Kepler-1013 b

Astrophysical Synthesis & Habitability Characterization

Kepler-1013 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-1013, located approximately 1377.2 light-years (422.25 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0673% across the stellar disk), this world measures 2.15 Earth radii and has a measured mass of 5.27 Earth masses. Combining its mass and radius yields a mean bulk density of 2.92 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.14 g⊕ (11.18 m/s²), and an escape velocity of 17.5 km/s.

In its orbital architecture around Kepler-1013, Kepler-1013 b completes one full revolution every 18.931 Earth days at a semi-major axis of 0.137 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 78.7 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 766 K (+493°C / +919°F) and receiving 16.10 S⊕ (~21,913 W/m²), Kepler-1013 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-1013 is classified as a stellar host with an effective photospheric temperature of 4,954 K, a radius of 0.76 R☉, a mass of 0.81 M☉, an estimated bolometric luminosity of 0.312 L☉. Stellar evolution modeling indicates an estimated stellar age of 4.27 Gyr and a metallicity of [Fe/H] = 0.04 dex (near-solar heavy-element abundance). From Earth, Kepler-1013 shines at apparent V-band magnitude 14.563 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

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