Kepler-1255 b

Astrophysical Synthesis & Habitability Characterization

Kepler-1255 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-1255, located approximately 5274.2 light-years (1617.07 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0361% across the stellar disk), this world measures 2.32 Earth radii and has a measured mass of 5.99 Earth masses. Combining its mass and radius yields a mean bulk density of 2.65 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.11 g⊕ (10.89 m/s²), and an escape velocity of 18 km/s.

In its orbital architecture around Kepler-1255, Kepler-1255 b completes one full revolution every 36.292 Earth days at a semi-major axis of 0.2226 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 66.7 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 694 K (+421°C / +790°F) and receiving 39.67 S⊕ (~53,992 W/m²), Kepler-1255 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-1255 is classified as a stellar host with an effective photospheric temperature of 6,018 K, a radius of 1.12 R☉, a mass of 1.08 M☉, an estimated bolometric luminosity of 1.476 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.55 Gyr and a metallicity of [Fe/H] = 0.02 dex (near-solar heavy-element abundance). From Earth, Kepler-1255 shines at apparent V-band magnitude 15.308 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Discovery Facility: Kepler · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).