Titan, with its thick and hazy atmosphere, is a key world in our solar system for understanding light scattering processes.
Titan
Thermal Inertia Controls on Titan’s Surface Temperature and Planetary Boundary Layer Structure
Understanding Titan’s planetary boundary layer (PBL) — the lowest region of the atmosphere influenced by surface conditions — remains challenging due to Titan’s thick atmosphere and limited observations.
The Detection-vs-Retrieval Challenge: Titan As An Exoplanet
Cassini’s observations of Titan’s atmosphere are exemplary benchmarks for exoplanet atmospheric studies owing to (1) their precision and (2) our independent knowledge of Titan.
Measurement of Photochemical Haze Refractive Indices and Hygroscopicity: Influence of CO2 in CH4/H2S/N2 Mixtures
Atmospheric organic hazes are widespread across various planetary bodies and have significant effects on both the surface and atmosphere. In this study, we investigate the optical and hygroscopic properties of […]
Titan In-situ Resource Utilization (ISRU) Sample Return (TISR)
Titan is unique in the outer solar system in that it is the only moon with a thick atmosphere, and the only body in the solar system outside the Earth […]
Cloud and Haze Parameterization in Atmospheric Retrievals: Insights from Titan’s Cassini Data and JWST Observations of Hot Jupiters
Context: Before JWST, telescope observations were not sensitive enough to constrain the nature of clouds in exo-atmospheres. Recent observations, however, have inferred cloud signatures as well as haze-enhanced scattering slopes […]
Titan’s Mysterious Wobbling Atmosphere Is Like A Gyroscope
The puzzling behaviour of Titan’s atmosphere has been revealed by researchers at the University of Bristol for the first time.
The Atmosphere of Titan in Late Northern Summer from JWST and Keck Observations
Saturn’s moon Titan undergoes a long annual cycle of 29.45 Earth years. Titan’s northern winter and spring were investigated in detail by the Cassini-Huygens spacecraft (2004-2017), but the northern summer […]
Evidence Of Clouds Bubbling Up Over Titan’s Northern Hemisphere
Maunakea, Hawaiʻi – Astronomers using W. M. Keck Observatory on Maunakea, Hawaiʻi Island have, for the first time, found evidence for cloud convection in the northern hemisphere of Titan, Saturn’s […]
Webb Telescope Studies The Weather On Titan – A Prime Astrobiology Target
A science team has combined data from the NASA/ESA/CSA James Webb Space Telescope and the Keck II telescope to see evidence of cloud convection on Saturn’s moon Titan in the […]
