I'm not sure "Earthlike" is the best way to describe these extremely hot exoplanets that are likely tidally-locked in their very close orbit around what is likely a hostile, flaring M-class star.
Other than that, they should be great.
Perhaps "Venuslike" would be better, assuming they have any atmosphere left.
| | | | Percent of HZ width; -200% is | | | |
| | | | 2x the HZ width toward star] | | | |
Name | Radius (E) | Mass (J) | a, AU | Std. Meth. | Temp. Meth | Equil. Temp. | Per., days |
HD 260655 b | 1.214 | 0.007 | 0.029 | -193.30% | -190.70% | 649K (708F) | 2.77 |
HD 260655 c | 1.502 | 0.01 | 0.047 | -172.50% | -168.30% | 510K (458F) | 5.71 |