STATION 02: EXOPLANETLEDGER.ORG · WORLD DOSSIER // Luhman 16 b
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CONFIRMED EXOPLANET · Gas Giant

Luhman 16 b

Orbits Host Star: Luhman 16 A
Planetary Radius
11.900 R⊕
Planetary Mass
9344.155 M⊕
Surface Gravity
65.99 g / g⊕
Equilibrium Temp
—
Orbital Period
9697 days
Discovery Year
2017 (Imaging)
Earth Similarity (ESI)
0.25 / 1.00
Insolation Flux
0.00 S⊕

Astrophysical Synthesis & Habitability Characterization

Luhman 16 b is a confirmed gas giant exoplanet orbiting the star Luhman 16 A. First announced in 2017 by Multiple Observatories using the Imaging detection technique (resolved directly via high-contrast coronagraphic or interferometric imaging), this world measures 11.9 Earth radii (1.06 Jupiter radii) and has a measured mass of 9344.155 Earth masses (29.4 Jupiter masses). Combining its mass and radius yields a mean bulk density of 30.57 g/cm³ (an iron-enriched, high-compression rocky core), a surface gravity of 65.99 g⊕ (647.14 m/s²), and an escape velocity of 313.5 km/s.

In its orbital architecture around Luhman 16 A, Luhman 16 b completes one full revolution every 9697 Earth days (26.55Julian years) at a semi-major axis of 3.52 AU (corresponding to the middle-system regime between Mars at 1.52 AU and Jupiter at 5.20 AU). Its mean orbital velocity is approximately 3.9 km/s (compared to Earth's 29.8 km/s). The planet follows a highly eccentric trajectory (e = 0.344, swinging from 2.3091 AU at periapsis out to 4.7309 AU at apoapsis), pointing to past dynamical scattering or secular gravitational perturbations.

☁️ Atmospheric Regime (Volatile / Gas Envelope): With a radius of 11.900 R⊕, Luhman 16 b exceeds the empirical ~1.8–2.2 R⊕ Fulton radius valley threshold, indicating a substantial hydrogen-helium or supercritical volatile envelope without a conventional solid terrestrial surface.

The host star Luhman 16 A is classified as a stellar host with a mass of 0.0338 M☉.

Earth Similarity Index (ESI): 0.25 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: Multiple Observatories · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name Luhman 16 A
Spectral Type Unclassified
Effective Temp (Teff) —
Stellar Radius —
Stellar Mass 0.0338 M☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude —
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 3.520000 AU
Orbital Period 9697 days
Mean Orbital Velocity 3.9 km/s
Orbital Eccentricity (e) 0.34400
Orbital Inclination (i) 79.9200°
Mean Bulk Density 30.57 g/cm³ (313.5 km/s vesc)
Insolation Flux 0.0000 S⊕
Habitable Zone Status Exterior / Non-HZ
Celestial Distance —

🔭 Deep Space Viewport // Host Star Field

RA: 10h49m18.78s · DEC: -53d19m09.74s (J2000: 162.32826°, -53.31937°)
Target Field: Luhman 16 A (J2000 162.32826°, -53.31937°)
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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