Kepler-1458 b

Astrophysical Synthesis & Habitability Characterization

Kepler-1458 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-1458, located approximately 1775.8 light-years (544.45 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0725% across the stellar disk), this world measures 2.76 Earth radii and has a measured mass of 8.05 Earth masses. Combining its mass and radius yields a mean bulk density of 2.11 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.06 g⊕ (10.4 m/s²), and an escape velocity of 19.1 km/s.

In its orbital architecture around Kepler-1458, Kepler-1458 b completes one full revolution every 47.987 Earth days at a semi-major axis of 0.24869 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 56.4 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 493 K (+220°C / +428°F) and receiving 8.29 S⊕ (~11,287 W/m²), Kepler-1458 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-1458 is classified as a stellar host with an effective photospheric temperature of 5,653 K, a radius of 0.94 R☉, a mass of 0.96 M☉, an estimated bolometric luminosity of 0.81 L☉. Stellar evolution modeling indicates an estimated stellar age of 4.17 Gyr and a metallicity of [Fe/H] = 0.02 dex (near-solar heavy-element abundance). From Earth, Kepler-1458 shines at apparent V-band magnitude 14.434 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

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