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CONFIRMED EXOPLANET · Super-Earth

K2-149 b

Orbits Host Star: K2-149 (Type M1.0 V) · Distance: 403.400 Light-Years (123.676 pc)
Planetary Radius
1.640 R⊕
Planetary Mass
3.330 M⊕
Surface Gravity
1.24 g / g⊕
Equilibrium Temp
472K (+199°C / +390°F)
Orbital Period
11.332 days
Discovery Year
2018 (Transit)
Earth Similarity (ESI)
0.61 / 1.00
Insolation Flux
7.00 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-149 b is a confirmed super-earth exoplanet orbiting the star K2-149, located approximately 403.4 light-years (123.68 parsecs) from the Solar System. First announced in 2018 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.0701% across the stellar disk), this world measures 1.64 Earth radii and has a measured mass of 3.33 Earth masses. Combining its mass and radius yields a mean bulk density of 4.16 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.24 g⊕ (12.16 m/s²), and an escape velocity of 15.9 km/s.

In its orbital architecture around K2-149, K2-149 b completes one full revolution every 11.332 Earth days at a semi-major axis of 0.083 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 79.7 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 472 K (+199°C / +390°F) and receiving 7.00 S⊕ (~9,527 W/m²), K2-149 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-149 is classified as a low-mass red dwarf of spectral type M1.0 V with an effective photospheric temperature of 3,745 K, a radius of 0.568 R☉, a mass of 0.595 M☉, an estimated bolometric luminosity of 0.057 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = 0.11 dex (metal-rich relative to the Sun). From Earth, K2-149 shines at apparent V-band magnitude 14.543 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.61 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 K2-149
Spectral Type M1.0 V
Effective Temp (Teff) 3,745 K
Stellar Radius 0.5680 R☉
Stellar Mass 0.5950 M☉
Bolometric Luminosity 0.057 L☉
Metallicity [Fe/H] 0.110 dex
Stellar Age —
Apparent Magnitude V: 14.543 · G: 13.780
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.083000 AU
Orbital Period 11.332 days
Mean Orbital Velocity 79.7 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 4.16 g/cm³ (15.9 km/s vesc)
Insolation Flux 7.0000 S⊕ (~9,527 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 403.400 LY (123.676 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 00h39m17.22s · DEC: +07d16m37.18s (J2000: 9.82175°, 7.27699°)
Target Field: K2-149 (J2000 9.82175°, 7.27699°)
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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