Astronomy and Astrophysics – Astronomy
Scientific paper
May 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000apj...534l.215w&link_type=abstract
The Astrophysical Journal, Volume 534, Issue 2, pp. L215-L217.
Astronomy and Astrophysics
Astronomy
31
Planets And Satellites: Individual: Jupiter
Scientific paper
Aromatic compounds have been considered a likely candidate for enhanced aerosol formation in the polar region of Jupiter. We develop a new chemical model for aromatic compounds in the Jovian auroral thermosphere/ionosphere. The model is based on a previous model for hydrocarbon chemistry in the Jovian atmosphere and is constrained by observations from Voyager, Galileo, and the Infrared Space Observatory. Precipitation of energetic electrons provides the major energy source for the production of benzene and other heavier aromatic hydrocarbons. The maximum mixing ratio of benzene in the polar model is 2×10-9, a value that can be compared with the observed value of (2+2-1)×10-9 in the north polar auroral region. Sufficient quantities of the higher ring species are produced so that their saturated vapor pressures are exceeded. Condensation of these molecules is expected to lead to aerosol formation.
Ajello Joseph M.
Lee Anthony Y. -T.
Wong Ah San
Yung Yuk L.
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