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CONFIRMED EXOPLANET · Gas Giant

G 196-3 b

Orbits Host Star: G 196-3 · Distance: 71.100 Light-Years (21.791 pc)
Planetary Radius
12.000 R⊕
Planetary Mass
8263.539 M⊕
Surface Gravity
57.39 g / g⊕
Equilibrium Temp
1670K (+1397°C / +2547°F)
Orbital Period
—
Discovery Year
2024 (Imaging)
Earth Similarity (ESI)
0.07 / 1.00
Insolation Flux
0.00 S⊕

Astrophysical Synthesis & Habitability Characterization

G 196-3 b is a confirmed gas giant exoplanet orbiting the star G 196-3, located approximately 71.1 light-years (21.79 parsecs) from the Solar System. First announced in 2024 by European Space Agency (ESA) Gaia Satellite using the Imaging detection technique (resolved directly via high-contrast coronagraphic or interferometric imaging), this world measures 12 Earth radii (1.07 Jupiter radii) and has a measured mass of 8263.539 Earth masses (26 Jupiter masses). Combining its mass and radius yields a mean bulk density of 26.37 g/cm³ (an iron-enriched, high-compression rocky core), a surface gravity of 57.39 g⊕ (562.8 m/s²), and an escape velocity of 293.5 km/s.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1670 K (+1397°C / +2547°F), G 196-3 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star G 196-3 is classified as a stellar host with an effective photospheric temperature of 3,517 K, a radius of 0.5224 R☉, a mass of 0.5198 M☉, an estimated bolometric luminosity of 0.037 L☉. From Earth, G 196-3 shines at apparent V-band magnitude 11.672 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.07 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: European Space Agency (ESA) Gaia Satellite · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name G 196-3
Spectral Type Unclassified
Effective Temp (Teff) 3,517 K
Stellar Radius 0.5224 R☉
Stellar Mass 0.5198 M☉
Bolometric Luminosity 0.037 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 11.672 · G: 10.612
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 350.000000 AU
Orbital Period —
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 26.37 g/cm³ (293.5 km/s vesc)
Insolation Flux 0.0000 S⊕
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 71.100 LY (21.791 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 10h04m21.23s · DEC: +50d23m10.25s (J2000: 151.08848°, 50.38618°)
Target Field: G 196-3 (J2000 151.08848°, 50.38618°)
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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