Calculating Barycentre RA/Dec of hyper-wide Binaries?
Posted: 20.04.2013, 05:48
I've noticed that a number of stars in Celestia containing two or more stellar components that have barycenters defined, but without orbital data; being instead placed by the traditional RA and Dec coordinates and distance.
So, how does one calculate the barycenter in situations like that; and also if one wanted to implement orbital definitions (real or fictional) of their own for said binaries, like what was apparently done for ALF Cen?
So, how does one calculate the barycenter in situations like that; and also if one wanted to implement orbital definitions (real or fictional) of their own for said binaries, like what was apparently done for ALF Cen?