A seismic investigation on Saturn's moon Enceladus could determine the thickness of the ice shell, along with variations from the mean thickness, by recovering phase and group …
Z Xu, P Lognonné - Geophysical Journal International, 2024 - academic.oup.com
Atmospheric and oceanic pressure perturbations deform the ground surface and the seafloor, respectively. This mechanical deformation, where the fluid perturbations propagate …
Previous 1‐D spherically symmetric seismic modeling studies have shown that in the presence of a clathrate lid on Titan significant thermal profile differences result, particularly …
Titan's impact craters are hundreds of meters shallower than expected, compared to similar- sized craters on Ganymede. Only 90 crater candidates have been identified, the majority of …
CA Nixon, N Carrasco, C Sotin - arXiv preprint arXiv:2501.00971, 2025 - arxiv.org
In this chapter we attempt to distill the very large number of possible future inquiries of Titan into a relatively concise list of twenty high level questions-each of which of would …
The search for life beyond Earth has been closely tied to the presence of liquid water. Often, astrobiologists focus on three key criteria for life: liquid water, nutrient availability, and …