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CONFIRMED EXOPLANET · Gas Giant

K2-121 b

Orbits Host Star: K2-121 · Distance: 552.500 Light-Years (169.398 pc)
Planetary Radius
7.160 R⊕
Planetary Mass
51.000 M⊕
Surface Gravity
0.99 g / g⊕
Equilibrium Temp
716K (+443°C / +829°F)
Orbital Period
5.186 days
Discovery Year
2017 (Transit)
Earth Similarity (ESI)
0.23 / 1.00
Insolation Flux
62.50 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-121 b is a confirmed gas giant exoplanet orbiting the star K2-121, located approximately 552.5 light-years (169.4 parsecs) from the Solar System. First announced in 2017 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.9457% across the stellar disk), this world measures 7.16 Earth radii (0.64 Jupiter radii) and has a measured mass of 51 Earth masses (0.16 Jupiter masses). Combining its mass and radius yields a mean bulk density of 0.77 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.99 g⊕ (9.71 m/s²), and an escape velocity of 29.9 km/s.

In its orbital architecture around K2-121, K2-121 b completes one full revolution every 5.186 Earth days at a semi-major axis of 0.0525 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 110.1 km/s (compared to Earth's 29.8 km/s). Its moderate orbital eccentricity of e = 0.22 carries the world between 0.041 AU at periapsis and 0.0641 AU at apoapsis, driving measurable seasonal insolation cycles.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 716 K (+443°C / +829°F) and receiving 62.50 S⊕ (~85,063 W/m²), K2-121 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-121 is classified as a stellar host with an effective photospheric temperature of 4,526 K, a radius of 0.675 R☉, a mass of 0.71 M☉, an estimated bolometric luminosity of 0.172 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = 0.04 dex (near-solar heavy-element abundance). From Earth, K2-121 shines at apparent V-band magnitude 13.229 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.23 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 K2-121
Spectral Type Unclassified
Effective Temp (Teff) 4,526 K
Stellar Radius 0.6750 R☉
Stellar Mass 0.7100 M☉
Bolometric Luminosity 0.172 L☉
Metallicity [Fe/H] 0.040 dex
Stellar Age —
Apparent Magnitude V: 13.229 · G: 12.925
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.052500 AU
Orbital Period 5.186 days
Mean Orbital Velocity 110.1 km/s
Orbital Eccentricity (e) 0.22000
Orbital Inclination (i) 89.0266°
Mean Bulk Density 0.77 g/cm³ (29.9 km/s vesc)
Insolation Flux 62.5000 S⊕ (~85,063 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 552.500 LY (169.398 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 08h27m44.80s · DEC: +17d34m45.58s (J2000: 126.93666°, 17.57933°)
Target Field: K2-121 (J2000 126.93666°, 17.57933°)
Surveys available: Digitized Sky Survey (DSS2 Optical), 2MASS (Near-Infrared), AllWISE (Mid-Infrared) · Field of View: 0.18° (10.8 arcmin)
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