Joule D=98 km Center: 27¡N, 216¡E Count Area: 1053 km^2 Observed Density (@ 1km): 31300 ± 5500 Age: 4.0 ± 0.1 (+sec: 4.1) Stoffler epoch: Pre-Nectarian Fit density (@ 1km): 49900 ± 6900 PF fit: good*, all craters within error, small area (~ 1000 km2) Age calculation notes: - poor fit - fit anchored at large D. Fit improved to good with layering with thickness H=0.20km. the top layer has Y=2e7, the bottom layer has Y=2e8 (SM). - good fit to large D - bad fit to small D - maybe geology, but worth trying strength scaling law or layer?; adding OSs slightly improves fit and produces older age. Fit improved using layering (LrN), age decreases slightly (MRK). - why does using layering work? Including a change in strength causes the PF to kink and shift for small D (transition occurs D ~ 1 km), which is why the fit is better. But is there justification for using this law here and not with other craters (i.e., is geology different)? The surface does have a weathered look, but can see small areas that look more "solid". There is one partially filled larger crater indicating a thin layer of fill (which see in other layers w/o kink). So a thin "weak" layer over a stronger layer is not unreasonable. Note a resurfacing event that removes small craters preferentially can produce the same effect and terrains of two ages. Although a region of of lower small crater density does not pop out. (MRK) USGS geology: Crater mapped as Nectarian. Small areas of floor material mapped as fill with Imbrian to Nectarian age (corresponds with counting area). Wilhelms: Crater is Nectarian. Perhaps a little fill with Orientale ejecta (Early Imbrian)? Floor material: Best guess is not original for areas counted. Flatter floor, material has contacts with wall/peak that look embayed, fill in larger crater on the floor, small central peak. Material looks softened. Loose? Geology Observations: Ejecta not visible(see ejecta, but likely from the nearby younger craters?). Rim is eroded (especially to south - landed on another crater?), but has a little sharpness on east side. Small central peak that looks heavily eroded. Floor has low hummocks (maybe original floor or collapses) with some smooth areas (smooth areas counted). A few secondary chains/clusters with various sized craters (up to ~ 2 km) - mostly degraded. SFD Observations: Craters < ~ 2 km dominated by class 4. Largest craters dominated by class 3. Classes 1 and 2 lower in density. Has flat SFD for full diameter range. Slope(Diff)=2.9 ± 0.3. Discussion notes: Change floor "possibly" to "not likely" Notes from Brian's adjustment: - Counting boundary: Irregular, but might be OK. A bit iffy near 6:00. Some missing type 4's. - Secondaries: One cluster missed at 7:30, another in the center. - Removal of large, buried craters: The large crater at 6:00 depends on whether the boundary is changed. - Size adjustment of large craters: The large crater at 6:00 should be slightly larger. - Explaining unusual cases: - Future actions: - Completed actions: Changed the boundary (Michelle). Add some type 4 craters and clusters (BLE). Altered a few classifications (MRK). Last Edited by MRK 12/13/2012