I'm sorry, but you did a pretty sloppy job on this.
1. A 130 solar mass star like S-1 will not become a red hypergiant. If it did, it would self-destruct due to the enormous radiation pressure overpowering its gravity. Stars like Eta Carinae do the following: form, photoevaporate planet-forming disks around themselves and any other star nearby, cast off lots of their outer layers due to radiation pressure, blow up, become black holes. This is over only a few million years.
2. You have not bothered to change the masses of your Rigels, your Wolf 359s, Chenia (AKA Arcturus), GT Star (AKA Sol), Solaris (AKA Polaris), or Estrela de Rosario (AKA Pollux). This shows a great lack of effort. At least take the time to make the most important star (the one we're supposed to make a system for) unique.
3. Agia A and Agia B are named as if they are binaries, as opposed to in completely different locations. You also clearly started with Wolf 359s and failed to change the diameter, resulting in densities impossible for main-sequence stars.
4. Star clusters are several light years in diameter, not a couple hundred AU. See point 5 for why.
5. When I ran the system, chaos ensued. Estrela de Rosario was consumed by S-49 (which had also apparently eaten one of the other Rigels, as shortly afterward it had a mass of 36 suns) only 1.45 years in. S-49 was later itself consumed by S-1. As things stand, S-1 and S-96 appear to have formed a stable binary, as the only other surviving star large enough to affect the proceedings, namely S-9, fled the grisly spectacle in horror. GT Star and three of the remaining brown dwarfs also orbit the binary, although they may well be destroyed or ejected, as their orbits appear unstable.
Topic: S-1 Imaginary Cluster (Read 8221 times)
