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CONFIRMED EXOPLANET · Terrestrial

Kepler-1423 b

Orbits Host Star: Kepler-1423 · Distance: 1464.400 Light-Years (449.000 pc)
Planetary Radius
1.060 R⊕
Planetary Mass
1.200 M⊕
Surface Gravity
1.07 g / g⊕
Equilibrium Temp
741K (+468°C / +874°F)
Orbital Period
23.955 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.44 / 1.00
Insolation Flux
71.16 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-1423 b is a confirmed terrestrial exoplanet orbiting the star Kepler-1423, located approximately 1464.4 light-years (449 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0168% across the stellar disk), this world measures 1.06 Earth radii and has a measured mass of 1.2 Earth masses. Combining its mass and radius yields a mean bulk density of 5.56 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.07 g⊕ (10.49 m/s²), and an escape velocity of 11.9 km/s.

In its orbital architecture around Kepler-1423, Kepler-1423 b completes one full revolution every 23.955 Earth days at a semi-major axis of 0.1586 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 72 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 741 K (+468°C / +874°F) and receiving 71.16 S⊕ (~96,849 W/m²), Kepler-1423 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-1423 is classified as a stellar host with an effective photospheric temperature of 4,939 K, a radius of 0.75 R☉, a mass of 0.79 M☉, an estimated bolometric luminosity of 0.3 L☉. Stellar evolution modeling indicates an estimated stellar age of 4.68 Gyr and a metallicity of [Fe/H] = -0.02 dex (near-solar heavy-element abundance). From Earth, Kepler-1423 shines at apparent V-band magnitude 14.721 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.44 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-1423
Spectral Type Unclassified
Effective Temp (Teff) 4,939 K
Stellar Radius 0.7500 R☉
Stellar Mass 0.7900 M☉
Bolometric Luminosity 0.3 L☉
Metallicity [Fe/H] -0.020 dex
Stellar Age 4.680 Gyr
Apparent Magnitude V: 14.721 · G: 14.558
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.158600 AU
Orbital Period 23.955 days
Mean Orbital Velocity 72 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 89.1200°
Mean Bulk Density 5.56 g/cm³ (11.9 km/s vesc)
Insolation Flux 71.1600 S⊕ (~96,849 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1464.400 LY (449.000 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h12m58.50s · DEC: +41d06m36.24s (J2000: 288.24375°, 41.11007°)
Target Field: Kepler-1423 (J2000 288.24375°, 41.11007°)
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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