Published December 1, 2016 | Version v1
Journal article

SUBMILLIMETER OBSERVATION OF JUPITER'S STRATOSPHERIC COMPOSITION: DETECTION OF CARBON MONOSULFIDE (J = 7 − 6) 19 YEARS AFTER THE COMETARY IMPACT

  • 1. Nature and Science Museum, Tokyo University of Agriculture and Technology (TUAT), Tokyo (Japan)
  • 2. Institute for Space-Earth Environment Research (ISEE), Nagoya University, Aichi (Japan)
  • 3. Graduate School of Environment, Nagoya University, Aichi (Japan)
  • 4. The University of Electro-Communications, Tokyo (Japan)
  • 5. School of Science, Ibaraki University, Ibaraki (Japan)

Description

In Jupiter's stratosphere, gaseous carbon monosulfide (CS) was first discovered in 1994 by millimeter and ultraviolet observations as a product induced by the collision of comet Shoemaker–Levy 9 (SL9). To constrain sulfur chemistry, in 2013, 19 years after the SL9 event, we observed Jupiter's stratospheric CS J = 7 − 6 rotational transition at 0.8 mm wavelength by using the Atacama Submillimeter Telescope Experiment 10 m single-dish telescope. The CS molecular line was successfully detected with 120 mK intensity in the antenna temperature scale. The obtained CS total mass shows ∼90% decrease relative to that observed in 1998. From the line shape analysis, CS is suggested to be present above the 0.2 0.15 + 0.4 mbar pressure level, which is comparable to that determined in 1998.

Availability note (English)

Available from http://dx.doi.org/10.3847/0004-6256/152/6/179

Additional details

Identifiers

Publishing Information

Journal Title
Astronomical Journal (New York, N.Y. Online)
Journal Volume
152
Journal Issue
6
Journal Page Range
[5 p.]
ISSN
1538-3881