Table 1
Observational details of the nine craters examined in this work.
Name | VIMS | RADAR | Crater floor | Ejecta blanket |
---|---|---|---|---|
(flyby-date) | (flyby-date) | Coordinates | Coordinates | |
Geometry-Resolution | Geometry-Resolution | |||
(i,e,α,res) | (i,e,α,res) | |||
Dune craters | ||||
Ksa | T125 (11/2016) | T77 (06/2011) | 14.2°N-65.4°W | 15°N-64.9°W |
41°/41°/68°/22 km | 41°/41°/68°/22 km | |||
Selk | T40 (01/2008) | T36 (10/2007) | 6.7°N-160.7°W | 7.5°N-161.7°W |
T95 (10/2013) | 34°/12°/40°/04 km | 35°/12°/39°/04 km | ||
Santorini | T113 (09/2015) | T56 (06/2009) | 2°N-157.2°W | 1.4°N-146°W |
T44 (05/2008) | 56°/02°/57°/14 km | 55°/02°/57°/14 km | ||
Guabonito | T113 (09/2015) | T13 (04/2006) | 11.4°N-151.8°W | 12.1°N-152.1°W |
T48 (12/2008) | 65°/14°/53°/10 km | 65°/16°/53°/10 km | ||
Menrva (*) | T114 (11/2015) | T3 (02/2005) | 20.5°N-86.4°W | 17.7°N-83.1°W |
T77 (06/2011) | 46°/36°/60°/08 km | 43°/33°/60°/08 km | ||
Sinlap | T110 (03/2015) | T3 (02/2005) | 11.5°N-15.7°W | 10.9°N-17.2°W |
T17 (09/2006) | 28°/07°/35°/09 km | 30°/05°/34°/09 km | ||
T108 (01/2015) | ||||
Plain craters | ||||
Forseti | T13 (04/2016) | T23 (01/2007) | 25.7°N-11.1°W | 25.6°N-10.9°W |
T84 (06/2012) | 51°/27°/37°/10 km | 51°/27°/37°/10 km | ||
T113 (09/2015) | ||||
Afekan | T38 (12/2007) | T43 (05/2008) | 25.6°N-200°W | 25.3°N-201°W |
T83 (05/2012) | 44°/24°/42°/16 km | 44°/24°/42°/16 km | ||
Soi | T12 (03/2016) | T16 (07/2006) | 24.2°N-141.2°W | 24.6°N-142.2°W |
T55 (05/2009) | 44°/26°/23°/46 km | 44°/26°/23°/46 km | ||
T56 (06/2009) | ||||
Titan Units | Centroid Coordinates | VIMS | ||
(i,e,α,res) | ||||
Undifferentiated plain | T08 (10/2005) | T55 (05/2009) | 30.4°N-133.3°W | 51°/34°/23°/75 km |
(NE of Soi crater) | ||||
Dunes | T65 (01/2010) | T92 (07/2013) | 5°N-237°W | 43°/23°/43°/91 km |
(Belet field) |
Notes. In addition, we have included two typical Titan regions (i.e., an undifferentiated plain and a dune field) from Solomonidou et al. (2016, 2018) for context purposes. Here we report the related Flybys (“T” stands for Cassini Flybys of Titan) and dates for the VIMS and RADAR data used in this work, the center coordinates of the two units of interest (crater floors and ejecta blankets), and geometry details (angles of Incidence (i), Emission (e), Phase (α), and Spatial Resolution (res)) of the VIMS cubes. (*)Menrva straddles the dune and the plain regions.
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