Kepler-1412 b
Astrophysical Synthesis & Habitability Characterization
Kepler-1412 b is a confirmed terrestrial exoplanet orbiting the star Kepler-1412, located approximately 2464.7 light-years (755.68 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0036% across the stellar disk), this world measures 0.83 Earth radii and has a measured mass of 0.498 Earth masses. Combining its mass and radius yields a mean bulk density of 4.8 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 0.72 g⊕ (7.06 m/s²), and an escape velocity of 8.7 km/s.
In its orbital architecture around Kepler-1412, Kepler-1412 b completes one full revolution every 3.615 Earth days at a semi-major axis of 0.04608 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 138.7 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 1397 K (+1124°C / +2055°F) and receiving 1,087.78 S⊕ (~1,480,470 W/m²), Kepler-1412 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-1412 is classified as a stellar host with an effective photospheric temperature of 5,880 K, a radius of 1.27 R☉, a mass of 1.06 M☉, an estimated bolometric luminosity of 1.73 L☉. Stellar evolution modeling indicates an estimated stellar age of 6.31 Gyr and a metallicity of [Fe/H] = 0.04 dex (near-solar heavy-element abundance). From Earth, Kepler-1412 shines at apparent V-band magnitude 13.347 (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-1412 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,880 K |
| Stellar Radius | 1.2700 R☉ |
| Stellar Mass | 1.0600 M☉ |
| Bolometric Luminosity | 1.73 L☉ |
| Metallicity [Fe/H] | 0.040 dex |
| Stellar Age | 6.310 Gyr |
| Apparent Magnitude | V: 13.347 · G: 13.193 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.046080 AU |
| Orbital Period | 3.615 days |
| Mean Orbital Velocity | 138.7 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.8300° |
| Mean Bulk Density | 4.8 g/cm³ (8.7 km/s vesc) |
| Insolation Flux | 1087.7810 S⊕ (~1,480,470 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 2464.700 LY (755.678 pc) |