HD 101930 b
Astrophysical Synthesis & Habitability Characterization
HD 101930 b is a confirmed gas giant exoplanet orbiting the star HD 101930, located approximately 97.9 light-years (30.03 parsecs) from the Solar System. First announced in 2005 by La Silla Observatory using the Radial Velocity detection technique (measuring periodic Doppler reflex motion in the host star's spectrum), this world measures 10.6 Earth radii (0.95 Jupiter radii) and has a measured mass of 79.458 Earth masses (0.25 Jupiter masses). Combining its mass and radius yields a mean bulk density of 0.37 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.71 g⊕ (6.96 m/s²), and an escape velocity of 30.6 km/s.
In its orbital architecture around HD 101930, HD 101930 b completes one full revolution every 70.46 Earth days at a semi-major axis of 0.3 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 46.3 km/s (compared to Earth's 29.8 km/s). Its moderate orbital eccentricity of e = 0.11 carries the world between 0.267 AU at periapsis and 0.333 AU at apoapsis, driving measurable seasonal insolation cycles.
⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 417 K (+144°C / +291°F) and receiving 5.44 S⊕ (~7,410 W/m²), HD 101930 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star HD 101930 is classified as an orange K-type star of spectral type K1 V with an effective photospheric temperature of 5,108 K, a radius of 0.86 R☉, a mass of 0.57 M☉, an estimated bolometric luminosity of 0.452 L☉. Stellar evolution modeling indicates an estimated stellar age of 1 Gyr and a metallicity of [Fe/H] = 0.15 dex (metal-rich relative to the Sun). From Earth, HD 101930 shines at apparent V-band magnitude 8.21 (accessible to binoculars and small amateur telescopes) in the Southern celestial hemisphere.
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: La Silla Observatory · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).
☀️ Host Star Telemetry
| Host Star Name | HD 101930 |
| Spectral Type | K1 V |
| Effective Temp (Teff) | 5,108 K |
| Stellar Radius | 0.8600 R☉ |
| Stellar Mass | 0.5700 M☉ |
| Bolometric Luminosity | 0.452 L☉ |
| Metallicity [Fe/H] | 0.150 dex |
| Stellar Age | 1.000 Gyr |
| Apparent Magnitude | V: 8.210 · G: 7.967 |
| System Architecture | 2 Stars, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.300000 AU |
| Orbital Period | 70.46 days |
| Mean Orbital Velocity | 46.3 km/s |
| Orbital Eccentricity (e) | 0.11000 |
| Orbital Inclination (i) | — |
| Mean Bulk Density | 0.37 g/cm³ (30.6 km/s vesc) |
| Insolation Flux | 5.4444 S⊕ (~7,410 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 97.900 LY (30.027 pc) |