Kepler-1342 b
Astrophysical Synthesis & Habitability Characterization
Kepler-1342 b is a confirmed super-earth exoplanet orbiting the star Kepler-1342, located approximately 2905.1 light-years (890.72 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0286% across the stellar disk), this world measures 1.66 Earth radii and has a measured mass of 3.39 Earth masses. Combining its mass and radius yields a mean bulk density of 4.09 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.23 g⊕ (12.06 m/s²), and an escape velocity of 16 km/s.
In its orbital architecture around Kepler-1342, Kepler-1342 b completes one full revolution every 2.216 Earth days at a semi-major axis of 0.0313 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 153.7 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 1283 K (+1010°C / +1850°F) and receiving 559.28 S⊕ (~761,173 W/m²), Kepler-1342 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-1342 is classified as a stellar host with an effective photospheric temperature of 5,527 K, a radius of 0.9 R☉, a mass of 0.93 M☉, an estimated bolometric luminosity of 0.678 L☉. Stellar evolution modeling indicates an estimated stellar age of 4.37 Gyr and a metallicity of [Fe/H] = 0.03 dex (near-solar heavy-element abundance). From Earth, Kepler-1342 shines at apparent V-band magnitude 15.726 (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-1342 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,527 K |
| Stellar Radius | 0.9000 R☉ |
| Stellar Mass | 0.9300 M☉ |
| Bolometric Luminosity | 0.678 L☉ |
| Metallicity [Fe/H] | 0.030 dex |
| Stellar Age | 4.370 Gyr |
| Apparent Magnitude | V: 15.726 · G: 15.384 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.031300 AU |
| Orbital Period | 2.216 days |
| Mean Orbital Velocity | 153.7 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 82.3000° |
| Mean Bulk Density | 4.09 g/cm³ (16 km/s vesc) |
| Insolation Flux | 559.2750 S⊕ (~761,173 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 2905.100 LY (890.724 pc) |