STATION 02: EXOPLANETLEDGER.ORG · WORLD DOSSIER // K2-248 b
← Return to All Worlds
CONFIRMED EXOPLANET · Sub-Neptune

K2-248 b

Orbits Host Star: K2-248 · Distance: 1325.000 Light-Years (406.254 pc)
Planetary Radius
2.570 R⊕
Planetary Mass
7.130 M⊕
Surface Gravity
1.08 g / g⊕
Equilibrium Temp
886K (+613°C / +1135°F)
Orbital Period
7.173 days
Discovery Year
2018 (Transit)
Earth Similarity (ESI)
0.28 / 1.00
Insolation Flux
132.33 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-248 b is a confirmed sub-neptune exoplanet orbiting the star K2-248, located approximately 1325 light-years (406.25 parsecs) from the Solar System. First announced in 2018 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.0656% across the stellar disk), this world measures 2.57 Earth radii and has a measured mass of 7.13 Earth masses. Combining its mass and radius yields a mean bulk density of 2.32 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.08 g⊕ (10.59 m/s²), and an escape velocity of 18.6 km/s.

In its orbital architecture around K2-248, K2-248 b completes one full revolution every 7.173 Earth days at a semi-major axis of 0.0699 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 106 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 886 K (+613°C / +1135°F) and receiving 132.33 S⊕ (~180,104 W/m²), K2-248 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-248 is classified as a stellar host with an effective photospheric temperature of 5,528 K, a radius of 0.92 R☉, a mass of 0.88 M☉, an estimated bolometric luminosity of 0.709 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.1 dex (near-solar heavy-element abundance). From Earth, K2-248 shines at apparent V-band magnitude 13.497 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.28 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 K2-248
Spectral Type Unclassified
Effective Temp (Teff) 5,528 K
Stellar Radius 0.9200 R☉
Stellar Mass 0.8800 M☉
Bolometric Luminosity 0.709 L☉
Metallicity [Fe/H] -0.100 dex
Stellar Age —
Apparent Magnitude V: 13.497 · G: 13.262
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.069900 AU
Orbital Period 7.173 days
Mean Orbital Velocity 106 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 2.32 g/cm³ (18.6 km/s vesc)
Insolation Flux 132.3323 S⊕ (~180,104 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1325.000 LY (406.254 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 12h11m16.16s · DEC: -09d24m51.01s (J2000: 182.81733°, -9.41417°)
Target Field: K2-248 (J2000 182.81733°, -9.41417°)
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 ↗