Kepler-374 d
Astrophysical Synthesis & Habitability Characterization
Kepler-374 d is a confirmed super-earth exoplanet orbiting the star Kepler-374, located approximately 4127.9 light-years (1265.61 parsecs) from the Solar System. First announced in 2014 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0174% across the stellar disk), this world measures 1.31 Earth radii and has a measured mass of 2.27 Earth masses. Combining its mass and radius yields a mean bulk density of 5.57 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.32 g⊕ (12.94 m/s²), and an escape velocity of 14.7 km/s.
In its orbital architecture around Kepler-374, Kepler-374 d completes one full revolution every 5.028 Earth days at a semi-major axis of 0.056 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 121.2 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 1272 K (+999°C / +1830°F) and receiving 548.10 S⊕ (~745,963 W/m²), Kepler-374 d orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-374 is classified as a stellar host with an effective photospheric temperature of 5,977 K, a radius of 0.911 R☉, a mass of 1.033 M☉, an estimated bolometric luminosity of 0.95 L☉. Stellar evolution modeling indicates an estimated stellar age of 8.51 Gyr and a metallicity of [Fe/H] = 0.111 dex (metal-rich relative to the Sun). From Earth, Kepler-374 shines at apparent V-band magnitude 14.701 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The Kepler-374 system is a multi-planet architecture hosting 3 confirmed worlds, with Kepler-374 d sharing its stellar neighborhood alongside Kepler-374 b, Kepler-374 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-374 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,977 K |
| Stellar Radius | 0.9110 R☉ |
| Stellar Mass | 1.0330 M☉ |
| Bolometric Luminosity | 0.95 L☉ |
| Metallicity [Fe/H] | 0.111 dex |
| Stellar Age | 8.510 Gyr |
| Apparent Magnitude | V: 14.701 · G: 14.661 |
| System Architecture | 1 Star, 3 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.056000 AU |
| Orbital Period | 5.028 days |
| Mean Orbital Velocity | 121.2 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 88.3700° |
| Mean Bulk Density | 5.57 g/cm³ (14.7 km/s vesc) |
| Insolation Flux | 548.0990 S⊕ (~745,963 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 4127.900 LY (1265.610 pc) |