Kepler-1524 b

Astrophysical Synthesis & Habitability Characterization

Kepler-1524 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-1524, located approximately 1245.2 light-years (381.77 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0674% across the stellar disk), this world measures 3.54 Earth radii (0.32 Jupiter radii) and has a measured mass of 12.3 Earth masses. Combining its mass and radius yields a mean bulk density of 1.53 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.98 g⊕ (9.61 m/s²), and an escape velocity of 20.9 km/s.

In its orbital architecture around Kepler-1524, Kepler-1524 b completes one full revolution every 70.967 Earth days at a semi-major axis of 0.3392 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 52 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 438 K (+165°C / +329°F) and receiving 8.44 S⊕ (~11,491 W/m²), Kepler-1524 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-1524 is classified as a stellar host with an effective photospheric temperature of 6,179 K, a radius of 1.25 R☉, a mass of 1.17 M☉, an estimated bolometric luminosity of 2.044 L☉. Stellar evolution modeling indicates an estimated stellar age of 2.88 Gyr and a metallicity of [Fe/H] = 0.04 dex (near-solar heavy-element abundance). From Earth, Kepler-1524 shines at apparent V-band magnitude 12.802 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

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