Large Volcanic Event on Io Inferred from Jovian Sodium Nebula Brightening
Abstract
Using narrow-band images recorded on over 150 nights by the 35 cm coronagraph that comprises the Planetary Science Institute’s Io Input/Output Facility (IoIO), we detected a 6-month long enhancement in the Jovian sodium nebula. The onset of the enhancement occurred in the mid 2017 December-early 2018 January timeframe. Sodium emission over the IoIO 0.°4 field of view was seen to increase through 2018 January and peak in 2018 early March. By early June 2018, the surface brightness of the emission returned to the value seen in 2017 April-June, making this the longest such event observed by this technique and comparable in length to that observed by the Galileo Dust Detector in 2000. A new infrared hot spot was found on Io near Susanoo/Mulungu Paterae between January 2 and 12, however this hot spot was neither bright nor long-lasting enough to have been independently identified as the source of a major sodium nebula enhancement. Furthermore, no other report of this event has been made despite a significant number of observations of the Jovian system by and in support of NASA’s Juno mission. This detection therefore places those observations in valuable context and highlights the importance of synoptic observations by facilities such as IoIO, which provide a global view of neutral material in the Jovian magnetosphere.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- February 2019
- DOI:
- 10.3847/2041-8213/aafdb7
- Bibcode:
- 2019ApJ...871L..23M
- Keywords:
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- instrumentation: miscellaneous;
- planets and satellites: individual: Jupiter;
- Io