Topromium

Topromium is a very valuable material discovered by Nasrin Sherazi found in asteroids and some celestial bodies in low concentrations. Sometimes a large lump of topromium forms on asteroids. Topromium is very valuable as it is a very efficient and effective High Temperature Superconductor. It can even superconduct at room temperature. It has a great flaw though, it is extremely brittle and it has to be mixed with cagnium for it to not break by the smallest touch.

Topromium's chemical formula is (399)Ns380(380)St399(400)Fy95. All topromium made before 2418 did not contain 95 (400)Fy atoms. This was needed for the synthesis and was found to not affect its properties. These different types are known as NS-topromium and NSF-topromium. NS later became a synonym for naturally occuring topromium and NSF for artificially synthesized topromium.

Occurence
Topromium is one of three major components of prominite, which can be found very rarely in some celestial bodies. It is usually found or in very low concentrations or in large lumps of almost pure prominite, usually on asteroids.

Synthesis
Topromium is extremely hard to synthesize without a dedicated machine because of the mere second-long half-time of nasrinium and the milisecond-long half-time of stabilium, which means they have to be synthesized at almost the exact same time and then immediatly bonded together. This is why first ferryum (with a half-time of around 3 hours) is created using bombardment in an accelerator and then the decay and later fission of ferryum is used in over 31 steps before the eventual topromium bond is created. Ferryum has to remain as a stabilizer as trying to remove it would lead to molecule-wide splitting and the nasrinium and stabilium would then almost immediatly decay. The method, known as ferryum-FD-reduction (or FFDR), was discovered by Nasrin Sherazi and Michella Ferry.