Kepler-1014 b
Astrophysical Synthesis & Habitability Characterization
Kepler-1014 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-1014, located approximately 2037.8 light-years (624.8 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.068% across the stellar disk), this world measures 2.39 Earth radii and has a measured mass of 6.3 Earth masses. Combining its mass and radius yields a mean bulk density of 2.54 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.1 g⊕ (10.79 m/s²), and an escape velocity of 18.2 km/s.
In its orbital architecture around Kepler-1014, Kepler-1014 b completes one full revolution every 16.571 Earth days at a semi-major axis of 0.121 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 79.4 km/s (compared to Earth's 29.8 km/s). The orbit is modeled as circular (e = 0.00), maintaining a constant stellar distance throughout its year.
⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 614 K (+341°C / +646°F) and receiving 33.48 S⊕ (~45,565 W/m²), Kepler-1014 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-1014 is classified as a stellar host with an effective photospheric temperature of 5,388 K, a radius of 0.84 R☉, a mass of 0.88 M☉, an estimated bolometric luminosity of 0.534 L☉. Stellar evolution modeling indicates an estimated stellar age of 4.79 Gyr and a metallicity of [Fe/H] = -0.06 dex (near-solar heavy-element abundance). From Earth, Kepler-1014 shines at apparent V-band magnitude 14.866 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.
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-1014 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,388 K |
| Stellar Radius | 0.8400 R☉ |
| Stellar Mass | 0.8800 M☉ |
| Bolometric Luminosity | 0.534 L☉ |
| Metallicity [Fe/H] | -0.060 dex |
| Stellar Age | 4.790 Gyr |
| Apparent Magnitude | V: 14.866 · G: 14.627 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.121000 AU |
| Orbital Period | 16.571 days |
| Mean Orbital Velocity | 79.4 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.1600° |
| Mean Bulk Density | 2.54 g/cm³ (18.2 km/s vesc) |
| Insolation Flux | 33.4790 S⊕ (~45,565 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 2037.800 LY (624.800 pc) |