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CONFIRMED EXOPLANET · Terrestrial

K2-279 b

Orbits Host Star: K2-279 · Distance: 596.800 Light-Years (182.983 pc)
Planetary Radius
1.210 R⊕
Planetary Mass
1.920 M⊕
Surface Gravity
1.31 g / g⊕
Equilibrium Temp
879K (+606°C / +1123°F)
Orbital Period
7.123 days
Discovery Year
2018 (Transit)
Earth Similarity (ESI)
0.36 / 1.00
Insolation Flux
139.11 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-279 b is a confirmed terrestrial exoplanet orbiting the star K2-279, located approximately 596.8 light-years (182.98 parsecs) from the Solar System. First announced in 2018 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.0166% across the stellar disk), this world measures 1.21 Earth radii and has a measured mass of 1.92 Earth masses. Combining its mass and radius yields a mean bulk density of 5.98 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.31 g⊕ (12.85 m/s²), and an escape velocity of 14.1 km/s.

In its orbital architecture around K2-279, K2-279 b completes one full revolution every 7.123 Earth days at a semi-major axis of 0.067 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 102.3 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 879 K (+606°C / +1123°F) and receiving 139.11 S⊕ (~189,323 W/m²), K2-279 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-279 is classified as a stellar host with an effective photospheric temperature of 5,558 K, a radius of 0.86 R☉, a mass of 0.79 M☉, an estimated bolometric luminosity of 0.633 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.37 dex (metal-poor relative to the Sun). From Earth, K2-279 shines at apparent V-band magnitude 11.491 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.36 Earth Baseline = 1.00
0.00 Dissimilar 0.50 Mars Scale 0.70 Analog Regime 1.00 Earth

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 K2-279
Spectral Type Unclassified
Effective Temp (Teff) 5,558 K
Stellar Radius 0.8600 R☉
Stellar Mass 0.7900 M☉
Bolometric Luminosity 0.633 L☉
Metallicity [Fe/H] -0.370 dex
Stellar Age —
Apparent Magnitude V: 11.491 · G: 11.591
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.067000 AU
Orbital Period 7.123 days
Mean Orbital Velocity 102.3 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 5.98 g/cm³ (14.1 km/s vesc)
Insolation Flux 139.1055 S⊕ (~189,323 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 596.800 LY (182.983 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 13h39m07.03s · DEC: -06d02m30.33s (J2000: 204.77929°, -6.04176°)
Target Field: K2-279 (J2000 204.77929°, -6.04176°)
Surveys available: Digitized Sky Survey (DSS2 Optical), 2MASS (Near-Infrared), AllWISE (Mid-Infrared) · Field of View: 0.18° (10.8 arcmin)
Aladin Lite v3 · Centre de Données astronomiques de Strasbourg (CDS)
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