K2-171 b
Astrophysical Synthesis & Habitability Characterization
K2-171 b is a confirmed sub-neptune exoplanet orbiting the star K2-171, located approximately 1976.9 light-years (606.13 parsecs) from the Solar System. First announced in 2018 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.0206% across the stellar disk), this world measures 2.687 Earth radii and has a measured mass of 7.69 Earth masses. Combining its mass and radius yields a mean bulk density of 2.19 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.07 g⊕ (10.49 m/s²), and an escape velocity of 18.9 km/s.
In its orbital architecture around K2-171, K2-171 b completes one full revolution every 5.628 Earth days.
☁️ Atmospheric Regime (Volatile / Gas Envelope): With a radius of 2.687 R⊕, K2-171 b 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 K2-171 is classified as a stellar host with an effective photospheric temperature of 5,250 K, a radius of 1.7175 R☉, a mass of 0.8916 M☉, an estimated bolometric luminosity of 2.011 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.09 dex (near-solar heavy-element abundance). From Earth, K2-171 shines at apparent V-band magnitude 12.745 (faint and requiring research-grade or CCD telescopic photometry) 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: K2 · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).
☀️ Host Star Telemetry
| Host Star Name | K2-171 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,250 K |
| Stellar Radius | 1.7175 R☉ |
| Stellar Mass | 0.8916 M☉ |
| Bolometric Luminosity | 2.011 L☉ |
| Metallicity [Fe/H] | -0.090 dex |
| Stellar Age | — |
| Apparent Magnitude | V: 12.745 · G: 12.439 |
| System Architecture | 1 Star, 1 Planet |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | — |
| Orbital Period | 5.628 days |
| Orbital Eccentricity (e) | Circular (0.00) |
| Orbital Inclination (i) | 85.0482° |
| Mean Bulk Density | 2.19 g/cm³ (18.9 km/s vesc) |
| Insolation Flux | — |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 1976.900 LY (606.128 pc) |