Gertrude's depth was estimated to be roughly 1–3 kilometers by planetary scientist P. M. Schenk in 1989. The
crater rim of Gertrude is elevated by 2 km over the crater floor. In the center of the crater there is a large dome, which resulted from the uplift of the surface immediately after the impact. The dome has the diameter of about 150 km and is 2–3 km high. The rim and dome are low for crater with such a large diameter indicating that the relief has relaxed since the impact. The surface of the dome has only few superimposed smaller craters, which means that it was modified later. Linear ridges cut across Gertude and the nearby
Messina Chasmata. Gertrude is additionally surrounded by plains with less cratering compared to much of Titania's surface, likely representing Gertrude's ancient
ejecta blanket. Gertrude is unusually shallow; extrapolating from depth-to-diameter (d/D) ratios of smaller craters on Titania, Gertrude's original depth may have been ~6–6.5 km. This implies that Gertrude underwent a period of relaxation, where the crust slowly creeps and gradually mutes topographical extremes. The central doming of Gertrude's floor is indicative of relaxation; Gertrude's floor appears similar to the central domed floor of a large relaxed crater on
Saturn's moon
Rhea,
Tirawa. == Notes ==