Kepler-1600 c
Astrophysical Synthesis & Habitability Characterization
Kepler-1600 c is a confirmed super-earth exoplanet orbiting the star Kepler-1600, located approximately 3362 light-years (1030.81 parsecs) from the Solar System. First announced in 2021 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0456% across the stellar disk), this world measures 1.942 Earth radii and has a measured mass of 4.43 Earth masses. Combining its mass and radius yields a mean bulk density of 3.34 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.17 g⊕ (11.47 m/s²), and an escape velocity of 16.9 km/s.
In its orbital architecture around Kepler-1600, Kepler-1600 c completes one full revolution every 7.298 Earth days at a semi-major axis of 0.06961 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 103.8 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 786 K (+513°C / +955°F) and receiving 84.70 S⊕ (~115,277 W/m²), Kepler-1600 c orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-1600 is classified as a stellar host with an effective photospheric temperature of 5,119 K, a radius of 0.834 R☉, a mass of 0.818 M☉, an estimated bolometric luminosity of 0.429 L☉. Stellar evolution modeling indicates an estimated stellar age of 6.92 Gyr and a metallicity of [Fe/H] = 0.1 dex (metal-rich relative to the Sun). From Earth, Kepler-1600 shines at apparent V-band magnitude 16.076 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The Kepler-1600 system is a multi-planet architecture hosting 2 confirmed worlds, with Kepler-1600 c sharing its stellar neighborhood alongside Kepler-1600 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-1600 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,119 K |
| Stellar Radius | 0.8340 R☉ |
| Stellar Mass | 0.8180 M☉ |
| Bolometric Luminosity | 0.429 L☉ |
| Metallicity [Fe/H] | 0.100 dex |
| Stellar Age | 6.920 Gyr |
| Apparent Magnitude | V: 16.076 · G: 15.814 |
| System Architecture | 1 Star, 2 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.069610 AU |
| Orbital Period | 7.298 days |
| Mean Orbital Velocity | 103.8 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 88.6300° |
| Mean Bulk Density | 3.34 g/cm³ (16.9 km/s vesc) |
| Insolation Flux | 84.7000 S⊕ (~115,277 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 3362.000 LY (1030.810 pc) |