Kepler-1551 b

Astrophysical Synthesis & Habitability Characterization

Kepler-1551 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-1551, located approximately 4774 light-years (1463.72 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.04% across the stellar disk), this world measures 2.66 Earth radii and has a measured mass of 7.56 Earth masses. Combining its mass and radius yields a mean bulk density of 2.21 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-1551, Kepler-1551 b completes one full revolution every 24.497 Earth days at a semi-major axis of 0.1772 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 722 K (+449°C / +840°F) and receiving 60.42 S⊕ (~82,233 W/m²), Kepler-1551 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-1551 is classified as a stellar host with an effective photospheric temperature of 6,136 K, a radius of 1.22 R☉, a mass of 1.14 M☉, an estimated bolometric luminosity of 1.893 L☉. Stellar evolution modeling indicates an estimated stellar age of 2.88 Gyr and a metallicity of [Fe/H] = 0.01 dex (near-solar heavy-element abundance). From Earth, Kepler-1551 shines at apparent V-band magnitude 15.371 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

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