Julianne I. Moses

TL;DR: In this paper, the authors synthesize and explore lessons gleaned from decades of study of planetary atmospheric chemistry to understand their implications for ex-planetary atmospheres, and demonstrate that there are commonalities across the atmospheres of our solar system that provide valuable guidance and lessons for observing and interpreting exoplanetary atmosphere.

TL;DR: In this paper, a full orbit of the planet and extracting its spectroscopic phase curve in the 5-12 $\mu$m range with JWST/MIRI were obtained.

TL;DR: In this article, an analysis of IRTF-TEXES spectra of Jupiter's mid-to-high latitudes in order to test the hypothesis that the CH4 homopause altitude is higher in Jupiter's auroral regions compared to elsewhere on the planet is presented.

TL;DR: It is considered that the upper atmosphere of Neptune might be much cooler than it was during the 1989 Voyager 2 encounter, and the impact of an enhanced influx of external material that could act to reduce H3+ density is examined.

TL;DR: Uranus and Neptune represent the least explored environments of our Solar System, and yet may provide the archetype for the most common outcome of planetary formation throughout our galaxy as mentioned in this paper, and they are the last remaining class of planet in our system to have a dedicated orbital mission.