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CONFIRMED EXOPLANET · Sub-Neptune

Kepler-473 b

Orbits Host Star: Kepler-473 · Distance: 2954.800 Light-Years (905.937 pc)
Planetary Radius
4.080 R⊕
Planetary Mass
15.600 M⊕
Surface Gravity
0.94 g / g⊕
Equilibrium Temp
879K (+606°C / +1123°F)
Orbital Period
14.557 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.23 / 1.00
Insolation Flux
243.38 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-473 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-473, located approximately 2954.8 light-years (905.94 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0779% across the stellar disk), this world measures 4.08 Earth radii (0.36 Jupiter radii) and has a measured mass of 15.6 Earth masses. Combining its mass and radius yields a mean bulk density of 1.27 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.94 g⊕ (9.22 m/s²), and an escape velocity of 21.9 km/s.

In its orbital architecture around Kepler-473, Kepler-473 b completes one full revolution every 14.557 Earth days at a semi-major axis of 0.12048 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 90 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 879 K (+606°C / +1123°F) and receiving 243.38 S⊕ (~331,235 W/m²), Kepler-473 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-473 is classified as a stellar host with an effective photospheric temperature of 5,816 K, a radius of 1.34 R☉, a mass of 1.06 M☉, an estimated bolometric luminosity of 1.843 L☉. Stellar evolution modeling indicates an estimated stellar age of 6.92 Gyr and a metallicity of [Fe/H] = 0.12 dex (metal-rich relative to the Sun). From Earth, Kepler-473 shines at apparent V-band magnitude 13.548 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.23 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-473
Spectral Type Unclassified
Effective Temp (Teff) 5,816 K
Stellar Radius 1.3400 R☉
Stellar Mass 1.0600 M☉
Bolometric Luminosity 1.843 L☉
Metallicity [Fe/H] 0.120 dex
Stellar Age 6.920 Gyr
Apparent Magnitude V: 13.548 · G: 13.369
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.120480 AU
Orbital Period 14.557 days
Mean Orbital Velocity 90 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 89.8600°
Mean Bulk Density 1.27 g/cm³ (21.9 km/s vesc)
Insolation Flux 243.3760 S⊕ (~331,235 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 2954.800 LY (905.937 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h06m31.22s · DEC: +38d56m44.13s (J2000: 286.63008°, 38.94559°)
Target Field: Kepler-473 (J2000 286.63008°, 38.94559°)
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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