Kepler-757 b
Astrophysical Synthesis & Habitability Characterization
Kepler-757 b is a confirmed super-earth exoplanet orbiting the star Kepler-757, located approximately 3485.6 light-years (1068.68 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0122% across the stellar disk), this world measures 1.36 Earth radii and has a measured mass of 2.42 Earth masses. Combining its mass and radius yields a mean bulk density of 5.3 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 14.9 km/s.
In its orbital architecture around Kepler-757, Kepler-757 b completes one full revolution every 1.023 Earth days at a semi-major axis of 0.019 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 202.1 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 1734 K (+1461°C / +2662°F) and receiving 3,345.45 S⊕ (~4,553,162 W/m²), Kepler-757 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-757 is classified as a stellar host with an effective photospheric temperature of 6,014 K, a radius of 1.13 R☉, a mass of 1.08 M☉, an estimated bolometric luminosity of 1.499 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.31 Gyr and a metallicity of [Fe/H] = 0.02 dex (near-solar heavy-element abundance). From Earth, Kepler-757 shines at apparent V-band magnitude 15.066 (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-757 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 6,014 K |
| Stellar Radius | 1.1300 R☉ |
| Stellar Mass | 1.0800 M☉ |
| Bolometric Luminosity | 1.499 L☉ |
| Metallicity [Fe/H] | 0.020 dex |
| Stellar Age | 3.310 Gyr |
| Apparent Magnitude | V: 15.066 · G: 14.764 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.019000 AU |
| Orbital Period | 1.023 days |
| Mean Orbital Velocity | 202.1 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.8100° |
| Mean Bulk Density | 5.3 g/cm³ (14.9 km/s vesc) |
| Insolation Flux | 3345.4530 S⊕ (~4,553,162 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 3485.600 LY (1068.680 pc) |