Abundances of trace constituents in Jupiter's atmosphere inferred from Herschel/PACS observations
- 1Max-Planck-Institut für Astronomie, 69117 Heidelberg, Germany (gapp@mpia.de)
- 2Max-Planck-Institut für Sonnensystemforschung, 37077 Göttingen, Germany
- 3Kyoto Sangyo University, Kyoto 603-8555, Japan
- 4Max-Planck-Institut für Extraterrestrische Physik, 85746 Garching, Germany
- 5LESIA–Observatoire de Paris, CNRS, UPMC Univ. Paris 06, Univ. Denis Diderot, Sorbonne Paris Cite, Meudon, France
- 6NASA Goddard Space Flight Center, Greenbelt, MD, USA
Context. On October 31, 2009, the Photodetector Array Camera and Spectrometer (PACS) onboard the Herschel Space Observatory observed far infrared spectra of Jupiter in the wavelength range between 50 and 220µm as part of the program ‘Water and Related Chemistry in the Solar System’. The spectra have an effective spectral resolution between 900 and 3500, depending on wavelength and grating order.
Aims. We investigate the disk-averaged chemical composition of Jupiter's atmosphere as a function of height using these observations.
Methods. We used the Planetary Spectrum Generator (PSG) and the least squares fitting technique to infer the abundances of trace constituents.
Results. The PACS data include numerous spectral lines attributable to ammonia (NH3), methane (CH4), phosphine (PH3), water (H2O) and deuterated hydrogen (HD) in the Jovian atmosphere and probe the chemical composition from p∼275 mbar to p∼900 mbar. From the observations, we infer an ammonia abundance profile that decreases from a mole fraction of (1.7±0.8)x10-4 at p∼900 mbar to (1.7±0.9)x10-8 at p∼275 mbar, following a fractional scale height of about 0.114. For phosphine, we find a mole fraction of (7.2±1.2)x10-7 at pressures higher than (550±100) mbar and a decrease of its abundance at lower pressures following a fractional scale height of (0.09±0.02). Our analysis delivers a methane mole fraction of (1.49±0.09)x10-3. Analyzing the HD R(0) line at 112.1 µm yields a new measurement of Jupiter's D/H ratio, D/H=(1.5±0.6)x10-5. Finally, the PACS data allow us to put the most stringent 3σ upper limits yet on the mole fractions of hydrogen halides in the Jovian troposphere. These new upper limits are <1.1x10-11 for hydrogen fluoride (HF), <6.0x10-11 for hydrogen chloride (HCl), <2.3x10-10 for hydrogen bromide (HBr) and <1.2x10-9 for hydrogen iodide (HI) and support the proposed condensation of hydrogen halides into ammonium halide salts in the Jovian troposphere.
How to cite: Gapp, C., Rengel, M., Hartogh, P., Sagawa, H., Feuchtgruber, H., Lellouch, E., and Villanueva, G. L.: Abundances of trace constituents in Jupiter's atmosphere inferred from Herschel/PACS observations, Europlanet Science Congress 2024, Berlin, Germany, 8–13 Sep 2024, EPSC2024-208, https://doi.org/10.5194/epsc2024-208, 2024.
