This model is made by myself using MATLAB R2016a on the incomplete map from Schenk (2009) filled with the low resolution map from Tajedinne (2017). Some features can be artifacts of the overlying between the maps. It's scaled to 1 in 107 or one in ten million. The model of this has about 5cm in diameter. On this scale the Moon is a basketball and Mars' moons Phobos and Deimos are 2 and 1 mm respectively. It's also included a one in four million scaled model for more details, wich model is about 12 cm.
The file's names explained: name_1_x_10_y.stl is 1 : x * 10y. So _1_6_10_7 is 1:600000000 or one in 60 million.
Enceladus is the sixth largest moon of Saturn. It looks like a smaller version of the moon of Jupiter, Europa. Both of them have a thick water ice crust, stripes and water vapor "geysers" at the south pole. It is widely accepted that both have subsurface oceans, responsible for tectonic activity. The "snow ball" appearence is because of the falling material from the "geysers". The escaping material is the source of the E ring of Saturn.
Orbital period: 1.37 d
Composition: Icy body, differenciated interior, subsurface ocean, rocky core.
Density: 1.609 g/cm3.
Dimensions: 513.2 km × 502.8 km × 496.6 km
Model scale: 1:1x107 (5cm) 1:4x106 (12cm)
Level map from Schenk et al. (2009)
Topographic map from Tajedinne et al. (2017)