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CONFIRMED EXOPLANET · Sub-Neptune

Kepler-711 b

Orbits Host Star: Kepler-711 · Distance: 2037.100 Light-Years (624.575 pc)
Planetary Radius
3.410 R⊕
Planetary Mass
11.500 M⊕
Surface Gravity
0.99 g / g⊕
Equilibrium Temp
487K (+214°C / +417°F)
Orbital Period
23.589 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.45 / 1.00
Insolation Flux
15.57 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-711 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-711, located approximately 2037.1 light-years (624.58 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.1527% across the stellar disk), this world measures 3.41 Earth radii (0.3 Jupiter radii) and has a measured mass of 11.5 Earth masses. Combining its mass and radius yields a mean bulk density of 1.6 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.99 g⊕ (9.71 m/s²), and an escape velocity of 20.5 km/s.

In its orbital architecture around Kepler-711, Kepler-711 b completes one full revolution every 23.589 Earth days at a semi-major axis of 0.1429 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 65.9 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 487 K (+214°C / +417°F) and receiving 15.57 S⊕ (~21,189 W/m²), Kepler-711 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-711 is classified as a stellar host with an effective photospheric temperature of 5,222 K, a radius of 0.8 R☉, a mass of 0.84 M☉, an estimated bolometric luminosity of 0.427 L☉. Stellar evolution modeling indicates an estimated stellar age of 4.37 Gyr and a metallicity of [Fe/H] = -0.04 dex (near-solar heavy-element abundance). From Earth, Kepler-711 shines at apparent V-band magnitude 15.635 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.45 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-711
Spectral Type Unclassified
Effective Temp (Teff) 5,222 K
Stellar Radius 0.8000 R☉
Stellar Mass 0.8400 M☉
Bolometric Luminosity 0.427 L☉
Metallicity [Fe/H] -0.040 dex
Stellar Age 4.370 Gyr
Apparent Magnitude V: 15.635 · G: 15.329
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.142900 AU
Orbital Period 23.589 days
Mean Orbital Velocity 65.9 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 86.8600°
Mean Bulk Density 1.6 g/cm³ (20.5 km/s vesc)
Insolation Flux 15.5690 S⊕ (~21,189 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 2037.100 LY (624.575 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h49m50.41s · DEC: +42d50m23.34s (J2000: 297.46005°, 42.83982°)
Target Field: Kepler-711 (J2000 297.46005°, 42.83982°)
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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