STATION 02: EXOPLANETLEDGER.ORG · WORLD DOSSIER // 2M0437 b
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CONFIRMED EXOPLANET · Gas Giant

2M0437 b

Orbits Host Star: 2MASS J04372171+2651014 (Type M V) · Distance: 419.100 Light-Years (128.484 pc)
Planetary Radius
13.000 R⊕
Planetary Mass
1271.314 M⊕
Surface Gravity
7.52 g / g⊕
Equilibrium Temp
1450K (+1177°C / +2151°F)
Orbital Period
—
Discovery Year
2021 (Imaging)
Earth Similarity (ESI)
0.11 / 1.00
Insolation Flux
0.00 S⊕

Astrophysical Synthesis & Habitability Characterization

2M0437 b is a confirmed gas giant exoplanet orbiting the star 2MASS J04372171+2651014, located approximately 419.1 light-years (128.48 parsecs) from the Solar System. First announced in 2021 by Subaru Telescope using the Imaging detection technique (resolved directly via high-contrast coronagraphic or interferometric imaging), this world measures 13 Earth radii (1.16 Jupiter radii) and has a measured mass of 1271.314 Earth masses (4 Jupiter masses). Combining its mass and radius yields a mean bulk density of 3.19 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 7.52 g⊕ (73.75 m/s²), and an escape velocity of 110.6 km/s.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1450 K (+1177°C / +2151°F), 2M0437 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star 2MASS J04372171+2651014 is classified as a low-mass red dwarf of spectral type M V with an effective photospheric temperature of 3,100 K, a radius of 0.84 R☉, a mass of 0.17 M☉, an estimated bolometric luminosity of 0.058 L☉. Stellar evolution modeling indicates an estimated stellar age of 0.003 Gyr and a metallicity of [Fe/H] = 0.01 dex (near-solar heavy-element abundance). From Earth, 2MASS J04372171+2651014 shines at apparent V-band magnitude 16.186 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.11 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: Subaru Telescope · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name 2MASS J04372171+2651014
Spectral Type M V
Effective Temp (Teff) 3,100 K
Stellar Radius 0.8400 R☉
Stellar Mass 0.1700 M☉
Bolometric Luminosity 0.058 L☉
Metallicity [Fe/H] 0.010 dex
Stellar Age 0.003 Gyr
Apparent Magnitude V: 16.186 · G: 14.337
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 118.000000 AU
Orbital Period —
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 3.19 g/cm³ (110.6 km/s vesc)
Insolation Flux 0.0000 S⊕
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 419.100 LY (128.484 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 04h37m21.73s · DEC: +26d51m01.08s (J2000: 69.34055°, 26.8503°)
Target Field: 2MASS J04372171+2651014 (J2000 69.34055°, 26.8503°)
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
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