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CONFIRMED EXOPLANET · Sub-Neptune

Kepler-893 b

Orbits Host Star: Kepler-893 · Distance: 4193.000 Light-Years (1285.590 pc)
Planetary Radius
3.030 R⊕
Planetary Mass
9.430 M⊕
Surface Gravity
1.03 g / g⊕
Equilibrium Temp
1034K (+761°C / +1402°F)
Orbital Period
6.339 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.22 / 1.00
Insolation Flux
266.27 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-893 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-893, located approximately 4193 light-years (1285.59 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.0787% across the stellar disk), this world measures 3.03 Earth radii (0.27 Jupiter radii) and has a measured mass of 9.43 Earth masses. Combining its mass and radius yields a mean bulk density of 1.87 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 1.03 g⊕ (10.1 m/s²), and an escape velocity of 19.7 km/s.

In its orbital architecture around Kepler-893, Kepler-893 b completes one full revolution every 6.339 Earth days at a semi-major axis of 0.0699 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 120 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 1034 K (+761°C / +1402°F) and receiving 266.27 S⊕ (~362,395 W/m²), Kepler-893 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-893 is classified as a stellar host with an effective photospheric temperature of 5,820 K, a radius of 0.99 R☉, a mass of 1 M☉, an estimated bolometric luminosity of 1.009 L☉. Stellar evolution modeling indicates an estimated stellar age of 3.8 Gyr and a metallicity of [Fe/H] = -0.03 dex (near-solar heavy-element abundance). From Earth, Kepler-893 shines at apparent V-band magnitude 15.347 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.22 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-893
Spectral Type Unclassified
Effective Temp (Teff) 5,820 K
Stellar Radius 0.9900 R☉
Stellar Mass 1.0000 M☉
Bolometric Luminosity 1.009 L☉
Metallicity [Fe/H] -0.030 dex
Stellar Age 3.800 Gyr
Apparent Magnitude V: 15.347 · G: 15.174
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.069900 AU
Orbital Period 6.339 days
Mean Orbital Velocity 120 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 82.4200°
Mean Bulk Density 1.87 g/cm³ (19.7 km/s vesc)
Insolation Flux 266.2710 S⊕ (~362,395 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 4193.000 LY (1285.590 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 18h59m51.13s · DEC: +43d54m46.90s (J2000: 284.96306°, 43.91303°)
Target Field: Kepler-893 (J2000 284.96306°, 43.91303°)
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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