Gertrude (crater)
 Gertrude is the large crater near the top of this Voyager 2 image. | |
| Feature type | Peak-ring impact basin |
|---|---|
| Location | Titania |
| Coordinates | 15°48′S 72°54′W / 15.80°S 72.90°W[1] |
| Diameter | ~326 km (203 mi) (GPN)[1] 400 ± 15 km (248.5 ± 9.3 mi) (Moore et al.)[2] |
| Depth | ~1–3 km (0.62–1.86 mi) |
| Discoverer | Voyager 2 |
| Eponym | Gertrude, mother of Prince Hamlet |
Gertrude /ˈɡɜːrtruːd/ is the largest known crater on Uranus's moon Titania. A peak-ring impact basin, it is roughly 326–400 kilometers across,[1][2] 1/5 to 1/4 of Titania's diameter.[a] Gertrude was first observed by the Voyager 2 spacecraft on its January 1986 flyby of the Uranian system. It is named after Gertrude, the mother of Prince Hamlet in William Shakespeare's play Hamlet. The name Gertrude was officially adopted by the International Astronomical Union (IAU) in 1988.[1] Features on Titania are named after female Shakespearean characters.
Geology and characteristics
[edit]Gertrude's depth was estimated to be roughly 1–3 kilometers by planetary scientist P. M. Schenk in 1989.[4] 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.[2] 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.[5]
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.[4]
Notes
[edit]- ^ Titania's diameter is 1576.8 ± 1.2 km.[3] Crater-diameter ratios are given by dividing the impact crater diameter by the object's bulk diameter. Using a diameter of 326 kilometers from the Gazetteer of Planetary Nomenclature yields a crater-diameter ratio of 0.207;[1] using a diameter of 400 kilometers from Moore and collaborators yields a crater-diameter ratio of 0.254.[2]
References
[edit]- ^ a b c d e "Gertrude". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program. (Center Latitude: -15.80°, Center Longitude: 287.10°; Planetocentric, +East)
- ^ a b c d Moore, Jeffrey M.; Schenk, Paul M.; Bruesch, Lindsey S.; Asphaug, Erik; McKinnon, William B. (October 2004). "Large impact features on middle-sized icy satellites" (PDF). Icarus. 171 (2): 421–443. Bibcode:2004Icar..171..421M. doi:10.1016/j.icarus.2004.05.009.
- ^ Widemann, T.; Sicardy, B.; Dusser, R.; Martinez, C.; Beisker, W.; Bredner, E.; Dunham, D.; Maley, P.; Lellouch, E.; Arlot, J. -E.; Berthier, J.; Colas, F.; Hubbard, W. B.; Hill, R.; Lecacheux, J.; Lecampion, J. -F.; Pau, S.; Rapaport, M.; Roques, F.; Thuillot, W.; Hills, C. R.; Elliott, A. J.; Miles, R.; Platt, T.; Cremaschini, C.; Dubreuil, P.; Cavadore, C.; Demeautis, C.; Henriquet, P.; et al. (February 2009). "Titania's radius and an upper limit on its atmosphere from the September 8, 2001 stellar occultation" (PDF). Icarus. 199 (2): 458–476. Bibcode:2009Icar..199..458W. doi:10.1016/j.icarus.2008.09.011.
- ^ a b Schenk, P. M. (10 April 1989). "Crater formation and modification on the icy satellites of Uranus and Saturn: depth/diameter and central peak occurrence". Journal of Geophysical Research. 94: 3813–3832. Bibcode:1989JGR....94.3813S. doi:10.1029/JB094iB04p03813.
- ^ Beddingfield, Chloe B.; Leonard, Erin J.; Nordheim, Tom A.; Cartwright, Richard J.; Castillo-Rogez, Julie C. (8 November 2023). "Titania's Heat Fluxes Revealed by Messina Chasmata". The Planetary Science Journal. 4 (11). Bibcode:2023PSJ.....4..211B. doi:10.3847/PSJ/ad0367.
External links
[edit]- Gertrude peeks over the terminator at the Planetary Society