KIC 8311864
The planet candidate found orbiting KIC 8311864 has an orbital period of 384.85 days. Based on the initial assessment of the properties of this star, this planet candidate would have a radius 1.19 times that of the Earth (or RE) and an Seff I estimate to be 0.56. Based on the work by Rogers, which indicates that planets transition from being predominantly rocky to non-rocky at a radius no greater than 1.6 RE, it seems likely that this candidate is a rocky planet like the Earth (see “
Habitable Planet Reality Check: Terrestrial Planet Size Limit”). With an effective temperature of 5,587° K (hinting that the star is a G-type star slightly cooler than the Sun), the HZ for KIC 8311864 as defined by Kopparapu
et al. corresponds to an Seff from 1.08 to 0.34 assuming an Earth-mass planet orbiting this star indicating that this planet candidate is comfortably inside the HZ.
Even though this initial assessment seems very promising, a more in depth analysis currently underway by a team led by Jon Jenkins (NASA Ames Research Center) indicates that the stellar properties that they have derived from spectroscopic analysis of KIC 8311864 differ significantly from those currently in the Kepler target data base. Their data, which will be the subject of a discovery paper currently being prepared, indicate that this star is actually ~50% larger than originally thought. As a result, the radius of the planet candidate will also be larger – on the order of 1.8 RE. With this larger radius estimate, this planet candidate now has about a one-in-three chance of being a rocky planet and is more likely to be a mini-Neptune instead. The update in stellar properties also implies that the Seff might be about double the earlier estimate placing this world near the inner edge of the HZ.
While we will have to wait until the paper by Jenkins
et al. is released to get all of the details and perform a better habitability assessment, this world’s prospects for being potentially habitable are not as good as first believed but it is still worth additional consideration. The situation with this new find also illustrates the need for follow-up observations of host stars to refine important stellar parameters which in turn affect the derived properties of planetary finds.
KIC 9674320
The planet candidate found orbiting KIC 9674320 has an orbital period of 317.05 days. Assuming that the stellar parameters for KIC 9674320 in the Kepler target data base are accurate, this world has a radius of 1.66 RE and an Seff that I estimate to be 0.57. With an effective temperature of 5,370° K (hinting this star is a late G-type or maybe an early K-type star), the HZ for KIC 9674320 as defined by Kopparapu
et al. has Seff values ranging from 1.06 to 0.33 for an Earth-mass planet. While the size of this planet makes it a bit more likely to be a mini-Neptune instead of a terrestrial planet, its Seff value seems to place it comfortably inside the HZ. As the episode with KIC 8322864 has shown us, however, detailed follow-up observations will be needed to pin down the properties of this planet candidate and its host star more accurately. But at this point, it seems to be a promising potentially habitable planet candidate orbiting a Sun-like star.