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CONFIRMED EXOPLANET · Sub-Neptune

K2-202 b

Orbits Host Star: K2-202 · Distance: 979.800 Light-Years (300.397 pc)
Planetary Radius
2.302 R⊕
Planetary Mass
5.910 M⊕
Surface Gravity
1.12 g / g⊕
Equilibrium Temp
—
Orbital Period
3.405 days
Discovery Year
2018 (Transit)
Earth Similarity (ESI)
0.73 / 1.00 Moderate

Astrophysical Synthesis & Habitability Characterization

K2-202 b is a confirmed sub-neptune exoplanet orbiting the star K2-202, located approximately 979.8 light-years (300.4 parsecs) from the Solar System. First announced in 2018 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.0537% across the stellar disk), this world measures 2.302 Earth radii and has a measured mass of 5.91 Earth masses. Combining its mass and radius yields a mean bulk density of 2.67 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.12 g⊕ (10.98 m/s²), and an escape velocity of 17.9 km/s.

In its orbital architecture around K2-202, K2-202 b completes one full revolution every 3.405 Earth days.

☁️ Atmospheric Regime (Volatile / Gas Envelope): With a radius of 2.302 R⊕, K2-202 b exceeds the empirical ~1.8–2.2 R⊕ Fulton radius valley threshold, indicating a substantial hydrogen-helium or supercritical volatile envelope without a conventional solid terrestrial surface.

The host star K2-202 is classified as a stellar host with an effective photospheric temperature of 5,491 K, a radius of 0.9107 R☉, a mass of 0.9715 M☉, an estimated bolometric luminosity of 0.676 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = 0.27 dex (metal-rich relative to the Sun). From Earth, K2-202 shines at apparent V-band magnitude 13.354 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.73 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 K2-202
Spectral Type Unclassified
Effective Temp (Teff) 5,491 K
Stellar Radius 0.9107 R☉
Stellar Mass 0.9715 M☉
Bolometric Luminosity 0.676 L☉
Metallicity [Fe/H] 0.270 dex
Stellar Age —
Apparent Magnitude V: 13.354 · G: 13.044
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 3.405 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 87.6725°
Mean Bulk Density 2.67 g/cm³ (17.9 km/s vesc)
Insolation Flux —
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 979.800 LY (300.397 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 18h53m03.44s · DEC: -22d24m25.40s (J2000: 283.26432°, -22.40706°)
Target Field: K2-202 (J2000 283.26432°, -22.40706°)
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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