STATION 02: EXOPLANETLEDGER.ORG · WORLD DOSSIER // ROXs 12 b
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CONFIRMED EXOPLANET · Gas Giant

ROXs 12 b

Orbits Host Star: ROXs 12 (Type M0) · Distance: 445.700 Light-Years (136.650 pc)
Planetary Radius
12.200 R⊕
Planetary Mass
5085.000 M⊕
Surface Gravity
34.16 g / g⊕
Equilibrium Temp
13K (-260°C / -436°F)
Orbital Period
—
Discovery Year
2013 (Imaging)
Earth Similarity (ESI)
0.01 / 1.00
Insolation Flux
0.00 S⊕

Astrophysical Synthesis & Habitability Characterization

ROXs 12 b is a confirmed gas giant exoplanet orbiting the star ROXs 12, located approximately 445.7 light-years (136.65 parsecs) from the Solar System. First announced in 2013 by W. M. Keck Observatory using the Imaging detection technique (resolved directly via high-contrast coronagraphic or interferometric imaging), this world measures 12.2 Earth radii (1.09 Jupiter radii) and has a measured mass of 5085 Earth masses (16 Jupiter masses). Combining its mass and radius yields a mean bulk density of 15.44 g/cm³ (an iron-enriched, high-compression rocky core), a surface gravity of 34.16 g⊕ (335 m/s²), and an escape velocity of 228.4 km/s.

The planet follows a highly eccentric trajectory (e = 0.83, swinging from 35.7 AU at periapsis out to 384.3 AU at apoapsis), pointing to past dynamical scattering or secular gravitational perturbations.

❄️ Thermal Regime (Cryogenic Zone): With an equilibrium temperature of 13 K (-260°C / -436°F), surface water and volatile species on ROXs 12 b would remain locked in cryogenic ice phases unless warmed by subsurface tidal or radiogenic heating.

The host star ROXs 12 is classified as a low-mass red dwarf of spectral type M0 with an effective photospheric temperature of 3,850 K, a radius of 1.0663 R☉, a mass of 0.87 M☉, an estimated bolometric luminosity of 0.224 L☉. Stellar evolution modeling indicates an estimated stellar age of 0.008 Gyr and a metallicity of [Fe/H] = 0.14 dex (metal-rich relative to the Sun). From Earth, ROXs 12 shines at apparent V-band magnitude 14.763 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.01 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: W. M. Keck Observatory · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name ROXs 12
Spectral Type M0
Effective Temp (Teff) 3,850 K
Stellar Radius 1.0663 R☉
Stellar Mass 0.8700 M☉
Bolometric Luminosity 0.224 L☉
Metallicity [Fe/H] 0.140 dex
Stellar Age 0.008 Gyr
Apparent Magnitude V: 14.763 · G: 13.266
System Architecture 2 Stars, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 210.000000 AU
Orbital Period —
Orbital Eccentricity (e) 0.83000
Orbital Inclination (i) —
Mean Bulk Density 15.44 g/cm³ (228.4 km/s vesc)
Insolation Flux 0.0000 S⊕
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 445.700 LY (136.650 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 16h26m28.03s · DEC: -25d26m48.10s (J2000: 246.6168°, -25.4467°)
Target Field: ROXs 12 (J2000 246.6168°, -25.4467°)
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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