K2-80 c
Astrophysical Synthesis & Habitability Characterization
K2-80 c is a confirmed super-earth exoplanet orbiting the star K2-80, located approximately 654.9 light-years (200.8 parsecs) from the Solar System. First announced in 2016 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.024% across the stellar disk), this world measures 1.47 Earth radii and has a measured mass of 2.76 Earth masses. Combining its mass and radius yields a mean bulk density of 4.79 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.28 g⊕ (12.55 m/s²), and an escape velocity of 15.3 km/s.
In its orbital architecture around K2-80, K2-80 c completes one full revolution every 5.605 Earth days at a semi-major axis of 0.0596 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 115.7 km/s (compared to Earth's 29.8 km/s).
⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1002 K (+729°C / +1344°F) and receiving 166.00 S⊕ (~225,926 W/m²), K2-80 c orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star K2-80 is classified as a stellar host with an effective photospheric temperature of 5,441 K, a radius of 0.87 R☉, a mass of 0.9 M☉, an estimated bolometric luminosity of 0.595 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = 0.07 dex (metal-rich relative to the Sun). From Earth, K2-80 shines at apparent V-band magnitude 12.694 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The K2-80 system is a multi-planet architecture hosting 3 confirmed worlds, with K2-80 c sharing its stellar neighborhood alongside K2-80 b, K2-80 d.
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 | K2-80 |
| Spectral Type | Unclassified |
| Effective Temp (Teff) | 5,441 K |
| Stellar Radius | 0.8700 R☉ |
| Stellar Mass | 0.9000 M☉ |
| Bolometric Luminosity | 0.595 L☉ |
| Metallicity [Fe/H] | 0.070 dex |
| Stellar Age | — |
| Apparent Magnitude | V: 12.694 · G: 12.377 |
| System Architecture | 1 Star, 3 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | 0.059600 AU |
| Orbital Period | 5.605 days |
| Mean Orbital Velocity | 115.7 km/s |
| Orbital Eccentricity (e) | Circular (0.00) |
| Orbital Inclination (i) | 87.9164° |
| Mean Bulk Density | 4.79 g/cm³ (15.3 km/s vesc) |
| Insolation Flux | 166.0000 S⊕ (~225,926 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 654.900 LY (200.802 pc) |