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CONFIRMED EXOPLANET · Sub-Neptune

K2-317 b

Orbits Host Star: K2-317 · Distance: 575.000 Light-Years (176.291 pc)
Planetary Radius
2.930 R⊕
Planetary Mass
8.910 M⊕
Surface Gravity
1.04 g / g⊕
Equilibrium Temp
432K (+159°C / +318°F)
Orbital Period
6.22 days
Discovery Year
2020 (Transit)
Earth Similarity (ESI)
0.53 / 1.00
Insolation Flux
4.58 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-317 b is a confirmed sub-neptune exoplanet orbiting the star K2-317, located approximately 575 light-years (176.29 parsecs) from the Solar System. First announced in 2020 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.5023% across the stellar disk), this world measures 2.93 Earth radii and has a measured mass of 8.91 Earth masses. Combining its mass and radius yields a mean bulk density of 1.95 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 1.04 g⊕ (10.2 m/s²), and an escape velocity of 19.5 km/s.

In its orbital architecture around K2-317, K2-317 b completes one full revolution every 6.22 Earth days at a semi-major axis of 0.0542 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 94.8 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 432 K (+159°C / +318°F) and receiving 4.58 S⊕ (~6,240 W/m²), K2-317 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-317 is classified as a stellar host with an effective photospheric temperature of 3,387 K, a radius of 0.379 R☉, a mass of 0.403 M☉, an estimated bolometric luminosity of 0.017 L☉. From Earth, K2-317 shines at apparent V-band magnitude 17.74 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.53 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 K2-317
Spectral Type Unclassified
Effective Temp (Teff) 3,387 K
Stellar Radius 0.3790 R☉
Stellar Mass 0.4030 M☉
Bolometric Luminosity 0.017 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 17.740 · G: 16.639
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.054200 AU
Orbital Period 6.22 days
Mean Orbital Velocity 94.8 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 89.2200°
Mean Bulk Density 1.95 g/cm³ (19.5 km/s vesc)
Insolation Flux 4.5848 S⊕ (~6,240 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 575.000 LY (176.291 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 15h14m28.53s · DEC: -21d01m21.80s (J2000: 228.61886°, -21.02272°)
Target Field: K2-317 (J2000 228.61886°, -21.02272°)
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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