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CONFIRMED EXOPLANET · Sub-Neptune

Kepler-943 b

Orbits Host Star: Kepler-943 · Distance: 7503.300 Light-Years (2300.530 pc)
Planetary Radius
5.930 R⊕
Planetary Mass
29.500 M⊕
Surface Gravity
0.84 g / g⊕
Equilibrium Temp
455K (+182°C / +360°F)
Orbital Period
49.77 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.37 / 1.00
Insolation Flux
10.16 S⊕

Astrophysical Synthesis & Habitability Characterization

Kepler-943 b is a confirmed sub-neptune exoplanet orbiting the star Kepler-943, located approximately 7503.3 light-years (2300.53 parsecs) from the Solar System. First announced in 2016 by Kepler using the Transit detection technique (producing an estimated primary transit depth of 0.3569% across the stellar disk), this world measures 5.93 Earth radii (0.53 Jupiter radii) and has a measured mass of 29.5 Earth masses. Combining its mass and radius yields a mean bulk density of 0.78 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.84 g⊕ (8.24 m/s²), and an escape velocity of 24.9 km/s.

In its orbital architecture around Kepler-943, Kepler-943 b completes one full revolution every 49.77 Earth days at a semi-major axis of 0.2559 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 55.9 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 455 K (+182°C / +360°F) and receiving 10.16 S⊕ (~13,828 W/m²), Kepler-943 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star Kepler-943 is classified as a stellar host with an effective photospheric temperature of 5,612 K, a radius of 0.91 R☉, a mass of 0.93 M☉, an estimated bolometric luminosity of 0.737 L☉. Stellar evolution modeling indicates an estimated stellar age of 4.27 Gyr and a metallicity of [Fe/H] = -0.07 dex (near-solar heavy-element abundance). From Earth, Kepler-943 shines at apparent V-band magnitude 15.76 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.37 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-943
Spectral Type Unclassified
Effective Temp (Teff) 5,612 K
Stellar Radius 0.9100 R☉
Stellar Mass 0.9300 M☉
Bolometric Luminosity 0.737 L☉
Metallicity [Fe/H] -0.070 dex
Stellar Age 4.270 Gyr
Apparent Magnitude V: 15.760 · G: 15.639
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.255900 AU
Orbital Period 49.77 days
Mean Orbital Velocity 55.9 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 88.8000°
Mean Bulk Density 0.78 g/cm³ (24.9 km/s vesc)
Insolation Flux 10.1600 S⊕ (~13,828 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 7503.300 LY (2300.530 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 18h57m05.74s · DEC: +41d32m05.93s (J2000: 284.27393°, 41.53498°)
Target Field: Kepler-943 (J2000 284.27393°, 41.53498°)
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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