STATION 02: EXOPLANETLEDGER.ORG · WORLD DOSSIER // HD 160691 c
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CONFIRMED EXOPLANET · Gas Giant

HD 160691 c

Orbits Host Star: HD 160691 (Type G3 IV-V) · Distance: 50.900 Light-Years (15.598 pc)
Planetary Radius
—
Planetary Mass
1398.445 M⊕
Surface Gravity
—
Equilibrium Temp
157K (-116°C / -177°F)
Orbital Period
3947 days
Discovery Year
2004 (Radial Velocity)
Insolation Flux
0.11 S⊕

Astrophysical Synthesis & Habitability Characterization

HD 160691 c is a confirmed gas giant exoplanet orbiting the star HD 160691, located approximately 50.9 light-years (15.6 parsecs) from the Solar System. First announced in 2004 by Anglo-Australian Telescope using the Radial Velocity detection technique (measuring periodic Doppler reflex motion in the host star's spectrum), this world has a minimum or true mass of 1398.445 Earth masses (4.4 M♃), while its physical transit radius has not yet been geometrically observed.

In its orbital architecture around HD 160691, HD 160691 c completes one full revolution every 3947 Earth days (10.81Julian years) at a semi-major axis of 4.17 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 11.5 km/s (compared to Earth's 29.8 km/s). With a near-circular eccentricity of e = 0.039 (ranging from 4.0074 AU at periapsis to 4.3326 AU at apoapsis), the planet experiences minimal orbital distance variation.

❄️ Thermal Regime (Cryogenic Zone): With an equilibrium temperature of 157 K (-116°C / -177°F) and an incident flux of 0.11 S⊕ (~149 W/m²), surface water and volatile species on HD 160691 c would remain locked in cryogenic ice phases unless warmed by subsurface tidal or radiogenic heating.

The host star HD 160691 is classified as a solar-type yellow star of spectral type G3 IV-V with an effective photospheric temperature of 5,773 K, a radius of 1.33 R☉, a mass of 1.13 M☉, an estimated bolometric luminosity of 1.763 L☉. Stellar evolution modeling indicates an estimated stellar age of 5.7 Gyr and a metallicity of [Fe/H] = 0.28 dex (metal-rich relative to the Sun). From Earth, HD 160691 shines at apparent V-band magnitude 5.12 (visible to the unaided human eye under dark skies) in the Southern celestial hemisphere. The HD 160691 system is a multi-planet architecture hosting 4 confirmed worlds, with HD 160691 c sharing its stellar neighborhood alongside HD 160691 d, HD 160691 e, HD 160691 b.

Discovery Facility: Anglo-Australian Telescope · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name HD 160691
Spectral Type G3 IV-V
Effective Temp (Teff) 5,773 K
Stellar Radius 1.3300 R☉
Stellar Mass 1.1300 M☉
Bolometric Luminosity 1.763 L☉
Metallicity [Fe/H] 0.280 dex
Stellar Age 5.700 Gyr
Apparent Magnitude V: 5.120 · G: 4.949
System Architecture 1 Star, 4 Planets

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 4.170000 AU
Orbital Period 3947 days
Mean Orbital Velocity 11.5 km/s
Orbital Eccentricity (e) 0.03900
Orbital Inclination (i) 60.0000°
Insolation Flux 0.1092 S⊕ (~149 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 50.900 LY (15.598 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 17h44m08.68s · DEC: -51d50m05.55s (J2000: 266.03616°, -51.83488°)
Target Field: HD 160691 (J2000 266.03616°, -51.83488°)
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 ↗

Other Worlds in the HD 160691 System (3)

NASA EXOPLANET ARCHIVE COMPOSITE PARAMETERS
Inspect Raw NASA Archive Record ↗