Kepler-349 b
Astrophysical Synthesis & Habitability Characterization
Kepler-349 b is a confirmed super-earth exoplanet orbiting the star Kepler-349, located approximately 3068.2 light-years (940.72 parsecs) from the Solar System. First announced in 2014 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0353% across the stellar disk), this world measures 1.9 Earth radii and has a measured mass of 94.5 Earth masses (0.3 Jupiter masses). Combining its mass and radius yields a mean bulk density of 75.97 g/cm³ (an iron-enriched, high-compression rocky core), a surface gravity of 26.18 g⊕ (256.74 m/s²), and an escape velocity of 78.9 km/s.
In its orbital architecture around Kepler-349, Kepler-349 b completes one full revolution every 5.93 Earth days at a semi-major axis of 0.065 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 119.3 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 972 K (+699°C / +1290°F) and receiving 248.27 S⊕ (~337,901 W/m²), Kepler-349 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-349 is classified as a stellar host with an effective photospheric temperature of 5,956 K, a radius of 0.927 R☉, a mass of 1.083 M☉, an estimated bolometric luminosity of 0.97 L☉. Stellar evolution modeling indicates an estimated stellar age of 0.55 Gyr and a metallicity of [Fe/H] = 0.151 dex (metal-rich relative to the Sun). From Earth, Kepler-349 shines at apparent V-band magnitude 14.915 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The Kepler-349 system is a multi-planet architecture hosting 2 confirmed worlds, with Kepler-349 b sharing its stellar neighborhood alongside Kepler-349 c.
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-349 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,956 K |
| Stellar Radius | 0.9270 R☉ |
| Stellar Mass | 1.0830 M☉ |
| Bolometric Luminosity | 0.97 L☉ |
| Metallicity [Fe/H] | 0.151 dex |
| Stellar Age | 0.550 Gyr |
| Apparent Magnitude | V: 14.915 · G: 14.721 |
| System Architecture | 1 Star, 2 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.065000 AU |
| Orbital Period | 5.93 days |
| Mean Orbital Velocity | 119.3 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.8500° |
| Mean Bulk Density | 75.97 g/cm³ (78.9 km/s vesc) |
| Insolation Flux | 248.2740 S⊕ (~337,901 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 3068.200 LY (940.724 pc) |