Kepler-1097 b

Astrophysical Synthesis & Habitability Characterization

Kepler-1097 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-1097, located approximately 2347.7 light-years (719.8 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.1431% across the stellar disk), this world measures 3.26 Earth radii (0.29 Jupiter radii) and has a measured mass of 10.7 Earth masses. Combining its mass and radius yields a mean bulk density of 1.7 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 1.01 g⊕ (9.9 m/s²), and an escape velocity of 20.3 km/s.

In its orbital architecture around Kepler-1097, Kepler-1097 b completes one full revolution every 187.747 Earth days at a semi-major axis of 0.5791 AU (situated at an orbital separation between Mercury's 0.39 AU and Venus's 0.72 AU). Its mean orbital velocity is approximately 33.6 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.

☁️ Atmospheric Regime (Volatile / Gas Envelope): With a radius of 3.260 R⊕, Kepler-1097 b exceeds the empirical ~1.8–2.2 R⊕ Fulton radius valley threshold, indicating a substantial hydrogen-helium or supercritical volatile envelope without a conventional solid terrestrial surface.

The host star Kepler-1097 is classified as a stellar host with an effective photospheric temperature of 5,211 K, a radius of 0.79 R☉, a mass of 0.82 M☉, an estimated bolometric luminosity of 0.413 L☉. Stellar evolution modeling indicates an estimated stellar age of 4.9 Gyr and a metallicity of [Fe/H] = -0.11 dex (metal-poor relative to the Sun). From Earth, Kepler-1097 shines at apparent V-band magnitude 15.652 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

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