Kepler-797 b
Astrophysical Synthesis & Habitability Characterization
Kepler-797 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-797, located approximately 4289.8 light-years (1315.26 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0439% across the stellar disk), this world measures 2.17 Earth radii and has a measured mass of 5.35 Earth masses. Combining its mass and radius yields a mean bulk density of 2.89 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.14 g⊕ (11.18 m/s²), and an escape velocity of 17.6 km/s.
In its orbital architecture around Kepler-797, Kepler-797 b completes one full revolution every 27.072 Earth days at a semi-major axis of 0.181 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 72.7 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 605 K (+332°C / +630°F) and receiving 90.10 S⊕ (~122,626 W/m²), Kepler-797 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-797 is classified as a stellar host with an effective photospheric temperature of 5,680 K, a radius of 0.95 R☉, a mass of 0.96 M☉, an estimated bolometric luminosity of 0.843 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.89 Gyr and a metallicity of [Fe/H] = -0.02 dex (near-solar heavy-element abundance). From Earth, Kepler-797 shines at apparent V-band magnitude 14.751 (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-797 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,680 K |
| Stellar Radius | 0.9500 R☉ |
| Stellar Mass | 0.9600 M☉ |
| Bolometric Luminosity | 0.843 L☉ |
| Metallicity [Fe/H] | -0.020 dex |
| Stellar Age | 3.890 Gyr |
| Apparent Magnitude | V: 14.751 · G: 14.542 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.181000 AU |
| Orbital Period | 27.072 days |
| Mean Orbital Velocity | 72.7 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.9700° |
| Mean Bulk Density | 2.89 g/cm³ (17.6 km/s vesc) |
| Insolation Flux | 90.1000 S⊕ (~122,626 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 4289.800 LY (1315.260 pc) |