Kepler-1149 b
Astrophysical Synthesis & Habitability Characterization
Kepler-1149 b is a confirmed super-earth exoplanet orbiting the star Kepler-1149, located approximately 3971.7 light-years (1217.73 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0171% across the stellar disk), this world measures 1.44 Earth radii and has a measured mass of 2.67 Earth masses. Combining its mass and radius yields a mean bulk density of 4.93 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.29 g⊕ (12.65 m/s²), and an escape velocity of 15.2 km/s.
In its orbital architecture around Kepler-1149, Kepler-1149 b completes one full revolution every 3.731 Earth days at a semi-major axis of 0.0473 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 137.9 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 1128 K (+855°C / +1571°F) and receiving 653.83 S⊕ (~889,864 W/m²), Kepler-1149 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-1149 is classified as a stellar host with an effective photospheric temperature of 5,833 K, a radius of 1.01 R☉, a mass of 1.02 M☉, an estimated bolometric luminosity of 1.059 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.98 Gyr and a metallicity of [Fe/H] = 0.02 dex (near-solar heavy-element abundance). From Earth, Kepler-1149 shines at apparent V-band magnitude 15.146 (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-1149 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,833 K |
| Stellar Radius | 1.0100 R☉ |
| Stellar Mass | 1.0200 M☉ |
| Bolometric Luminosity | 1.059 L☉ |
| Metallicity [Fe/H] | 0.020 dex |
| Stellar Age | 3.980 Gyr |
| Apparent Magnitude | V: 15.146 · G: 14.931 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.047300 AU |
| Orbital Period | 3.731 days |
| Mean Orbital Velocity | 137.9 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 81.9800° |
| Mean Bulk Density | 4.93 g/cm³ (15.2 km/s vesc) |
| Insolation Flux | 653.8310 S⊕ (~889,864 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 3971.700 LY (1217.730 pc) |