Detection of visible lightning on Saturn

  • Dyudina U
  • Ingersoll A
  • Ewald S
  • et al.
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Abstract

Until now, evidence for lightning on Saturn has been indirect – through radio emissions and cloud morphology. Here we report the first visible detection of lightning, on the night side on August 17, 2009 at −36.4° ± 0.1° planetocentric latitude and 10.6° ± 0.9° west longitude. No other locations produced lightning detectable by either imaging or radio. The lightning images are consistent with a single cloud flashing once per minute. The visible energy of a single flash is comparable to that on Earth and Jupiter, and ranges up to 1.7 × 10 9 Joules. The diameter of the lightning flashes is ∼200 km, which suggests the lightning is 125–250 km below cloud tops. This depth is above the base of the liquid H 2 O‐NH 3 cloud and may be either in the NH 4 SH cloud or in the H 2 O ice cloud. Saturn's lower internal heat transport and likely 5–10 fold enrichment of water largely explain the lower occurrence rate of moist convection on Saturn relative to Jupiter.

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Dyudina, U. A., Ingersoll, A. P., Ewald, S. P., Porco, C. C., Fischer, G., Kurth, W. S., & West, R. A. (2010). Detection of visible lightning on Saturn. Geophysical Research Letters, 37(9). https://doi.org/10.1029/2010gl043188

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