
