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CONFIRMED EXOPLANET · Sub-Neptune

K2-268 c

Orbits Host Star: K2-268 · Distance: 1069.100 Light-Years (327.783 pc)
Planetary Radius
2.690 R⊕
Planetary Mass
7.700 M⊕
Surface Gravity
1.06 g / g⊕
Equilibrium Temp
696K (+423°C / +793°F)
Orbital Period
9.328 days
Discovery Year
2018 (Transit)
Earth Similarity (ESI)
0.35 / 1.00
Insolation Flux
55.46 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-268 c is a confirmed sub-neptune exoplanet orbiting the star K2-268, located approximately 1069.1 light-years (327.78 parsecs) from the Solar System. First announced in 2018 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.1% across the stellar disk), this world measures 2.69 Earth radii and has a measured mass of 7.7 Earth masses. Combining its mass and radius yields a mean bulk density of 2.18 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.06 g⊕ (10.4 m/s²), and an escape velocity of 18.9 km/s.

In its orbital architecture around K2-268, K2-268 c completes one full revolution every 9.328 Earth days at a semi-major axis of 0.0819 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 95.5 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 696 K (+423°C / +793°F) and receiving 55.46 S⊕ (~75,486 W/m²), K2-268 c orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-268 is classified as a stellar host with an effective photospheric temperature of 5,106 K, a radius of 0.78 R☉, a mass of 0.84 M☉, an estimated bolometric luminosity of 0.371 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = 0.03 dex (near-solar heavy-element abundance). From Earth, K2-268 shines at apparent V-band magnitude 13.848 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The K2-268 system is a multi-planet architecture hosting 5 confirmed worlds, with K2-268 c sharing its stellar neighborhood alongside K2-268 b, K2-268 d, K2-268 e, K2-268 f.

Earth Similarity Index (ESI): 0.35 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 K2-268
Spectral Type Unclassified
Effective Temp (Teff) 5,106 K
Stellar Radius 0.7800 R☉
Stellar Mass 0.8400 M☉
Bolometric Luminosity 0.371 L☉
Metallicity [Fe/H] 0.030 dex
Stellar Age —
Apparent Magnitude V: 13.848 · G: 13.563
System Architecture 1 Star, 5 Planets

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.081900 AU
Orbital Period 9.328 days
Mean Orbital Velocity 95.5 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.7100°
Mean Bulk Density 2.18 g/cm³ (18.9 km/s vesc)
Insolation Flux 55.4636 S⊕ (~75,486 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1069.100 LY (327.783 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 08h54m50.28s · DEC: +11d50m53.78s (J2000: 133.70949°, 11.84827°)
Target Field: K2-268 (J2000 133.70949°, 11.84827°)
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)
SIMBAD Astronomical Query ↗ NASA ADS Research Papers ↗

Other Worlds in the K2-268 System (4)

NASA EXOPLANET ARCHIVE COMPOSITE PARAMETERS
Inspect Raw NASA Archive Record ↗