The detection of benzene in Saturn's upper atmosphere

T. T. Koskinen, J. I. Moses, R. A. West, S. Guerlet, A. Jouchoux

Research output: Contribution to journalArticle

13 Scopus citations

Abstract

The stratosphere of Saturn contains a photochemical haze that appears thicker at the poles and may originate from chemistry driven by the aurora. Models suggest that the formation of hydrocarbon haze is initiated at high altitudes by the production of benzene, which is followed by the formation of heavier ring polycyclic aromatic hydrocarbons. Until now there have been no observations of hydrocarbons or photochemical haze in the production region to constrain these models. We report the first vertical profiles of benzene and constraints on haze opacity in the upper atmosphere of Saturn retrieved from Cassini Ultraviolet Imaging Spectrograph stellar occultations. We detect benzene at several different latitudes and find that the observed abundances of benzene can be produced by solar-driven ion chemistry that is enhanced at high latitudes in the northern hemisphere during spring. We also detect evidence for condensation and haze at high southern latitudes in the polar night.

Original languageEnglish (US)
Pages (from-to)7895-7901
Number of pages7
JournalGeophysical Research Letters
Volume43
Issue number15
DOIs
StatePublished - Aug 16 2016

Keywords

  • Saturn
  • photochemistry

ASJC Scopus subject areas

  • Geophysics
  • Earth and Planetary Sciences(all)

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    Koskinen, T. T., Moses, J. I., West, R. A., Guerlet, S., & Jouchoux, A. (2016). The detection of benzene in Saturn's upper atmosphere. Geophysical Research Letters, 43(15), 7895-7901. https://doi.org/10.1002/2016GL070000