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CONFIRMED EXOPLANET · Super-Earth

K2-322 b

Orbits Host Star: K2-322 · Distance: 402.500 Light-Years (123.415 pc)
Planetary Radius
1.920 R⊕
Planetary Mass
4.350 M⊕
Surface Gravity
1.18 g / g⊕
Equilibrium Temp
635K (+362°C / +684°F)
Orbital Period
8.205 days
Discovery Year
2020 (Transit)
Earth Similarity (ESI)
0.44 / 1.00
Insolation Flux
25.90 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-322 b is a confirmed super-earth exoplanet orbiting the star K2-322, located approximately 402.5 light-years (123.42 parsecs) from the Solar System. First announced in 2020 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.0855% across the stellar disk), this world measures 1.92 Earth radii and has a measured mass of 4.35 Earth masses. Combining its mass and radius yields a mean bulk density of 3.39 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.18 g⊕ (11.57 m/s²), and an escape velocity of 16.8 km/s.

In its orbital architecture around K2-322, K2-322 b completes one full revolution every 8.205 Earth days at a semi-major axis of 0.0594 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 78.8 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 635 K (+362°C / +684°F) and receiving 25.90 S⊕ (~35,256 W/m²), K2-322 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-322 is classified as a stellar host with an effective photospheric temperature of 4,141 K, a radius of 0.602 R☉, a mass of 0.63 M☉, an estimated bolometric luminosity of 0.096 L☉. From Earth, K2-322 shines at apparent V-band magnitude 13.963 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.44 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 K2-322
Spectral Type Unclassified
Effective Temp (Teff) 4,141 K
Stellar Radius 0.6020 R☉
Stellar Mass 0.6300 M☉
Bolometric Luminosity 0.096 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 13.963 · G: 13.311
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.059400 AU
Orbital Period 8.205 days
Mean Orbital Velocity 78.8 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.1500°
Mean Bulk Density 3.39 g/cm³ (16.8 km/s vesc)
Insolation Flux 25.9048 S⊕ (~35,256 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 402.500 LY (123.415 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 10h26m29.45s · DEC: +04d45m50.47s (J2000: 156.6227°, 4.76402°)
Target Field: K2-322 (J2000 156.6227°, 4.76402°)
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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