STATION 02: EXOPLANETLEDGER.ORG · WORLD DOSSIER // Kepler-471 b
← Return to All Worlds
CONFIRMED EXOPLANET · Gas Giant

Kepler-471 b

Orbits Host Star: Kepler-471 · Distance: 4075.000 Light-Years (1249.410 pc)
Planetary Radius
14.960 R⊕
Planetary Mass
—
Surface Gravity
—
Equilibrium Temp
1308K (+1035°C / +1895°F)
Orbital Period
5.014 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.15 / 1.00
Insolation Flux
1,146.88 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-471 b is a confirmed gas giant exoplanet orbiting the star Kepler-471, located approximately 4075 light-years (1249.41 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.5806% across the stellar disk), this world has a measured radius of 14.96 Earth radii (1.33 R♃), though radial-velocity mass constraints remain unmeasured in the current composite catalogue.

In its orbital architecture around Kepler-471, Kepler-471 b completes one full revolution every 5.014 Earth days at a semi-major axis of 0.0626 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 135.8 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 1308 K (+1035°C / +1895°F) and receiving 1,146.88 S⊕ (~1,560,901 W/m²), Kepler-471 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-471 is classified as a stellar host with an effective photospheric temperature of 6,733 K, a radius of 1.8 R☉, a mass of 1.49 M☉, an estimated bolometric luminosity of 5.974 L☉. Stellar evolution modeling indicates an estimated stellar age of 1.58 Gyr and a metallicity of [Fe/H] = 0.07 dex (metal-rich relative to the Sun). From Earth, Kepler-471 shines at apparent V-band magnitude 13.767 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.15 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-471
Spectral Type Unclassified
Effective Temp (Teff) 6,733 K
Stellar Radius 1.8000 R☉
Stellar Mass 1.4900 M☉
Bolometric Luminosity 5.974 L☉
Metallicity [Fe/H] 0.070 dex
Stellar Age 1.580 Gyr
Apparent Magnitude V: 13.767 · G: 13.789
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.062600 AU
Orbital Period 5.014 days
Mean Orbital Velocity 135.8 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 89.5800°
Insolation Flux 1146.8780 S⊕ (~1,560,901 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 4075.000 LY (1249.410 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h56m23.40s · DEC: +43d29m51.31s (J2000: 299.09752°, 43.49759°)
Target Field: Kepler-471 (J2000 299.09752°, 43.49759°)
Surveys available: Digitized Sky Survey (DSS2 Optical), 2MASS (Near-Infrared), AllWISE (Mid-Infrared) · Field of View: 0.18° (10.8 arcmin)
Aladin Lite v3 · Centre de Données astronomiques de Strasbourg (CDS)
SIMBAD Astronomical Query ↗ NASA ADS Research Papers ↗
NASA EXOPLANET ARCHIVE COMPOSITE PARAMETERS
Inspect Raw NASA Archive Record ↗