Kepler-363 b
Astrophysical Synthesis & Habitability Characterization
Kepler-363 b is a confirmed terrestrial exoplanet orbiting the star Kepler-363, located approximately 2487.3 light-years (762.6 parsecs) from the Solar System. First announced in 2014 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0051% across the stellar disk), this world measures 1.16 Earth radii and has a measured mass of 1.65 Earth masses. Combining its mass and radius yields a mean bulk density of 5.83 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 13.3 km/s.
In its orbital architecture around Kepler-363, Kepler-363 b completes one full revolution every 3.615 Earth days at a semi-major axis of 0.048 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 144.5 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 1347 K (+1074°C / +1965°F) and receiving 1,000.24 S⊕ (~1,361,331 W/m²), Kepler-363 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-363 is classified as a stellar host with an effective photospheric temperature of 5,593 K, a radius of 1.485 R☉, a mass of 1.226 M☉, an estimated bolometric luminosity of 1.936 L☉. Stellar evolution modeling indicates an estimated stellar age of 5.5 Gyr and a metallicity of [Fe/H] = 0.397 dex (metal-rich relative to the Sun). From Earth, Kepler-363 shines at apparent V-band magnitude 13.472 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The Kepler-363 system is a multi-planet architecture hosting 3 confirmed worlds, with Kepler-363 b sharing its stellar neighborhood alongside Kepler-363 c, Kepler-363 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-363 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,593 K |
| Stellar Radius | 1.4850 R☉ |
| Stellar Mass | 1.2260 M☉ |
| Bolometric Luminosity | 1.936 L☉ |
| Metallicity [Fe/H] | 0.397 dex |
| Stellar Age | 5.500 Gyr |
| Apparent Magnitude | V: 13.472 · G: 13.316 |
| System Architecture | 1 Star, 3 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.048000 AU |
| Orbital Period | 3.615 days |
| Mean Orbital Velocity | 144.5 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 86.0200° |
| Mean Bulk Density | 5.83 g/cm³ (13.3 km/s vesc) |
| Insolation Flux | 1000.2430 S⊕ (~1,361,331 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 2487.300 LY (762.596 pc) |