I'm half way through my first Sag A* run and I've finally realised that terraform candidates are about as plentiful and as rewarding as those tasty water worlds I keep on making a detour to scan, they're just a lot harder to eyeball from the System Map.
I've noticed that the terraform candidates that I've found so far are all rocky, metallic or water worlds of 0.5-2 Earth Masses and about 0.5-1.5 AU from the primary (although there may be a bit of selection bias there, I'm not scanning every body in a system and may be missing some). This kind of fits the idea that terraforming candidates are solid bodies with a gravity which can hold an atmosphere without crushing humans and which sit in the goldilocks zone around a star (not too hot, not too cold), the specific atmosphere being replaceable through terraforming.
Is there more to this or some sort of guide to roughly where Terraforming candidates show up? If not then I'm screen-capping every terraform candidate I find and I'd love other commander's data too, if it really is something as simple as the right combination of distance from primary and mass then with enough data points we should be able to come up with a good rule of thumb for eyeballing these from the system map without scanning every body in the system.
I've noticed that the terraform candidates that I've found so far are all rocky, metallic or water worlds of 0.5-2 Earth Masses and about 0.5-1.5 AU from the primary (although there may be a bit of selection bias there, I'm not scanning every body in a system and may be missing some). This kind of fits the idea that terraforming candidates are solid bodies with a gravity which can hold an atmosphere without crushing humans and which sit in the goldilocks zone around a star (not too hot, not too cold), the specific atmosphere being replaceable through terraforming.
Is there more to this or some sort of guide to roughly where Terraforming candidates show up? If not then I'm screen-capping every terraform candidate I find and I'd love other commander's data too, if it really is something as simple as the right combination of distance from primary and mass then with enough data points we should be able to come up with a good rule of thumb for eyeballing these from the system map without scanning every body in the system.