STATION 02: EXOPLANETLEDGER.ORG · WORLD DOSSIER // K2-68 b
← Return to All Worlds
CONFIRMED EXOPLANET · Super-Earth

K2-68 b

Orbits Host Star: K2-68 · Distance: 550.100 Light-Years (168.652 pc)
Planetary Radius
1.580 R⊕
Planetary Mass
3.120 M⊕
Surface Gravity
1.25 g / g⊕
Equilibrium Temp
707K (+434°C / +813°F)
Orbital Period
8.054 days
Discovery Year
2016 (Transit)
Earth Similarity (ESI)
0.42 / 1.00
Insolation Flux
41.00 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-68 b is a confirmed super-earth exoplanet orbiting the star K2-68, located approximately 550.1 light-years (168.65 parsecs) from the Solar System. First announced in 2016 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.0461% across the stellar disk), this world measures 1.58 Earth radii and has a measured mass of 3.12 Earth masses. Combining its mass and radius yields a mean bulk density of 4.36 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 K2-68, K2-68 b completes one full revolution every 8.054 Earth days at a semi-major axis of 0.0708 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 95.6 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 707 K (+434°C / +813°F) and receiving 41.00 S⊕ (~55,801 W/m²), K2-68 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-68 is classified as a stellar host with an effective photospheric temperature of 4,746 K, a radius of 0.675 R☉, a mass of 0.73 M☉, an estimated bolometric luminosity of 0.207 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.21 dex (metal-poor relative to the Sun). From Earth, K2-68 shines at apparent V-band magnitude 12.987 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.42 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 K2-68
Spectral Type Unclassified
Effective Temp (Teff) 4,746 K
Stellar Radius 0.6750 R☉
Stellar Mass 0.7300 M☉
Bolometric Luminosity 0.207 L☉
Metallicity [Fe/H] -0.210 dex
Stellar Age —
Apparent Magnitude V: 12.987 · G: 12.657
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.070800 AU
Orbital Period 8.054 days
Mean Orbital Velocity 95.6 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.7153°
Mean Bulk Density 4.36 g/cm³ (15.7 km/s vesc)
Insolation Flux 41.0000 S⊕ (~55,801 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 550.100 LY (168.652 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 22h16m04.69s · DEC: -10d34m02.51s (J2000: 334.01955°, -10.56736°)
Target Field: K2-68 (J2000 334.01955°, -10.56736°)
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 ↗
NASA EXOPLANET ARCHIVE COMPOSITE PARAMETERS
Inspect Raw NASA Archive Record ↗