Viajero
Volunteer Moderator
Dear devs,
Following on the fun discussion about Canis Majoris I was wondering what level of fidelity will be used to model some of the most peculiar stars out there...
I mean I guess Procedural Generation can churn out lots of "Sol-like" stars out there etc, with varying colours and sizes etc. But what about stars like Eta Carinae (or any other more weird types for that matter)?
Eta Carinae seems to be actually a double star with a built in thick red nebula wrapping around the 2 stars that may look something like the pics below.
Will PG allow for such level of fidelity? Or is FD planning to do a large amount of manual work on this? Or maybe it has been settled that these peculiar stars will simply look like "normal" stars maybe?
Following on the fun discussion about Canis Majoris I was wondering what level of fidelity will be used to model some of the most peculiar stars out there...
I mean I guess Procedural Generation can churn out lots of "Sol-like" stars out there etc, with varying colours and sizes etc. But what about stars like Eta Carinae (or any other more weird types for that matter)?
Eta Carinae seems to be actually a double star with a built in thick red nebula wrapping around the 2 stars that may look something like the pics below.
Will PG allow for such level of fidelity? Or is FD planning to do a large amount of manual work on this? Or maybe it has been settled that these peculiar stars will simply look like "normal" stars maybe?


