Kepler-1437 b
Astrophysical Synthesis & Habitability Characterization
Kepler-1437 b is a confirmed super-earth exoplanet orbiting the star Kepler-1437, located approximately 6854.8 light-years (2101.69 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0195% across the stellar disk), this world measures 1.37 Earth radii and has a measured mass of 2.45 Earth masses. Combining its mass and radius yields a mean bulk density of 5.25 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.31 g⊕ (12.85 m/s²), and an escape velocity of 15 km/s.
In its orbital architecture around Kepler-1437, Kepler-1437 b completes one full revolution every 10.93 Earth days at a semi-major axis of 0.0951 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 94.7 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 770 K (+497°C / +927°F) and receiving 83.14 S⊕ (~113,154 W/m²), Kepler-1437 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-1437 is classified as a stellar host with an effective photospheric temperature of 5,557 K, a radius of 0.9 R☉, a mass of 0.93 M☉, an estimated bolometric luminosity of 0.693 L☉. Stellar evolution modeling indicates an estimated stellar age of 4.57 Gyr and a metallicity of [Fe/H] = -0.02 dex (near-solar heavy-element abundance). From Earth, Kepler-1437 shines at apparent V-band magnitude 15.701 (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-1437 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,557 K |
| Stellar Radius | 0.9000 R☉ |
| Stellar Mass | 0.9300 M☉ |
| Bolometric Luminosity | 0.693 L☉ |
| Metallicity [Fe/H] | -0.020 dex |
| Stellar Age | 4.570 Gyr |
| Apparent Magnitude | V: 15.701 · G: 15.661 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.095100 AU |
| Orbital Period | 10.93 days |
| Mean Orbital Velocity | 94.7 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.2000° |
| Mean Bulk Density | 5.25 g/cm³ (15 km/s vesc) |
| Insolation Flux | 83.1400 S⊕ (~113,154 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 6854.800 LY (2101.690 pc) |