Kepler-792 b
Astrophysical Synthesis & Habitability Characterization
Kepler-792 b is a confirmed super-earth exoplanet orbiting the star Kepler-792, located approximately 4649.3 light-years (1425.47 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0257% across the stellar disk), this world measures 1.96 Earth radii and has a measured mass of 4.5 Earth masses. Combining its mass and radius yields a mean bulk density of 3.3 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.17 g⊕ (11.47 m/s²), and an escape velocity of 16.9 km/s.
In its orbital architecture around Kepler-792, Kepler-792 b completes one full revolution every 11.301 Earth days at a semi-major axis of 0.0988 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 95.1 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 852 K (+579°C / +1074°F) and receiving 176.03 S⊕ (~239,580 W/m²), Kepler-792 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-792 is classified as a stellar host with an effective photospheric temperature of 5,971 K, a radius of 1.12 R☉, a mass of 1.09 M☉, an estimated bolometric luminosity of 1.431 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.39 Gyr and a metallicity of [Fe/H] = 0.08 dex (metal-rich relative to the Sun). From Earth, Kepler-792 shines at apparent V-band magnitude 15.117 (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-792 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,971 K |
| Stellar Radius | 1.1200 R☉ |
| Stellar Mass | 1.0900 M☉ |
| Bolometric Luminosity | 1.431 L☉ |
| Metallicity [Fe/H] | 0.080 dex |
| Stellar Age | 3.390 Gyr |
| Apparent Magnitude | V: 15.117 · G: 14.976 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.098800 AU |
| Orbital Period | 11.301 days |
| Mean Orbital Velocity | 95.1 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.6900° |
| Mean Bulk Density | 3.3 g/cm³ (16.9 km/s vesc) |
| Insolation Flux | 176.0320 S⊕ (~239,580 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 4649.300 LY (1425.470 pc) |