[astro-ph.EP] We developed TitanMPAS, a new Titan global and regional climate model, to simulate atmospheric dynamics and methane cycles.
![Titan surface properties: topography (a), albedo (b), thermal inertia (c) and lake distribution (d). All three maps use 180◦ W to 180◦ E convention. The Huygens lander location is near 167◦ E and 10◦ S in the topography map. -- [astro-ph.EP]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/11/TitanMPAS.png?resize=1200%2C715&ssl=1)
[astro-ph.EP] We developed TitanMPAS, a new Titan global and regional climate model, to simulate atmospheric dynamics and methane cycles.