HD 110067 e
Astrophysical Synthesis & Habitability Characterization
HD 110067 e is a confirmed super-earth exoplanet orbiting the star HD 110067, located approximately 104.9 light-years (32.16 parsecs) from the Solar System. First announced in 2023 by Multiple Observatories using the Transit detection technique (producing an estimated primary transit depth of 0.0509% across the stellar disk), this world measures 1.94 Earth radii and has a measured mass of 3.9 Earth masses. Combining its mass and radius yields a mean bulk density of 2.95 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.04 g⊕ (10.2 m/s²), and an escape velocity of 15.9 km/s.
In its orbital architecture around HD 110067, HD 110067 e completes one full revolution every 30.793 Earth days at a semi-major axis of 0.1785 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 63.1 km/s (compared to Earth's 29.8 km/s).
⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 533 K (+260°C / +500°F) and receiving 13.63 S⊕ (~18,550 W/m²), HD 110067 e orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star HD 110067 is classified as an orange K-type star of spectral type K0.0 V with an effective photospheric temperature of 5,266 K, a radius of 0.788 R☉, a mass of 0.798 M☉, an estimated bolometric luminosity of 0.428 L☉. Stellar evolution modeling indicates an estimated stellar age of 8.1 Gyr and a metallicity of [Fe/H] = -0.2 dex (metal-poor relative to the Sun). From Earth, HD 110067 shines at apparent V-band magnitude 8.419 (accessible to binoculars and small amateur telescopes) in the Northern celestial hemisphere. The HD 110067 system is a multi-planet architecture hosting 6 confirmed worlds, with HD 110067 e sharing its stellar neighborhood alongside HD 110067 b, HD 110067 c, HD 110067 d, HD 110067 f, HD 110067 g.
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: Multiple Observatories · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).
☀️ Host Star Telemetry
| Host Star Name | HD 110067 |
| Spectral Type | K0.0 V |
| Effective Temp (Teff) | 5,266 K |
| Stellar Radius | 0.7880 R☉ |
| Stellar Mass | 0.7980 M☉ |
| Bolometric Luminosity | 0.428 L☉ |
| Metallicity [Fe/H] | -0.200 dex |
| Stellar Age | 8.100 Gyr |
| Apparent Magnitude | V: 8.419 · G: 8.172 |
| System Architecture | 3 Stars, 6 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.178500 AU |
| Orbital Period | 30.793 days |
| Mean Orbital Velocity | 63.1 km/s |
| Orbital Eccentricity (e) | Circular (0.00) |
| Orbital Inclination (i) | 89.8670° |
| Mean Bulk Density | 2.95 g/cm³ (15.9 km/s vesc) |
| Insolation Flux | 13.6296 S⊕ (~18,550 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 104.900 LY (32.159 pc) |