Kepler-1900 b
Astrophysical Synthesis & Habitability Characterization
Kepler-1900 b is a confirmed super-earth exoplanet orbiting the star Kepler-1900, located approximately 5024.2 light-years (1540.43 parsecs) from the Solar System. First announced in 2021 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0204% across the stellar disk), this world measures 1.623 Earth radii and has a measured mass of 3.27 Earth masses. Combining its mass and radius yields a mean bulk density of 4.22 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.24 g⊕ (12.16 m/s²), and an escape velocity of 15.9 km/s.
In its orbital architecture around Kepler-1900, Kepler-1900 b completes one full revolution every 2.986 Earth days at a semi-major axis of 0.042 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 153 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 1356 K (+1083°C / +1981°F) and receiving 798.35 S⊕ (~1,086,554 W/m²), Kepler-1900 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star Kepler-1900 is classified as a stellar host with an effective photospheric temperature of 6,173 K, a radius of 1.041 R☉, a mass of 1.104 M☉, an estimated bolometric luminosity of 1.412 L☉. Stellar evolution modeling indicates an estimated stellar age of 0.4 Gyr and a metallicity of [Fe/H] = -0.04 dex (near-solar heavy-element abundance). From Earth, Kepler-1900 shines at apparent V-band magnitude 15.502 (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-1900 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 6,173 K |
| Stellar Radius | 1.0410 R☉ |
| Stellar Mass | 1.1040 M☉ |
| Bolometric Luminosity | 1.412 L☉ |
| Metallicity [Fe/H] | -0.040 dex |
| Stellar Age | 0.400 Gyr |
| Apparent Magnitude | V: 15.502 · G: 15.282 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.042000 AU |
| Orbital Period | 2.986 days |
| Mean Orbital Velocity | 153 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 88.1100° |
| Mean Bulk Density | 4.22 g/cm³ (15.9 km/s vesc) |
| Insolation Flux | 798.3500 S⊕ (~1,086,554 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 5024.200 LY (1540.430 pc) |