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CONFIRMED EXOPLANET · Gas Giant

GSC 06214-00210 b

Orbits Host Star: GSC 06214-00210 (Type K7) · Distance: 353.900 Light-Years (108.500 pc)
Planetary Radius
20.176 R⊕
Planetary Mass
5000.000 M⊕
Surface Gravity
12.28 g / g⊕
Equilibrium Temp
2300K (+2027°C / +3681°F)
Orbital Period
—
Discovery Year
2010 (Imaging)
Earth Similarity (ESI)
0.06 / 1.00
Insolation Flux
0.00 S⊕

Astrophysical Synthesis & Habitability Characterization

GSC 06214-00210 b is a confirmed gas giant exoplanet orbiting the star GSC 06214-00210, located approximately 353.9 light-years (108.5 parsecs) from the Solar System. First announced in 2010 by Palomar Observatory using the Imaging detection technique (resolved directly via high-contrast coronagraphic or interferometric imaging), this world measures 20.176 Earth radii (1.8 Jupiter radii) and has a measured mass of 5000 Earth masses (15.73 Jupiter masses). Combining its mass and radius yields a mean bulk density of 3.36 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 12.28 g⊕ (120.43 m/s²), and an escape velocity of 176.1 km/s.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 2300 K (+2027°C / +3681°F), GSC 06214-00210 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star GSC 06214-00210 is classified as an orange K-type star of spectral type K7 with an effective photospheric temperature of 4,200 K, a radius of 0.9048 R☉, a mass of 0.9 M☉, an estimated bolometric luminosity of 0.229 L☉. Stellar evolution modeling indicates an estimated stellar age of 0.005 Gyr and a metallicity of [Fe/H] = -0.06 dex (near-solar heavy-element abundance). From Earth, GSC 06214-00210 shines at apparent V-band magnitude 12.416 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.06 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: Palomar Observatory · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name GSC 06214-00210
Spectral Type K7
Effective Temp (Teff) 4,200 K
Stellar Radius 0.9048 R☉
Stellar Mass 0.9000 M☉
Bolometric Luminosity 0.229 L☉
Metallicity [Fe/H] -0.060 dex
Stellar Age 0.005 Gyr
Apparent Magnitude V: 12.416 · G: 11.863
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 320.000000 AU
Orbital Period —
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 3.36 g/cm³ (176.1 km/s vesc)
Insolation Flux 0.0000 S⊕
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 353.900 LY (108.500 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 16h21m54.65s · DEC: -20d43m09.62s (J2000: 245.47769°, -20.71934°)
Target Field: GSC 06214-00210 (J2000 245.47769°, -20.71934°)
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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