Kepler-1453 b

Astrophysical Synthesis & Habitability Characterization

Kepler-1453 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-1453, located approximately 3901 light-years (1196.04 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0678% across the stellar disk), this world measures 2.67 Earth radii and has a measured mass of 7.61 Earth masses. Combining its mass and radius yields a mean bulk density of 2.2 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.07 g⊕ (10.49 m/s²), and an escape velocity of 18.9 km/s.

In its orbital architecture around Kepler-1453, Kepler-1453 b completes one full revolution every 47.161 Earth days at a semi-major axis of 0.262 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 60.4 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 503 K (+230°C / +446°F) and receiving 11.89 S⊕ (~16,181 W/m²), Kepler-1453 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-1453 is classified as a stellar host with an effective photospheric temperature of 5,665 K, a radius of 0.94 R☉, a mass of 0.97 M☉, an estimated bolometric luminosity of 0.816 L☉. Stellar evolution modeling indicates an estimated stellar age of 4.27 Gyr and a metallicity of [Fe/H] = 0.01 dex (near-solar heavy-element abundance). From Earth, Kepler-1453 shines at apparent V-band magnitude 15.695 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

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