Kepler-889 b
Astrophysical Synthesis & Habitability Characterization
Kepler-889 b is a confirmed terrestrial exoplanet orbiting the star Kepler-889, located approximately 1951.4 light-years (598.31 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0064% across the stellar disk), this world measures 1.09 Earth radii and has a measured mass of 1.32 Earth masses. Combining its mass and radius yields a mean bulk density of 5.62 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.11 g⊕ (10.89 m/s²), and an escape velocity of 12.3 km/s.
In its orbital architecture around Kepler-889, Kepler-889 b completes one full revolution every 3.744 Earth days at a semi-major axis of 0.04975 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 144.5 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 1328 K (+1055°C / +1931°F) and receiving 954.59 S⊕ (~1,299,194 W/m²), Kepler-889 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-889 is classified as a stellar host with an effective photospheric temperature of 5,961 K, a radius of 1.25 R☉, a mass of 1.14 M☉, an estimated bolometric luminosity of 1.77 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.98 Gyr and a metallicity of [Fe/H] = 0.19 dex (metal-rich relative to the Sun). From Earth, Kepler-889 shines at apparent V-band magnitude 12.998 (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-889 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,961 K |
| Stellar Radius | 1.2500 R☉ |
| Stellar Mass | 1.1400 M☉ |
| Bolometric Luminosity | 1.77 L☉ |
| Metallicity [Fe/H] | 0.190 dex |
| Stellar Age | 3.980 Gyr |
| Apparent Magnitude | V: 12.998 · G: 12.680 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.049750 AU |
| Orbital Period | 3.744 days |
| Mean Orbital Velocity | 144.5 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.0100° |
| Mean Bulk Density | 5.62 g/cm³ (12.3 km/s vesc) |
| Insolation Flux | 954.5880 S⊕ (~1,299,194 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 1951.400 LY (598.313 pc) |