Abundances of Jupiter's Trace Hydrocarbons From Voyager and Cassini
Conor A. Nixon (1, 2), Richard K. Achterberg (1, 2), Paul N., Romani (2), Mark Allen (3, 4), Xi Zhang (3), Nicholas A. Teanby (5),, Patrick G. J. Irwin (5), F. Michael Flasar (2) ((1) University of Maryland,, (2) NASA Goddard Space Flight Center

TL;DR
This study compares the vertical and latitudinal distributions of hydrocarbons on Jupiter from Voyager and Cassini data, revealing different seasonal variations in acetylene and ethane, which inform about atmospheric chemistry and dynamics.
Contribution
It provides the first detailed comparison of hydrocarbon distributions on Jupiter across two different epochs, highlighting seasonal changes in C2H2 and C2H6.
Findings
C2H6 shows increased and more symmetric abundance in 2000 compared to 1979.
C2H2 exhibits little variation in 1979 but decreases poleward in 2000.
Different seasonal behaviors of hydrocarbons suggest complex atmospheric processes.
Abstract
The flybys of Jupiter by the Voyager spacecraft in 1979, and over two decades later by Cassini in 2000, have provided us with unique datasets from two different epochs, allowing the investigation of seasonal change in the atmosphere. In this paper we model zonal averages of thermal infrared spectra from the two instruments, Voyager 1 IRIS and Cassini CIRS, to retrieve the vertical and meridional profiles of temperature, and the abundances of the two minor hydrocarbons, acetylene (C2H2) and ethane (C2H6). The spatial variation of these gases is controlled by both chemistry and dynamics, and therefore their observed distribution gives us an insight into both processes. We find that the two gases paint quite different pictures of seasonal change. Whilst the 2-D cross-section of C2H6 abundance is slightly increased and more symmetric in 2000 (northern summer solstice) compared to 1979…
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Taxonomy
TopicsAstro and Planetary Science · Space Exploration and Technology · Planetary Science and Exploration
