STATION 02: EXOPLANETLEDGER.ORG · WORLD DOSSIER // K2-244 b
← Return to All Worlds
CONFIRMED EXOPLANET · Super-Earth

K2-244 b

Orbits Host Star: K2-244 · Distance: 694.400 Light-Years (212.902 pc)
Planetary Radius
1.750 R⊕
Planetary Mass
3.710 M⊕
Surface Gravity
1.21 g / g⊕
Equilibrium Temp
638K (+365°C / +689°F)
Orbital Period
21.069 days
Discovery Year
2018 (Transit)
Earth Similarity (ESI)
0.45 / 1.00
Insolation Flux
37.90 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-244 b is a confirmed super-earth exoplanet orbiting the star K2-244, located approximately 694.4 light-years (212.9 parsecs) from the Solar System. First announced in 2018 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.0304% across the stellar disk), this world measures 1.75 Earth radii and has a measured mass of 3.71 Earth masses. Combining its mass and radius yields a mean bulk density of 3.82 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.21 g⊕ (11.87 m/s²), and an escape velocity of 16.3 km/s.

In its orbital architecture around K2-244, K2-244 b completes one full revolution every 21.069 Earth days at a semi-major axis of 0.1418 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 73.2 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 638 K (+365°C / +689°F) and receiving 37.90 S⊕ (~51,583 W/m²), K2-244 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-244 is classified as a stellar host with an effective photospheric temperature of 5,677 K, a radius of 0.92 R☉, a mass of 0.86 M☉, an estimated bolometric luminosity of 0.789 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.29 dex (metal-poor relative to the Sun). From Earth, K2-244 shines at apparent V-band magnitude 11.78 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.45 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 K2-244
Spectral Type Unclassified
Effective Temp (Teff) 5,677 K
Stellar Radius 0.9200 R☉
Stellar Mass 0.8600 M☉
Bolometric Luminosity 0.789 L☉
Metallicity [Fe/H] -0.290 dex
Stellar Age —
Apparent Magnitude V: 11.780 · G: 11.632
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.141800 AU
Orbital Period 21.069 days
Mean Orbital Velocity 73.2 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 89.2139°
Mean Bulk Density 3.82 g/cm³ (16.3 km/s vesc)
Insolation Flux 37.9007 S⊕ (~51,583 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 694.400 LY (212.902 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 12h13m52.48s · DEC: -03d49m54.51s (J2000: 183.46865°, -3.83181°)
Target Field: K2-244 (J2000 183.46865°, -3.83181°)
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)
SIMBAD Astronomical Query ↗ NASA ADS Research Papers ↗
NASA EXOPLANET ARCHIVE COMPOSITE PARAMETERS
Inspect Raw NASA Archive Record ↗