STATION 02: EXOPLANETLEDGER.ORG · WORLD DOSSIER // HD 203030 b
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CONFIRMED EXOPLANET · Gas Giant

HD 203030 b

Orbits Host Star: HD 203030 (Type G8 V) · Distance: 128.000 Light-Years (39.250 pc)
Planetary Radius
14.460 R⊕
Planetary Mass
3496.112 M⊕
Surface Gravity
16.72 g / g⊕
Equilibrium Temp
1040K (+767°C / +1413°F)
Orbital Period
—
Discovery Year
2006 (Imaging)
Earth Similarity (ESI)
0.16 / 1.00
Insolation Flux
0.00 S⊕

Astrophysical Synthesis & Habitability Characterization

HD 203030 b is a confirmed gas giant exoplanet orbiting the star HD 203030, located approximately 128 light-years (39.25 parsecs) from the Solar System. First announced in 2006 by Palomar Observatory using the Imaging detection technique (resolved directly via high-contrast coronagraphic or interferometric imaging), this world measures 14.46 Earth radii (1.29 Jupiter radii) and has a measured mass of 3496.112 Earth masses (11 Jupiter masses). Combining its mass and radius yields a mean bulk density of 6.38 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 16.72 g⊕ (163.97 m/s²), and an escape velocity of 173.9 km/s.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1040 K (+767°C / +1413°F), HD 203030 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star HD 203030 is classified as a solar-type yellow star of spectral type G8 V with an effective photospheric temperature of 5,603 K, a radius of 0.8565 R☉, a mass of 0.94 M☉, an estimated bolometric luminosity of 0.649 L☉. Stellar evolution modeling indicates an estimated stellar age of 0.1 Gyr and a metallicity of [Fe/H] = 0.3 dex (metal-rich relative to the Sun). From Earth, HD 203030 shines at apparent V-band magnitude 8.45 (accessible to binoculars and small amateur telescopes) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.16 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 HD 203030
Spectral Type G8 V
Effective Temp (Teff) 5,603 K
Stellar Radius 0.8565 R☉
Stellar Mass 0.9400 M☉
Bolometric Luminosity 0.649 L☉
Metallicity [Fe/H] 0.300 dex
Stellar Age 0.100 Gyr
Apparent Magnitude V: 8.450 · G: 8.247
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 487.100000 AU
Orbital Period —
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 6.38 g/cm³ (173.9 km/s vesc)
Insolation Flux 0.0000 S⊕
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 128.000 LY (39.250 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 21h18m58.37s · DEC: +26d13m50.10s (J2000: 319.74322°, 26.23058°)
Target Field: HD 203030 (J2000 319.74322°, 26.23058°)
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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