Many of us deal with physical parameters to be constraint... that is performing theory, but in which way I can make sure that my experimental sample is a representative sample?
Imagining that my data base is formed by N stars of certain type, these are the only ones that have hitherto been observed. One may say okay if N=1000 that is big enough, how could I be certain about it?
One possibility is to wait maybe 10 years more to collect more observational database and corroborate theory with the new bigger group...but again how can I be certain again? Our Galaxy contains millions millions of stars of these group, how could I validate my theory? That is to extend what happens in one sample to the whole sample that is a whole galaxy