I heavily doubt any superheavy transuranic elements would be found in any appreciable quantities on another planet. Even if they're formed from something like a supernova, they decay too fast to really "exist". Even if a specific isotope lies in the theoretical "belt of stability", that pretty much means it decays in a few minutes rather than in miniscule fractions of a second. As an example, take Francium. It decays in less than an hour. We still don't know a lot about it because, due to its quick decay, it is so hard to find, and when found, hard to analyze quickly enough.
As to where to add the elements, we know this already. You need to know about electron orbital theory to understand what I'm about to say. 118 currently resides in the seventh period of group 8 because it has its 7p orbital completely filled, like the other elements in that group. 119 goes below Francium (It theoretically has one 8s electron, like Francium's lone 7s and Cesium's lone 6s), and 120 goes below Radium (It theoretically has two 8s electrons, like Radium's 7s pair and Barium's 6s pair).
Now, here's the wrinkle. Electron orbital theory predicts a 5g orbital appearing at element 121. This would be a new block on the table, like the f-block of Lanthanides and Actinides. Who knows what their properties would be (we have no frame of reference).