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CONFIRMED EXOPLANET · Super-Earth

K2-269 b

Orbits Host Star: K2-269 · Distance: 1176.600 Light-Years (360.760 pc)
Planetary Radius
1.570 R⊕
Planetary Mass
3.090 M⊕
Surface Gravity
1.25 g / g⊕
Equilibrium Temp
1429K (+1156°C / +2113°F)
Orbital Period
4.145 days
Discovery Year
2018 (Transit)
Earth Similarity (ESI)
0.20 / 1.00
Insolation Flux
1,041.53 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-269 b is a confirmed super-earth exoplanet orbiting the star K2-269, located approximately 1176.6 light-years (360.76 parsecs) from the Solar System. First announced in 2018 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.0099% across the stellar disk), this world measures 1.57 Earth radii and has a measured mass of 3.09 Earth masses. Combining its mass and radius yields a mean bulk density of 4.4 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.25 g⊕ (12.26 m/s²), and an escape velocity of 15.7 km/s.

In its orbital architecture around K2-269, K2-269 b completes one full revolution every 4.145 Earth days at a semi-major axis of 0.0531 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 139.4 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1429 K (+1156°C / +2113°F) and receiving 1,041.53 S⊕ (~1,417,519 W/m²), K2-269 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-269 is classified as a stellar host with an effective photospheric temperature of 6,209 K, a radius of 1.45 R☉, a mass of 1.16 M☉, an estimated bolometric luminosity of 2.804 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.08 dex (near-solar heavy-element abundance). From Earth, K2-269 shines at apparent V-band magnitude 11.784 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.20 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 K2-269
Spectral Type Unclassified
Effective Temp (Teff) 6,209 K
Stellar Radius 1.4500 R☉
Stellar Mass 1.1600 M☉
Bolometric Luminosity 2.804 L☉
Metallicity [Fe/H] -0.080 dex
Stellar Age —
Apparent Magnitude V: 11.784 · G: 11.377
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.053100 AU
Orbital Period 4.145 days
Mean Orbital Velocity 139.4 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 86.7200°
Mean Bulk Density 4.4 g/cm³ (15.7 km/s vesc)
Insolation Flux 1041.5274 S⊕ (~1,417,519 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1176.600 LY (360.760 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 08h40m37.23s · DEC: +13d00m52.85s (J2000: 130.15514°, 13.01468°)
Target Field: K2-269 (J2000 130.15514°, 13.01468°)
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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