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CONFIRMED EXOPLANET · Gas Giant

CoRoT-16 b

Orbits Host Star: CoRoT-16 (Type G5 V) · Distance: 2388.800 Light-Years (732.409 pc)
Planetary Radius
13.110 R⊕
Planetary Mass
170.032 M⊕
Surface Gravity
0.99 g / g⊕
Equilibrium Temp
1196K (+923°C / +1693°F)
Orbital Period
5.352 days
Discovery Year
2011 (Transit)
Earth Similarity (ESI)
0.10 / 1.00
Insolation Flux
96.18 S⊕

Astrophysical Synthesis & Habitability Characterization

CoRoT-16 b is a confirmed gas giant exoplanet orbiting the star CoRoT-16, located approximately 2388.8 light-years (732.41 parsecs) from the Solar System. First announced in 2011 by CoRoT using the Transit detection technique (producing an estimated primary transit depth of 1.0201% across the stellar disk), this world measures 13.11 Earth radii (1.17 Jupiter radii) and has a measured mass of 170.032 Earth masses (0.53 Jupiter masses). Combining its mass and radius yields a mean bulk density of 0.42 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.99 g⊕ (9.71 m/s²), and an escape velocity of 40.3 km/s.

In its orbital architecture around CoRoT-16, CoRoT-16 b completes one full revolution every 5.352 Earth days at a semi-major axis of 0.0618 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 125.6 km/s (compared to Earth's 29.8 km/s). The planet follows a highly eccentric trajectory (e = 0.33, swinging from 0.0414 AU at periapsis out to 0.0822 AU at apoapsis), pointing to past dynamical scattering or secular gravitational perturbations.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1196 K (+923°C / +1693°F) and receiving 96.18 S⊕ (~130,895 W/m²), CoRoT-16 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star CoRoT-16 is classified as a solar-type yellow star of spectral type G5 V with an effective photospheric temperature of 5,650 K, a radius of 1.19 R☉, a mass of 1.098 M☉, an estimated bolometric luminosity of 1.295 L☉. Stellar evolution modeling indicates an estimated stellar age of 6.73 Gyr and a metallicity of [Fe/H] = 0.19 dex (metal-rich relative to the Sun). From Earth, CoRoT-16 shines at apparent V-band magnitude 16.052 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.10 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: CoRoT · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name CoRoT-16
Spectral Type G5 V
Effective Temp (Teff) 5,650 K
Stellar Radius 1.1900 R☉
Stellar Mass 1.0980 M☉
Bolometric Luminosity 1.295 L☉
Metallicity [Fe/H] 0.190 dex
Stellar Age 6.730 Gyr
Apparent Magnitude V: 16.052 · G: 15.651
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.061800 AU
Orbital Period 5.352 days
Mean Orbital Velocity 125.6 km/s
Orbital Eccentricity (e) 0.33000
Orbital Inclination (i) 85.0100°
Mean Bulk Density 0.42 g/cm³ (40.3 km/s vesc)
Insolation Flux 96.1756 S⊕ (~130,895 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 2388.800 LY (732.409 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 18h34m05.92s · DEC: -06d00m09.37s (J2000: 278.52467°, -6.0026°)
Target Field: CoRoT-16 (J2000 278.52467°, -6.0026°)
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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