Kepler-992 b
Astrophysical Synthesis & Habitability Characterization
Kepler-992 b is a confirmed super-earth exoplanet orbiting the star Kepler-992, located approximately 846.8 light-years (259.64 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0403% across the stellar disk), this world measures 1.62 Earth radii and has a measured mass of 3.26 Earth masses. Combining its mass and radius yields a mean bulk density of 4.23 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.24 g⊕ (12.16 m/s²), and an escape velocity of 15.9 km/s.
In its orbital architecture around Kepler-992, Kepler-992 b completes one full revolution every 20.16 Earth days at a semi-major axis of 0.13372 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 72.2 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 510 K (+237°C / +459°F) and receiving 15.29 S⊕ (~20,811 W/m²), Kepler-992 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-992 is classified as a stellar host with an effective photospheric temperature of 4,944 K, a radius of 0.74 R☉, a mass of 0.8 M☉, an estimated bolometric luminosity of 0.294 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.02 Gyr and a metallicity of [Fe/H] = -0.04 dex (near-solar heavy-element abundance). From Earth, Kepler-992 shines at apparent V-band magnitude 13.557 (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-992 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 4,944 K |
| Stellar Radius | 0.7400 R☉ |
| Stellar Mass | 0.8000 M☉ |
| Bolometric Luminosity | 0.294 L☉ |
| Metallicity [Fe/H] | -0.040 dex |
| Stellar Age | 3.020 Gyr |
| Apparent Magnitude | V: 13.557 · G: 13.390 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.133720 AU |
| Orbital Period | 20.16 days |
| Mean Orbital Velocity | 72.2 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 86.3900° |
| Mean Bulk Density | 4.23 g/cm³ (15.9 km/s vesc) |
| Insolation Flux | 15.2910 S⊕ (~20,811 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 846.800 LY (259.639 pc) |