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CONFIRMED EXOPLANET · Gas Giant

HD 106906 b

Orbits Host Star: HD 106906 (Type F5 V) · Distance: 336.000 Light-Years (103.029 pc)
Planetary Radius
12.400 R⊕
Planetary Mass
3496.000 M⊕
Surface Gravity
22.74 g / g⊕
Equilibrium Temp
1800K (+1527°C / +2781°F)
Orbital Period
—
Discovery Year
2013 (Imaging)
Earth Similarity (ESI)
0.08 / 1.00
Insolation Flux
0.00 S⊕

Astrophysical Synthesis & Habitability Characterization

HD 106906 b is a confirmed gas giant exoplanet orbiting the star HD 106906, located approximately 336 light-years (103.03 parsecs) from the Solar System. First announced in 2013 by Las Campanas Observatory using the Imaging detection technique (resolved directly via high-contrast coronagraphic or interferometric imaging), this world measures 12.4 Earth radii (1.11 Jupiter radii) and has a measured mass of 3496 Earth masses (11 Jupiter masses). Combining its mass and radius yields a mean bulk density of 10.11 g/cm³ (an iron-enriched, high-compression rocky core), a surface gravity of 22.74 g⊕ (223 m/s²), and an escape velocity of 187.8 km/s.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1800 K (+1527°C / +2781°F), HD 106906 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star HD 106906 is classified as a warm F-type star of spectral type F5 V with an effective photospheric temperature of 6,516 K, a radius of 2.1235 R☉, a mass of 1.5 M☉, an estimated bolometric luminosity of 7.293 L☉. Stellar evolution modeling indicates an estimated stellar age of 0.013 Gyr and a metallicity of [Fe/H] = 0.04 dex (near-solar heavy-element abundance). From Earth, HD 106906 shines at apparent V-band magnitude 7.8 (accessible to binoculars and small amateur telescopes) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.08 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: Las Campanas Observatory · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name HD 106906
Spectral Type F5 V
Effective Temp (Teff) 6,516 K
Stellar Radius 2.1235 R☉
Stellar Mass 1.5000 M☉
Bolometric Luminosity 7.293 L☉
Metallicity [Fe/H] 0.040 dex
Stellar Age 0.013 Gyr
Apparent Magnitude V: 7.800 · G: 7.686
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 650.000000 AU
Orbital Period —
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 10.11 g/cm³ (187.8 km/s vesc)
Insolation Flux 0.0000 S⊕
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 336.000 LY (103.029 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 12h17m53.12s · DEC: -55d58m32.09s (J2000: 184.47133°, -55.97558°)
Target Field: HD 106906 (J2000 184.47133°, -55.97558°)
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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