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CONFIRMED EXOPLANET · Sub-Neptune

Kepler-608 b

Orbits Host Star: Kepler-608 · Distance: 3087.700 Light-Years (946.683 pc)
Planetary Radius
3.640 R⊕
Planetary Mass
12.900 M⊕
Surface Gravity
0.97 g / g⊕
Equilibrium Temp
1069K (+796°C / +1465°F)
Orbital Period
6.413 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.20 / 1.00
Insolation Flux
270.16 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-608 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-608, located approximately 3087.7 light-years (946.68 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.1092% across the stellar disk), this world measures 3.64 Earth radii (0.32 Jupiter radii) and has a measured mass of 12.9 Earth masses. Combining its mass and radius yields a mean bulk density of 1.47 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.97 g⊕ (9.51 m/s²), and an escape velocity of 21.1 km/s.

In its orbital architecture around Kepler-608, Kepler-608 b completes one full revolution every 6.413 Earth days at a semi-major axis of 0.0685 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 116.2 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 1069 K (+796°C / +1465°F) and receiving 270.16 S⊕ (~367,690 W/m²), Kepler-608 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-608 is classified as a stellar host with an effective photospheric temperature of 5,820 K, a radius of 1.01 R☉, a mass of 1 M☉, an estimated bolometric luminosity of 1.05 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.8 Gyr and a metallicity of [Fe/H] = -0.02 dex (near-solar heavy-element abundance). From Earth, Kepler-608 shines at apparent V-band magnitude 14.84 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.20 Earth Baseline = 1.00
0.00 Dissimilar 0.50 Mars Scale 0.70 Analog Regime 1.00 Earth

Methodology: Computed using the Schulze-Makuch et al. (2011) weighted metric comparing physical interior (radius, estimated density) and surface thermal regime (escape velocity, equilibrium temperature).

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

☀️ Host Star Telemetry

Host Star Name Kepler-608
Spectral Type Unclassified
Effective Temp (Teff) 5,820 K
Stellar Radius 1.0100 R☉
Stellar Mass 1.0000 M☉
Bolometric Luminosity 1.05 L☉
Metallicity [Fe/H] -0.020 dex
Stellar Age 3.800 Gyr
Apparent Magnitude V: 14.840 · G: 14.657
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.068500 AU
Orbital Period 6.413 days
Mean Orbital Velocity 116.2 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 86.1100°
Mean Bulk Density 1.47 g/cm³ (21.1 km/s vesc)
Insolation Flux 270.1620 S⊕ (~367,690 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 3087.700 LY (946.683 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h35m31.90s · DEC: +44d38m17.06s (J2000: 293.8829°, 44.63807°)
Target Field: Kepler-608 (J2000 293.8829°, 44.63807°)
Surveys available: Digitized Sky Survey (DSS2 Optical), 2MASS (Near-Infrared), AllWISE (Mid-Infrared) · Field of View: 0.18° (10.8 arcmin)
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