Kepler-1067 b
Astrophysical Synthesis & Habitability Characterization
Kepler-1067 b is a confirmed terrestrial exoplanet orbiting the star Kepler-1067, located approximately 2177.7 light-years (667.69 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0062% across the stellar disk), this world measures 0.8 Earth radii and has a measured mass of 0.437 Earth masses. Combining its mass and radius yields a mean bulk density of 4.71 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 0.68 g⊕ (6.67 m/s²), and an escape velocity of 8.3 km/s.
In its orbital architecture around Kepler-1067, Kepler-1067 b completes one full revolution every 0.762 Earth days at a semi-major axis of 0.0164 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 234.1 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 1872 K (+1599°C / +2910°F) and receiving 2,761.76 S⊕ (~3,758,751 W/m²), Kepler-1067 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-1067 is classified as a stellar host with an effective photospheric temperature of 5,592 K, a radius of 0.93 R☉, a mass of 0.95 M☉, an estimated bolometric luminosity of 0.759 L☉. Stellar evolution modeling indicates an estimated stellar age of 4.79 Gyr and a metallicity of [Fe/H] = 0.03 dex (near-solar heavy-element abundance). From Earth, Kepler-1067 shines at apparent V-band magnitude 14.395 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The Kepler-1067 system is a multi-planet architecture hosting 2 confirmed worlds, with Kepler-1067 b sharing its stellar neighborhood alongside Kepler-1067 c.
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-1067 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,592 K |
| Stellar Radius | 0.9300 R☉ |
| Stellar Mass | 0.9500 M☉ |
| Bolometric Luminosity | 0.759 L☉ |
| Metallicity [Fe/H] | 0.030 dex |
| Stellar Age | 4.790 Gyr |
| Apparent Magnitude | V: 14.395 · G: 14.273 |
| System Architecture | 1 Star, 2 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.016400 AU |
| Orbital Period | 0.762 days |
| Mean Orbital Velocity | 234.1 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 84.8800° |
| Mean Bulk Density | 4.71 g/cm³ (8.3 km/s vesc) |
| Insolation Flux | 2761.7570 S⊕ (~3,758,751 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 2177.700 LY (667.693 pc) |