Tsenta

Tsenta is a peculiar asteroid moonmoon of Tsentos II, its composition mostly consists of Dirty water as well as D2O2, H2O2, Hydrogen and Deuterium which indicates it's an outer system body. Tsenta further cements the part of our theory on Tsentos II as its clear evidence it has passed through the icy belt upon entering, and judging by its rings, which may indicate collision or a TTNS that reached its roche limit indicating that it Tsentos II had an eccentric orbit and eventually was captured by Zonkalym. This asteroid moonmoon is quite large and formed in a dwarf planet nursery area which may indicate that it possibly was part of a dwarf planet during the early formation era before having collided with another one, here, some scientists argue that it got its rings here due to the amount of dust and with most of the rings composition being an identical match, this can be backed by the lack of impact craters, yet one counter arguement would be that due to the slow nature of the outer belt (it was calm compared to the rest of the system at the time) it had collided or "bumped" or had been bumped by other celestial objects about the same size which may have given off debris over time hence giving birth to its ring system.