Kepler-1584 b

Astrophysical Synthesis & Habitability Characterization

Kepler-1584 b is a confirmed super-earth exoplanet orbiting the star Kepler-1584, located approximately 4619.4 light-years (1416.31 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0171% across the stellar disk), this world measures 1.61 Earth radii and has a measured mass of 3.22 Earth masses. Combining its mass and radius yields a mean bulk density of 4.25 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.24 g⊕ (12.16 m/s²), and an escape velocity of 15.8 km/s.

In its orbital architecture around Kepler-1584, Kepler-1584 b completes one full revolution every 13.4 Earth days at a semi-major axis of 0.1168 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 94.8 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 886 K (+613°C / +1135°F) and receiving 162.54 S⊕ (~221,222 W/m²), Kepler-1584 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-1584 is classified as a stellar host with an effective photospheric temperature of 6,069 K, a radius of 1.13 R☉, a mass of 1.1 M☉, an estimated bolometric luminosity of 1.554 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.31 Gyr and a metallicity of [Fe/H] = 0 dex (near-solar heavy-element abundance). From Earth, Kepler-1584 shines at apparent V-band magnitude 15.105 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

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