STATION 02: EXOPLANETLEDGER.ORG · WORLD DOSSIER // HD 100546 b
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CONFIRMED EXOPLANET · Gas Giant

HD 100546 b

Orbits Host Star: HD 100546 (Type B9 Vne) · Distance: 357.700 Light-Years (109.677 pc)
Planetary Radius
77.342 R⊕
Planetary Mass
2701.541 M⊕
Surface Gravity
0.45 g / g⊕
Equilibrium Temp
95K (-178°C / -288°F)
Orbital Period
—
Discovery Year
2014 (Imaging)
Earth Similarity (ESI)
0.05 / 1.00
Insolation Flux
0.01 S⊕

Astrophysical Synthesis & Habitability Characterization

HD 100546 b is a confirmed gas giant exoplanet orbiting the star HD 100546, located approximately 357.7 light-years (109.68 parsecs) from the Solar System. First announced in 2014 by Paranal Observatory using the Imaging detection technique (resolved directly via high-contrast coronagraphic or interferometric imaging), this world measures 77.342 Earth radii (6.9 Jupiter radii) and has a measured mass of 2701.541 Earth masses (8.5 Jupiter masses). Combining its mass and radius yields a mean bulk density of 0.03 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.45 g⊕ (4.41 m/s²), and an escape velocity of 66.1 km/s.

❄️ Thermal Regime (Cryogenic Zone): With an equilibrium temperature of 95 K (-178°C / -288°F) and an incident flux of 0.01 S⊕ (~15 W/m²), surface water and volatile species on HD 100546 b would remain locked in cryogenic ice phases unless warmed by subsurface tidal or radiogenic heating.

The host star HD 100546 is classified as a massive B-type star of spectral type B9 Vne with an effective photospheric temperature of 10,500 K, a radius of 1.8529 R☉, a mass of 2.4 M☉, an estimated bolometric luminosity of 37.441 L☉. Stellar evolution modeling indicates an estimated stellar age of 0.006 Gyr. From Earth, HD 100546 shines at apparent V-band magnitude 6.69 (accessible to binoculars and small amateur telescopes) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.05 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: Paranal Observatory · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name HD 100546
Spectral Type B9 Vne
Effective Temp (Teff) 10,500 K
Stellar Radius 1.8529 R☉
Stellar Mass 2.4000 M☉
Bolometric Luminosity 37.441 L☉
Metallicity [Fe/H] —
Stellar Age 0.006 Gyr
Apparent Magnitude V: 6.690 · G: 6.655
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 53.000000 AU
Orbital Period —
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 0.03 g/cm³ (66.1 km/s vesc)
Insolation Flux 0.0113 S⊕ (~15 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 357.700 LY (109.677 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 11h33m25.32s · DEC: -70d11m41.24s (J2000: 173.35551°, -70.19479°)
Target Field: HD 100546 (J2000 173.35551°, -70.19479°)
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)
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NASA EXOPLANET ARCHIVE COMPOSITE PARAMETERS
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