PS2.3 | Titan Exploration
Titan Exploration
Convener: Panayotis Lavvas | Co-conveners: Athena Coustenis, Tommi Koskinen, Conor Nixon, Anezina Solomonidou

Titan is one of the most complex environments in the solar system, a complexity expressed in a triad of manifestations: in the photochemically intense and seasonally varying atmosphere; in the unique hydrocarbon lakes and oceans, the dunes and other geomorphological features; and in the astrobiologically intriguing subsurface water ocean.
We invite the international Titan community to convene in the 2025 EGU general assembly where all above aspects will be discussed from observational, theoretical and experimental perspectives. We look forward discussing the latest discoveries from the analysis of Cassini-Huygens, JWST and ground-based observations, as well as exploring anticipated results from the forthcoming Dragonfly mission. This is also a great opportunity for the community to exchange ideas with colleagues studying the Earth, the only other planet matching Titan's systemic complexity.

Titan is one of the most complex environments in the solar system, a complexity expressed in a triad of manifestations: in the photochemically intense and seasonally varying atmosphere; in the unique hydrocarbon lakes and oceans, the dunes and other geomorphological features; and in the astrobiologically intriguing subsurface water ocean.
We invite the international Titan community to convene in the 2025 EGU general assembly where all above aspects will be discussed from observational, theoretical and experimental perspectives. We look forward discussing the latest discoveries from the analysis of Cassini-Huygens, JWST and ground-based observations, as well as exploring anticipated results from the forthcoming Dragonfly mission. This is also a great opportunity for the community to exchange ideas with colleagues studying the Earth, the only other planet matching Titan's systemic complexity.