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CONFIRMED EXOPLANET · Sub-Neptune

Kepler-681 b

Orbits Host Star: Kepler-681 · Distance: 2240.400 Light-Years (686.923 pc)
Planetary Radius
3.080 R⊕
Planetary Mass
9.690 M⊕
Surface Gravity
1.02 g / g⊕
Equilibrium Temp
489K (+216°C / +421°F)
Orbital Period
26.394 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.47 / 1.00
Insolation Flux
14.15 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-681 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-681, located approximately 2240.4 light-years (686.92 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.138% across the stellar disk), this world measures 3.08 Earth radii (0.27 Jupiter radii) and has a measured mass of 9.69 Earth masses. Combining its mass and radius yields a mean bulk density of 1.83 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 1.02 g⊕ (10 m/s²), and an escape velocity of 19.8 km/s.

In its orbital architecture around Kepler-681, Kepler-681 b completes one full revolution every 26.394 Earth days at a semi-major axis of 0.1635 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 67.4 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 489 K (+216°C / +421°F) and receiving 14.15 S⊕ (~19,260 W/m²), Kepler-681 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-681 is classified as a stellar host with an effective photospheric temperature of 5,021 K, a radius of 0.76 R☉, a mass of 0.8 M☉, an estimated bolometric luminosity of 0.329 L☉. Stellar evolution modeling indicates an estimated stellar age of 5.01 Gyr and a metallicity of [Fe/H] = -0.04 dex (near-solar heavy-element abundance). From Earth, Kepler-681 shines at apparent V-band magnitude 15.584 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.47 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-681
Spectral Type Unclassified
Effective Temp (Teff) 5,021 K
Stellar Radius 0.7600 R☉
Stellar Mass 0.8000 M☉
Bolometric Luminosity 0.329 L☉
Metallicity [Fe/H] -0.040 dex
Stellar Age 5.010 Gyr
Apparent Magnitude V: 15.584 · G: 15.227
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.163500 AU
Orbital Period 26.394 days
Mean Orbital Velocity 67.4 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 89.2800°
Mean Bulk Density 1.83 g/cm³ (19.8 km/s vesc)
Insolation Flux 14.1510 S⊕ (~19,260 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 2240.400 LY (686.923 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h17m35.94s · DEC: +51d15m00.87s (J2000: 289.39974°, 51.25024°)
Target Field: Kepler-681 (J2000 289.39974°, 51.25024°)
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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