Kepler-1350 c
Astrophysical Synthesis & Habitability Characterization
Kepler-1350 c is a confirmed super-earth exoplanet orbiting the star Kepler-1350, located approximately 1111.2 light-years (340.69 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0896% across the stellar disk), this world measures 1.73 Earth radii and has a measured mass of 3.64 Earth masses. Combining its mass and radius yields a mean bulk density of 3.88 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.22 g⊕ (11.96 m/s²), and an escape velocity of 16.2 km/s.
In its orbital architecture around Kepler-1350, Kepler-1350 c completes one full revolution every 1.767 Earth days at a semi-major axis of 0.0222 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 136.7 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 730 K (+457°C / +855°F) and receiving 94.05 S⊕ (~128,007 W/m²), Kepler-1350 c orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-1350 is classified as a stellar host with an effective photospheric temperature of 3,827 K, a radius of 0.53 R☉, a mass of 0.55 M☉, an estimated bolometric luminosity of 0.054 L☉. Stellar evolution modeling indicates an estimated stellar age of 4.57 Gyr and a metallicity of [Fe/H] = -0.06 dex (near-solar heavy-element abundance). From Earth, Kepler-1350 shines at apparent V-band magnitude 16.577 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The Kepler-1350 system is a multi-planet architecture hosting 2 confirmed worlds, with Kepler-1350 c sharing its stellar neighborhood alongside Kepler-1350 b.
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-1350 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 3,827 K |
| Stellar Radius | 0.5300 R☉ |
| Stellar Mass | 0.5500 M☉ |
| Bolometric Luminosity | 0.054 L☉ |
| Metallicity [Fe/H] | -0.060 dex |
| Stellar Age | 4.570 Gyr |
| Apparent Magnitude | V: 16.577 · G: 16.233 |
| System Architecture | 1 Star, 2 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.022200 AU |
| Orbital Period | 1.767 days |
| Mean Orbital Velocity | 136.7 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.6400° |
| Mean Bulk Density | 3.88 g/cm³ (16.2 km/s vesc) |
| Insolation Flux | 94.0540 S⊕ (~128,007 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 1111.200 LY (340.691 pc) |