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CONFIRMED EXOPLANET · Sub-Neptune

K2-292 b

Orbits Host Star: K2-292 (Type G3 V) · Distance: 372.800 Light-Years (114.293 pc)
Planetary Radius
2.630 R⊕
Planetary Mass
24.500 M⊕
Surface Gravity
3.54 g / g⊕
Equilibrium Temp
795K (+522°C / +972°F)
Orbital Period
16.984 days
Discovery Year
2019 (Transit)
Earth Similarity (ESI)
0.32 / 1.00
Insolation Flux
67.00 S⊕

Astrophysical Synthesis & Habitability Characterization

K2-292 b is a confirmed sub-neptune exoplanet orbiting the star K2-292, located approximately 372.8 light-years (114.29 parsecs) from the Solar System. First announced in 2019 by K2 using the Transit detection technique (producing an estimated primary transit depth of 0.0489% across the stellar disk), this world measures 2.63 Earth radii and has a measured mass of 24.5 Earth masses. Combining its mass and radius yields a mean bulk density of 7.43 g/cm³ (an iron-enriched, high-compression rocky core), a surface gravity of 3.54 g⊕ (34.72 m/s²), and an escape velocity of 34.1 km/s.

In its orbital architecture around K2-292, K2-292 b completes one full revolution every 16.984 Earth days at a semi-major axis of 0.13 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 83.3 km/s (compared to Earth's 29.8 km/s). With a near-circular eccentricity of e = 0.04 (ranging from 0.1248 AU at periapsis to 0.1352 AU at apoapsis), the planet experiences minimal orbital distance variation.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 795 K (+522°C / +972°F) and receiving 67.00 S⊕ (~91,187 W/m²), K2-292 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star K2-292 is classified as a solar-type yellow star of spectral type G3 V with an effective photospheric temperature of 5,725 K, a radius of 1.09 R☉, a mass of 1 M☉, an estimated bolometric luminosity of 1.145 L☉. Stellar evolution modeling indicates an estimated stellar age of 6.8 Gyr and a metallicity of [Fe/H] = 0.07 dex (metal-rich relative to the Sun). From Earth, K2-292 shines at apparent V-band magnitude 9.885 (accessible to binoculars and small amateur telescopes) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.32 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 K2-292
Spectral Type G3 V
Effective Temp (Teff) 5,725 K
Stellar Radius 1.0900 R☉
Stellar Mass 1.0000 M☉
Bolometric Luminosity 1.145 L☉
Metallicity [Fe/H] 0.070 dex
Stellar Age 6.800 Gyr
Apparent Magnitude V: 9.885 · G: 9.756
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.130000 AU
Orbital Period 16.984 days
Mean Orbital Velocity 83.3 km/s
Orbital Eccentricity (e) 0.04000
Orbital Inclination (i) 88.4000°
Mean Bulk Density 7.43 g/cm³ (34.1 km/s vesc)
Insolation Flux 67.0000 S⊕ (~91,187 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 372.800 LY (114.293 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 13h41m30.21s · DEC: -09d56m45.85s (J2000: 205.37588°, -9.94607°)
Target Field: K2-292 (J2000 205.37588°, -9.94607°)
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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