Kepler-332 c
Astrophysical Synthesis & Habitability Characterization
Kepler-332 c is a confirmed terrestrial exoplanet orbiting the star Kepler-332, located approximately 1122.6 light-years (344.19 parsecs) from the Solar System. First announced in 2014 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0193% across the stellar disk), this world measures 1.09 Earth radii and has a measured mass of 1.32 Earth masses. Combining its mass and radius yields a mean bulk density of 5.62 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.11 g⊕ (10.89 m/s²), and an escape velocity of 12.3 km/s.
In its orbital architecture around Kepler-332, Kepler-332 c completes one full revolution every 15.996 Earth days at a semi-major axis of 0.114 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 77.5 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 550 K (+277°C / +531°F) and receiving 19.99 S⊕ (~27,201 W/m²), Kepler-332 c orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-332 is classified as a stellar host with an effective photospheric temperature of 4,955 K, a radius of 0.72 R☉, a mass of 0.743 M☉, an estimated bolometric luminosity of 0.28 L☉. Stellar evolution modeling indicates an estimated stellar age of 2.82 Gyr and a metallicity of [Fe/H] = -0.13 dex (metal-poor relative to the Sun). From Earth, Kepler-332 shines at apparent V-band magnitude 14.243 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The Kepler-332 system is a multi-planet architecture hosting 3 confirmed worlds, with Kepler-332 c sharing its stellar neighborhood alongside Kepler-332 b, Kepler-332 d.
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-332 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 4,955 K |
| Stellar Radius | 0.7200 R☉ |
| Stellar Mass | 0.7430 M☉ |
| Bolometric Luminosity | 0.28 L☉ |
| Metallicity [Fe/H] | -0.130 dex |
| Stellar Age | 2.820 Gyr |
| Apparent Magnitude | V: 14.243 · G: 14.003 |
| System Architecture | 1 Star, 3 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.114000 AU |
| Orbital Period | 15.996 days |
| Mean Orbital Velocity | 77.5 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.8600° |
| Mean Bulk Density | 5.62 g/cm³ (12.3 km/s vesc) |
| Insolation Flux | 19.9860 S⊕ (~27,201 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 1122.600 LY (344.190 pc) |