Kepler-964 b
Astrophysical Synthesis & Habitability Characterization
Kepler-964 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-964, located approximately 1482.8 light-years (454.63 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0535% across the stellar disk), this world measures 2.12 Earth radii and has a measured mass of 5.14 Earth masses. Combining its mass and radius yields a mean bulk density of 2.97 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.14 g⊕ (11.18 m/s²), and an escape velocity of 17.4 km/s.
In its orbital architecture around Kepler-964, Kepler-964 b completes one full revolution every 13.523 Earth days at a semi-major axis of 0.1073 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 86.3 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 652 K (+379°C / +714°F) and receiving 43.92 S⊕ (~59,770 W/m²), Kepler-964 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-964 is classified as a stellar host with an effective photospheric temperature of 5,427 K, a radius of 0.84 R☉, a mass of 0.93 M☉, an estimated bolometric luminosity of 0.549 L☉. Stellar evolution modeling indicates an estimated stellar age of 1.91 Gyr and a metallicity of [Fe/H] = 0.03 dex (near-solar heavy-element abundance). From Earth, Kepler-964 shines at apparent V-band magnitude 14.061 (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-964 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,427 K |
| Stellar Radius | 0.8400 R☉ |
| Stellar Mass | 0.9300 M☉ |
| Bolometric Luminosity | 0.549 L☉ |
| Metallicity [Fe/H] | 0.030 dex |
| Stellar Age | 1.910 Gyr |
| Apparent Magnitude | V: 14.061 · G: 13.903 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.107300 AU |
| Orbital Period | 13.523 days |
| Mean Orbital Velocity | 86.3 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.5200° |
| Mean Bulk Density | 2.97 g/cm³ (17.4 km/s vesc) |
| Insolation Flux | 43.9160 S⊕ (~59,770 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 1482.800 LY (454.626 pc) |