STATION 02: EXOPLANETLEDGER.ORG · WORLD DOSSIER // HIP 81208 C b
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CONFIRMED EXOPLANET · Gas Giant

HIP 81208 C b

Orbits Host Star: HIP 81208 C (Type M) · Distance: 481.200 Light-Years (147.533 pc)
Planetary Radius
12.300 R⊕
Planetary Mass
4703.860 M⊕
Surface Gravity
31.09 g / g⊕
Equilibrium Temp
2050K (+1777°C / +3231°F)
Orbital Period
104100 days
Discovery Year
2023 (Imaging)
Earth Similarity (ESI)
0.06 / 1.00

Astrophysical Synthesis & Habitability Characterization

HIP 81208 C b is a confirmed gas giant exoplanet orbiting the star HIP 81208 C, located approximately 481.2 light-years (147.53 parsecs) from the Solar System. First announced in 2023 by Paranal Observatory using the Imaging detection technique (resolved directly via high-contrast coronagraphic or interferometric imaging), this world measures 12.3 Earth radii (1.1 Jupiter radii) and has a measured mass of 4703.86 Earth masses (14.8 Jupiter masses). Combining its mass and radius yields a mean bulk density of 13.94 g/cm³ (an iron-enriched, high-compression rocky core), a surface gravity of 31.09 g⊕ (304.89 m/s²), and an escape velocity of 218.8 km/s.

In its orbital architecture around HIP 81208 C, HIP 81208 C b completes one full revolution every 104100 Earth days (285.01Julian years) at a semi-major axis of 23.04 AU (a wide outer-system orbit beyond Jupiter's 5.20 AU distance in our Solar System). Its mean orbital velocity is approximately 2.4 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 2050 K (+1777°C / +3231°F), HIP 81208 C b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star HIP 81208 C is classified as a low-mass red dwarf of spectral type M with a mass of 0.135 M☉. Stellar evolution modeling indicates an estimated stellar age of 0.017 Gyr.

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: Paranal Observatory · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name HIP 81208 C
Spectral Type M
Effective Temp (Teff) —
Stellar Radius —
Stellar Mass 0.1350 M☉
Metallicity [Fe/H] —
Stellar Age 0.017 Gyr
Apparent Magnitude —
System Architecture 3 Stars, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 23.040000 AU
Orbital Period 104100 days
Mean Orbital Velocity 2.4 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 13.94 g/cm³ (218.8 km/s vesc)
Insolation Flux —
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 481.200 LY (147.533 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 16h35m13.8s · DEC: -35d43m29.13s (J2000: 248.8075°, -35.72476°)
Target Field: HIP 81208 C (J2000 248.8075°, -35.72476°)
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)
SIMBAD Astronomical Query ↗ NASA ADS Research Papers ↗
NASA EXOPLANET ARCHIVE COMPOSITE PARAMETERS
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