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CONFIRMED EXOPLANET · Sub-Neptune

K2-66 b

Orbits Host Star: K2-66 · Distance: 1676.000 Light-Years (513.877 pc)
Planetary Radius
2.490 R⊕
Planetary Mass
21.300 M⊕
Surface Gravity
3.44 g / g⊕
Equilibrium Temp
1372K (+1099°C / +2010°F)
Orbital Period
5.07 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.18 / 1.00
Insolation Flux
840.00 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-66 b is a confirmed sub-neptune exoplanet orbiting the star K2-66, located approximately 1676 light-years (513.88 parsecs) from the Solar System. First announced in 2016 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.0187% across the stellar disk), this world measures 2.49 Earth radii and has a measured mass of 21.3 Earth masses. Combining its mass and radius yields a mean bulk density of 7.61 g/cm³ (an iron-enriched, high-compression rocky core), a surface gravity of 3.44 g⊕ (33.73 m/s²), and an escape velocity of 32.7 km/s.

In its orbital architecture around K2-66, K2-66 b completes one full revolution every 5.07 Earth days at a semi-major axis of 0.05983 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 128.4 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 1372 K (+1099°C / +2010°F) and receiving 840.00 S⊕ (~1,143,240 W/m²), K2-66 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-66 is classified as a stellar host with an effective photospheric temperature of 5,887 K, a radius of 1.67 R☉, a mass of 1.11 M☉, an estimated bolometric luminosity of 3.005 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.047 dex (near-solar heavy-element abundance). From Earth, K2-66 shines at apparent V-band magnitude 11.71 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.18 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: K2 · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name K2-66
Spectral Type Unclassified
Effective Temp (Teff) 5,887 K
Stellar Radius 1.6700 R☉
Stellar Mass 1.1100 M☉
Bolometric Luminosity 3.005 L☉
Metallicity [Fe/H] -0.047 dex
Stellar Age —
Apparent Magnitude V: 11.710 · G: 11.996
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.059830 AU
Orbital Period 5.07 days
Mean Orbital Velocity 128.4 km/s
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 86.6000°
Mean Bulk Density 7.61 g/cm³ (32.7 km/s vesc)
Insolation Flux 840.0000 S⊕ (~1,143,240 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1676.000 LY (513.877 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 22h06m06.40s · DEC: -10d42m41.53s (J2000: 331.52666°, -10.71154°)
Target Field: K2-66 (J2000 331.52666°, -10.71154°)
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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