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CONFIRMED EXOPLANET · Sub-Neptune

K2-220 b

Orbits Host Star: K2-220 · Distance: 761.600 Light-Years (233.514 pc)
Planetary Radius
2.370 R⊕
Planetary Mass
6.210 M⊕
Surface Gravity
1.11 g / g⊕
Equilibrium Temp
761K (+488°C / +910°F)
Orbital Period
13.682 days
Discovery Year
2018 (Transit)
Earth Similarity (ESI)
0.34 / 1.00
Insolation Flux
79.70 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-220 b is a confirmed sub-neptune exoplanet orbiting the star K2-220, located approximately 761.6 light-years (233.51 parsecs) from the Solar System. First announced in 2018 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.0448% across the stellar disk), this world measures 2.37 Earth radii and has a measured mass of 6.21 Earth masses. Combining its mass and radius yields a mean bulk density of 2.57 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.11 g⊕ (10.89 m/s²), and an escape velocity of 18.1 km/s.

In its orbital architecture around K2-220, K2-220 b completes one full revolution every 13.682 Earth days at a semi-major axis of 0.1104 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 87.8 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 761 K (+488°C / +910°F) and receiving 79.70 S⊕ (~108,472 W/m²), K2-220 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-220 is classified as a stellar host with an effective photospheric temperature of 5,612 K, a radius of 1.026 R☉, a mass of 0.91 M☉, an estimated bolometric luminosity of 0.937 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.05 dex (near-solar heavy-element abundance). From Earth, K2-220 shines at apparent V-band magnitude 11.873 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.34 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 K2-220
Spectral Type Unclassified
Effective Temp (Teff) 5,612 K
Stellar Radius 1.0260 R☉
Stellar Mass 0.9100 M☉
Bolometric Luminosity 0.937 L☉
Metallicity [Fe/H] -0.050 dex
Stellar Age —
Apparent Magnitude V: 11.873 · G: 11.721
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.110400 AU
Orbital Period 13.682 days
Mean Orbital Velocity 87.8 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.8835°
Mean Bulk Density 2.57 g/cm³ (18.1 km/s vesc)
Insolation Flux 79.7000 S⊕ (~108,472 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 761.600 LY (233.514 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 00h51m04.80s · DEC: +09d31m00.37s (J2000: 12.77001°, 9.51677°)
Target Field: K2-220 (J2000 12.77001°, 9.51677°)
Surveys available: Digitized Sky Survey (DSS2 Optical), 2MASS (Near-Infrared), AllWISE (Mid-Infrared) · Field of View: 0.18° (10.8 arcmin)
Aladin Lite v3 · Centre de Données astronomiques de Strasbourg (CDS)
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