Kepler-1685 b

Astrophysical Synthesis & Habitability Characterization

Kepler-1685 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-1685, located approximately 3724.3 light-years (1141.89 parsecs) from the Solar System. First announced in 2020 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.08% across the stellar disk), this world measures 2.577 Earth radii and has a measured mass of 7.16 Earth masses. Combining its mass and radius yields a mean bulk density of 2.31 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.08 g⊕ (10.59 m/s²), and an escape velocity of 18.6 km/s.

In its orbital architecture around Kepler-1685, Kepler-1685 b completes one full revolution every 20.491 Earth days at a semi-major axis of 0.1485 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 78.8 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 625 K (+352°C / +666°F) and receiving 36.01 S⊕ (~49,010 W/m²), Kepler-1685 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-1685 is classified as a stellar host with an effective photospheric temperature of 5,484 K, a radius of 0.8355 R☉, a mass of 0.96 M☉, an estimated bolometric luminosity of 0.566 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = 0.21 dex (metal-rich relative to the Sun). From Earth, Kepler-1685 shines at apparent V-band magnitude 16.096 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

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