Kepler-154 b
Astrophysical Synthesis & Habitability Characterization
Kepler-154 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-154, located approximately 2985 light-years (915.21 parsecs) from the Solar System. First announced in 2014 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0428% across the stellar disk), this world measures 2.26 Earth radii and has a measured mass of 5.73 Earth masses. Combining its mass and radius yields a mean bulk density of 2.74 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.12 g⊕ (10.98 m/s²), and an escape velocity of 17.8 km/s.
In its orbital architecture around Kepler-154, Kepler-154 b completes one full revolution every 33.041 Earth days at a semi-major axis of 0.198 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 65.2 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 561 K (+288°C / +550°F) and receiving 28.11 S⊕ (~38,258 W/m²), Kepler-154 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-154 is classified as a stellar host with an effective photospheric temperature of 5,690 K, a radius of 1.001 R☉, a mass of 0.933 M☉, an estimated bolometric luminosity of 0.942 L☉. Stellar evolution modeling indicates an estimated stellar age of 8.91 Gyr and a metallicity of [Fe/H] = 0.02 dex (near-solar heavy-element abundance). From Earth, Kepler-154 shines at apparent V-band magnitude 14.646 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The Kepler-154 system is a multi-planet architecture hosting 5 confirmed worlds, with Kepler-154 b sharing its stellar neighborhood alongside Kepler-154 e, Kepler-154 f, Kepler-154 d, Kepler-154 c.
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-154 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,690 K |
| Stellar Radius | 1.0010 R☉ |
| Stellar Mass | 0.9330 M☉ |
| Bolometric Luminosity | 0.942 L☉ |
| Metallicity [Fe/H] | 0.020 dex |
| Stellar Age | 8.910 Gyr |
| Apparent Magnitude | V: 14.646 · G: 14.512 |
| System Architecture | 1 Star, 5 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.198000 AU |
| Orbital Period | 33.041 days |
| Mean Orbital Velocity | 65.2 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.6500° |
| Mean Bulk Density | 2.74 g/cm³ (17.8 km/s vesc) |
| Insolation Flux | 28.1100 S⊕ (~38,258 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 2985.000 LY (915.212 pc) |