Many of us have probably noticed this sort of thing: a planet that "should be terraformable", but for some weird reason the Stellar Forge doesn't want to classify it as such.
A case in point I have just stumbled upon: the worlds of the Boeft BV-F d11-59 system. Specifically, the three planets B8, B9 and B10. It's a binary system, so there's the complication that calculation of Goldilocks Zones is difficult.
Here's B8: 1.30 G HMC, 240 atmospheres CO2 atmosphere: a typical Venus-class planet, except that it's terraformable.
Now we have planet A9: a Water World, 1.67 gravities, 16 atmospheres high-ammonia atmostphere, kind of a proto-Earth. NOT terraformable.
Finally, planet B10: 1.49 G HMC, 0.72 atmospheres nitrogen atmosphere, a "large Mars" or perhaps a "warm Titan"; terraformable.
Why is B9 not terraformable, where B8 and B10 are? It's not a pressure problem, because B8 is higher than B9. Is it gravity? Is the co-orbiting eccentricity causing tidal heating? Anyone have any ideas?
A case in point I have just stumbled upon: the worlds of the Boeft BV-F d11-59 system. Specifically, the three planets B8, B9 and B10. It's a binary system, so there's the complication that calculation of Goldilocks Zones is difficult.
Here's B8: 1.30 G HMC, 240 atmospheres CO2 atmosphere: a typical Venus-class planet, except that it's terraformable.

Now we have planet A9: a Water World, 1.67 gravities, 16 atmospheres high-ammonia atmostphere, kind of a proto-Earth. NOT terraformable.

Finally, planet B10: 1.49 G HMC, 0.72 atmospheres nitrogen atmosphere, a "large Mars" or perhaps a "warm Titan"; terraformable.

Why is B9 not terraformable, where B8 and B10 are? It's not a pressure problem, because B8 is higher than B9. Is it gravity? Is the co-orbiting eccentricity causing tidal heating? Anyone have any ideas?