Kepler-80 f
Astrophysical Synthesis & Habitability Characterization
Kepler-80 f is a confirmed terrestrial exoplanet orbiting the star Kepler-80, located approximately 1205 light-years (369.45 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0268% across the stellar disk), this world measures 1.21 Earth radii and has a measured mass of 4459.73 Earth masses (14.03 Jupiter masses). Combining its mass and radius yields a mean bulk density of 13880.95 g/cm³ (an iron-enriched, high-compression rocky core), a surface gravity of 3046.06 g⊕ (29871.64 m/s²), and an escape velocity of 679.1 km/s.
In its orbital architecture around Kepler-80, Kepler-80 f completes one full revolution every 0.987 Earth days at a semi-major axis of 0.0175 AU (an ultra-close orbit less than one-seventh of Mercury's 0.387 AU distance from the Sun, where strong stellar tidal forces typically induce synchronous rotation). Its mean orbital velocity is approximately 192.9 km/s (compared to Earth's 29.8 km/s). Its moderate orbital eccentricity of e = 0.186 carries the world between 0.0142 AU at periapsis and 0.0208 AU at apoapsis, driving measurable seasonal insolation cycles.
⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1054 K (+781°C / +1438°F) and receiving 750.96 S⊕ (~1,022,062 W/m²), Kepler-80 f orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-80 is classified as an orange K-type star of spectral type K5 with an effective photospheric temperature of 4,540 K, a radius of 0.678 R☉, a mass of 0.73 M☉, an estimated bolometric luminosity of 0.175 L☉. Stellar evolution modeling indicates an estimated stellar age of 2 Gyr and a metallicity of [Fe/H] = 0.04 dex (near-solar heavy-element abundance). From Earth, Kepler-80 shines at apparent V-band magnitude 15.23 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The Kepler-80 system is a multi-planet architecture hosting 6 confirmed worlds, with Kepler-80 f sharing its stellar neighborhood alongside Kepler-80 d, Kepler-80 e, Kepler-80 b, Kepler-80 c, Kepler-80 g.
Methodology: Computed using the Schulze-Makuch et al. (2011) weighted metric comparing physical interior (radius, estimated density) and surface thermal regime (escape velocity, equilibrium temperature).
Discovery Facility: Kepler · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).
☀️ Host Star Telemetry
| Host Star Name | Kepler-80 |
| Spectral Type | K5 |
| Effective Temp (Teff) | 4,540 K |
| Stellar Radius | 0.6780 R☉ |
| Stellar Mass | 0.7300 M☉ |
| Bolometric Luminosity | 0.175 L☉ |
| Metallicity [Fe/H] | 0.040 dex |
| Stellar Age | 2.000 Gyr |
| Apparent Magnitude | V: 15.230 · G: 14.756 |
| System Architecture | 1 Star, 6 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.017500 AU |
| Orbital Period | 0.987 days |
| Mean Orbital Velocity | 192.9 km/s |
| Orbital Eccentricity (e) | 0.18600 |
| Orbital Inclination (i) | 86.5000° |
| Mean Bulk Density | 13880.95 g/cm³ (679.1 km/s vesc) |
| Insolation Flux | 750.9640 S⊕ (~1,022,062 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 1205.000 LY (369.451 pc) |