K2-285 c
Astrophysical Synthesis & Habitability Characterization
K2-285 c is a confirmed sub-neptune exoplanet orbiting the star K2-285, located approximately 505.4 light-years (154.96 parsecs) from the Solar System. First announced in 2018 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.1691% across the stellar disk), this world measures 3.53 Earth radii (0.31 Jupiter radii) and has a measured mass of 15.68 Earth masses. Combining its mass and radius yields a mean bulk density of 1.97 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 1.26 g⊕ (12.36 m/s²), and an escape velocity of 23.6 km/s.
In its orbital architecture around K2-285, K2-285 c completes one full revolution every 7.138 Earth days at a semi-major axis of 0.0824 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 125.6 km/s (compared to Earth's 29.8 km/s). The orbit is modeled as circular (e = 0.00), maintaining a constant stellar distance throughout its year.
⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 741 K (+468°C / +874°F) and receiving 50.35 S⊕ (~68,526 W/m²), K2-285 c orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star K2-285 is classified as an orange K-type star of spectral type K2 V with an effective photospheric temperature of 4,975 K, a radius of 0.787 R☉, a mass of 0.83 M☉, an estimated bolometric luminosity of 0.34 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = 0 dex (near-solar heavy-element abundance). From Earth, K2-285 shines at apparent V-band magnitude 12.075 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The K2-285 system is a multi-planet architecture hosting 4 confirmed worlds, with K2-285 c sharing its stellar neighborhood alongside K2-285 b, K2-285 d, K2-285 e.
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 | K2-285 |
| Spectral Type | K2 V |
| Effective Temp (Teff) | 4,975 K |
| Stellar Radius | 0.7870 R☉ |
| Stellar Mass | 0.8300 M☉ |
| Bolometric Luminosity | 0.34 L☉ |
| Metallicity [Fe/H] | 0.000 dex |
| Stellar Age | — |
| Apparent Magnitude | V: 12.075 · G: 11.804 |
| System Architecture | 1 Star, 4 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.082400 AU |
| Orbital Period | 7.138 days |
| Mean Orbital Velocity | 125.6 km/s |
| Orbital Eccentricity (e) | 0.00000 |
| Orbital Inclination (i) | 89.8610° |
| Mean Bulk Density | 1.97 g/cm³ (23.6 km/s vesc) |
| Insolation Flux | 50.3500 S⊕ (~68,526 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 505.400 LY (154.961 pc) |