Kepler-1082 b
Astrophysical Synthesis & Habitability Characterization
Kepler-1082 b is a confirmed terrestrial exoplanet orbiting the star Kepler-1082, located approximately 2412.1 light-years (739.56 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0081% across the stellar disk), this world measures 1.12 Earth radii and has a measured mass of 1.46 Earth masses. Combining its mass and radius yields a mean bulk density of 5.73 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.16 g⊕ (11.38 m/s²), and an escape velocity of 12.8 km/s.
In its orbital architecture around Kepler-1082, Kepler-1082 b completes one full revolution every 1.543 Earth days at a semi-major axis of 0.02571 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 181.2 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 1827 K (+1554°C / +2829°F) and receiving 2,949.56 S⊕ (~4,014,347 W/m²), Kepler-1082 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-1082 is classified as a stellar host with an effective photospheric temperature of 5,923 K, a radius of 1.14 R☉, a mass of 1.03 M☉, an estimated bolometric luminosity of 1.435 L☉. Stellar evolution modeling indicates an estimated stellar age of 5.75 Gyr and a metallicity of [Fe/H] = -0.06 dex (near-solar heavy-element abundance). From Earth, Kepler-1082 shines at apparent V-band magnitude 13.444 (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-1082 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,923 K |
| Stellar Radius | 1.1400 R☉ |
| Stellar Mass | 1.0300 M☉ |
| Bolometric Luminosity | 1.435 L☉ |
| Metallicity [Fe/H] | -0.060 dex |
| Stellar Age | 5.750 Gyr |
| Apparent Magnitude | V: 13.444 · G: 13.342 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.025710 AU |
| Orbital Period | 1.543 days |
| Mean Orbital Velocity | 181.2 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 87.2600° |
| Mean Bulk Density | 5.73 g/cm³ (12.8 km/s vesc) |
| Insolation Flux | 2949.5570 S⊕ (~4,014,347 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 2412.100 LY (739.557 pc) |