Aerosols are common in the atmospheres of exoplanets across a wide swath of
temperatures, masses and ages,–. These aerosols strongly impact observations of …

Comparatively little is known about atmospheric chemistry on Uranus and Neptune,
because remote spectral observations of these cold, distant 'Ice Giants' are challenging, and …

Observations of Jupiter's deep atmosphere by the Juno spacecraft have revealed several
puzzling facts: The concentration of ammonia is variable down to pressures of tens of bars …

The mid-infrared spectral region provides a unique window into the atmospheric
temperature, chemistry, and dynamics of the giant planets. From more than a century of mid …

We present mid-infrared spectroscopy of Jupiter's mid-to-high latitudes using the Gemini-
North/Texas Echelon Cross Echelle Spectrograph on 2017 March 17–19. These …

We present multiwavelength measurements of the thermal, chemical, and cloud contrasts
associated with the visibly dark formations (also known as 5‐μm hot spots) and intervening …

The spatial distribution of water, ammonia, phosphine, germane, and arsine in the Jupiter's
troposphere has been inferred from the Jovian Infrared Auroral Mapper (JIRAM) Juno data …

We obtained high-resolution spectra of Jupiter between 4.6 and 5.4 µm using NIRSPEC on
the Keck 2 telescope in February 2017. We measured the spatial variation of NH 3, H 2 O …

The cosmic deuterium fraction, set by primordial nucleosynthesis and diminished by
subsequent astration, is a valuable diagnostic tool to link the protosolar nebula to the history …

Both the identity of the coloring agent (s) in Jupiter's atmosphere and the exact structure of
Jupiter's uppermost cloud deck are yet to be conclusively understood. While the arrival of the …