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CONFIRMED EXOPLANET · Gas Giant

2MASS J22362452+4751425 b

Orbits Host Star: 2MASS J22362452+4751425 (Type K7 V) · Distance: 226.900 Light-Years (69.574 pc)
Planetary Radius
12.300 R⊕
Planetary Mass
3972.875 M⊕
Surface Gravity
26.26 g / g⊕
Equilibrium Temp
10K (-263°C / -441°F)
Orbital Period
—
Discovery Year
2016 (Imaging)
Earth Similarity (ESI)
0.01 / 1.00
Insolation Flux
0.00 S⊕

Astrophysical Synthesis & Habitability Characterization

2MASS J22362452+4751425 b is a confirmed gas giant exoplanet orbiting the star 2MASS J22362452+4751425, located approximately 226.9 light-years (69.57 parsecs) from the Solar System. First announced in 2016 by W. M. Keck Observatory using the Imaging detection technique (resolved directly via high-contrast coronagraphic or interferometric imaging), this world measures 12.3 Earth radii (1.1 Jupiter radii) and has a measured mass of 3972.875 Earth masses (12.5 Jupiter masses). Combining its mass and radius yields a mean bulk density of 11.77 g/cm³ (an iron-enriched, high-compression rocky core), a surface gravity of 26.26 g⊕ (257.52 m/s²), and an escape velocity of 201 km/s.

❄️ Thermal Regime (Cryogenic Zone): With an equilibrium temperature of 10 K (-263°C / -441°F), surface water and volatile species on 2MASS J22362452+4751425 b would remain locked in cryogenic ice phases unless warmed by subsurface tidal or radiogenic heating.

The host star 2MASS J22362452+4751425 is classified as an orange K-type star of spectral type K7 V with an effective photospheric temperature of 4,045 K, a radius of 0.6412 R☉, a mass of 0.6 M☉, an estimated bolometric luminosity of 0.099 L☉. Stellar evolution modeling indicates an estimated stellar age of 0.12 Gyr. From Earth, 2MASS J22362452+4751425 shines at apparent V-band magnitude 12.368 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.01 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: W. M. Keck Observatory · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name 2MASS J22362452+4751425
Spectral Type K7 V
Effective Temp (Teff) 4,045 K
Stellar Radius 0.6412 R☉
Stellar Mass 0.6000 M☉
Bolometric Luminosity 0.099 L☉
Metallicity [Fe/H] —
Stellar Age 0.120 Gyr
Apparent Magnitude V: 12.368 · G: 11.948
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 230.000000 AU
Orbital Period —
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 11.77 g/cm³ (201 km/s vesc)
Insolation Flux 0.0000 S⊕
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 226.900 LY (69.574 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 22h36m24.62s · DEC: +47d51m42.06s (J2000: 339.10259°, 47.86168°)
Target Field: 2MASS J22362452+4751425 (J2000 339.10259°, 47.86168°)
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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