Kepler-385 b
Astrophysical Synthesis & Habitability Characterization
Kepler-385 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-385, located approximately 4672.5 light-years (1432.61 parsecs) from the Solar System. First announced in 2014 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0494% across the stellar disk), this world measures 2.73 Earth radii and has a measured mass of 12.8 Earth masses. Combining its mass and radius yields a mean bulk density of 3.47 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.72 g⊕ (16.87 m/s²), and an escape velocity of 24.2 km/s.
In its orbital architecture around Kepler-385, Kepler-385 b completes one full revolution every 10.044 Earth days at a semi-major axis of 0.097 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 105.1 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 951 K (+678°C / +1252°F) and receiving 143.92 S⊕ (~195,874 W/m²), Kepler-385 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-385 is classified as a stellar host with an effective photospheric temperature of 6,326 K, a radius of 1.126 R☉, a mass of 0.992 M☉, an estimated bolometric luminosity of 1.822 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.31 Gyr and a metallicity of [Fe/H] = 0.01 dex (near-solar heavy-element abundance). From Earth, Kepler-385 shines at apparent V-band magnitude 15.76 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The Kepler-385 system is a multi-planet architecture hosting 3 confirmed worlds, with Kepler-385 b sharing its stellar neighborhood alongside Kepler-385 c, Kepler-385 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-385 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 6,326 K |
| Stellar Radius | 1.1260 R☉ |
| Stellar Mass | 0.9920 M☉ |
| Bolometric Luminosity | 1.822 L☉ |
| Metallicity [Fe/H] | 0.010 dex |
| Stellar Age | 3.310 Gyr |
| Apparent Magnitude | V: 15.760 · G: 15.192 |
| System Architecture | 1 Star, 3 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.097000 AU |
| Orbital Period | 10.044 days |
| Mean Orbital Velocity | 105.1 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 79.6400° |
| Mean Bulk Density | 3.47 g/cm³ (24.2 km/s vesc) |
| Insolation Flux | 143.9190 S⊕ (~195,874 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 4672.500 LY (1432.610 pc) |