This model of a realistic exoplanet is one of those moons/exoplanets one might expect to find in orbits of far away stars. Similar to the moons Europa and Enceladus orbiting our gas giants, this moon is an icy moon with a liquid ocean underneath. The cracks are caused by tidal forces and the movement of water. The planet has a bleu hue created by ether metal oxides, or from oxygenated water ice, indicating possible life. Which one i will leave to the imagination. Thanks to the HD textures and the low poly construction, this model can be used both as a far away background model, as well as a model for close up use.
The difference between this planet and the alfa version is that this planet is living in rougher times. a constant bombardment of meteorites made many craters on its surface. Unlike a planet with a rock surface, the ice will restore itself much faster and after some time the craters will disappear. A second difference with the alfa version is its color. the impact of the meteorites have stirred up the oceans and made them darker in color. This too will fade with time when the sediment settles at the bottom of the ocean.
Technical information
In real life, this planet would have a diameter of around 2.000 km in diameter. Some 3d programs do not display objects of this size very well. In order to avoid complications, and because most users want to decide the exact diameter themselves, the model itself is not scaled to the real life size.