Vedral

== Intro ==
Vedral is the secondary star of the Ruber Verinillius system, in the Seloria cluster. It is a small late-m red dwarf star, and is also known a RC 58611 AB, as it is in the Ruber catalogues (the whole system is), and it is in a close orbit with the primary star in this system, Eona. It is the oldest member of the trio, just 9 million years older than Eona. Vedral is surprisingly active, even though the tidal forces from Eona are calming it down.
== Other stuff ==
It is very similar to Eona except smaller, less massive, dimmer, and cooler. It orbits Eona in less that 2 days.
== Trivia ==
* Vedral is also very similar to Caylera.
Category:Stars
Category:Trolligi112477-ww
Category:Seloria cluster
Category:Ruber catalogues