HD 207832 c
Astrophysical Synthesis & Habitability Characterization
HD 207832 c is a confirmed gas giant exoplanet orbiting the star HD 207832, located approximately 192.2 light-years (58.93 parsecs) from the Solar System. First announced in 2012 by W. M. Keck Observatory using the Radial Velocity detection technique (measuring periodic Doppler reflex motion in the host star's spectrum), this world measures 14 Earth radii (1.25 Jupiter radii) and has a measured mass of 232.016 Earth masses (0.73 Jupiter masses). Combining its mass and radius yields a mean bulk density of 0.47 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 1.18 g⊕ (11.57 m/s²), and an escape velocity of 45.5 km/s.
In its orbital architecture around HD 207832, HD 207832 c completes one full revolution every 1155.7 Earth days (3.16Julian years) at a semi-major axis of 2.112 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 19.9 km/s (compared to Earth's 29.8 km/s). The planet follows a highly eccentric trajectory (e = 0.27, swinging from 1.5418 AU at periapsis out to 2.6822 AU at apoapsis), pointing to past dynamical scattering or secular gravitational perturbations.
☁️ Atmospheric Regime (Volatile / Gas Envelope): With a radius of 14.000 R⊕, HD 207832 c 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 HD 207832 is classified as a solar-type yellow star of spectral type G5 V with an effective photospheric temperature of 5,710 K, a radius of 0.901 R☉, a mass of 0.94 M☉, an estimated bolometric luminosity of 0.774 L☉. Stellar evolution modeling indicates an estimated stellar age of 1.36 Gyr and a metallicity of [Fe/H] = 0.06 dex (metal-rich relative to the Sun). From Earth, HD 207832 shines at apparent V-band magnitude 8.78 (accessible to binoculars and small amateur telescopes) in the Southern celestial hemisphere. The HD 207832 system is a multi-planet architecture hosting 2 confirmed worlds, with HD 207832 c sharing its stellar neighborhood alongside HD 207832 b.
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 | HD 207832 |
| Spectral Type | G5 V |
| Effective Temp (Teff) | 5,710 K |
| Stellar Radius | 0.9010 R☉ |
| Stellar Mass | 0.9400 M☉ |
| Bolometric Luminosity | 0.774 L☉ |
| Metallicity [Fe/H] | 0.060 dex |
| Stellar Age | 1.360 Gyr |
| Apparent Magnitude | V: 8.780 · G: 8.612 |
| System Architecture | 3 Stars, 2 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 2.112000 AU |
| Orbital Period | 1155.7 days |
| Mean Orbital Velocity | 19.9 km/s |
| Orbital Eccentricity (e) | 0.27000 |
| Orbital Inclination (i) | — |
| Mean Bulk Density | 0.47 g/cm³ (45.5 km/s vesc) |
| Insolation Flux | 0.1732 S⊕ (~236 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 192.200 LY (58.929 pc) |