Kepler-1629 b
Astrophysical Synthesis & Habitability Characterization
Kepler-1629 b is a confirmed sub-earth exoplanet orbiting the star Kepler-1629, located approximately 1096.2 light-years (336.09 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0049% across the stellar disk), this world measures 0.77 Earth radii and has a measured mass of 0.381 Earth masses. Combining its mass and radius yields a mean bulk density of 4.6 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 0.64 g⊕ (6.28 m/s²), and an escape velocity of 7.9 km/s.
In its orbital architecture around Kepler-1629, Kepler-1629 b completes one full revolution every 3.876 Earth days at a semi-major axis of 0.0485 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 136.1 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 1081 K (+808°C / +1486°F) and receiving 315.46 S⊕ (~429,337 W/m²), Kepler-1629 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-1629 is classified as a stellar host with an effective photospheric temperature of 5,776 K, a radius of 1.01 R☉, a mass of 1.01 M☉, an estimated bolometric luminosity of 1.019 L☉. Stellar evolution modeling indicates an estimated stellar age of 4.27 Gyr and a metallicity of [Fe/H] = 0.05 dex (near-solar heavy-element abundance). From Earth, Kepler-1629 shines at apparent V-band magnitude 12.786 (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-1629 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,776 K |
| Stellar Radius | 1.0100 R☉ |
| Stellar Mass | 1.0100 M☉ |
| Bolometric Luminosity | 1.019 L☉ |
| Metallicity [Fe/H] | 0.050 dex |
| Stellar Age | 4.270 Gyr |
| Apparent Magnitude | V: 12.786 · G: 12.714 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.048500 AU |
| Orbital Period | 3.876 days |
| Mean Orbital Velocity | 136.1 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.8900° |
| Mean Bulk Density | 4.6 g/cm³ (7.9 km/s vesc) |
| Insolation Flux | 315.4570 S⊕ (~429,337 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 1096.200 LY (336.090 pc) |