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CONFIRMED EXOPLANET · Gas Giant

KMT-2022-BLG-1818L c

Orbits Host Star: KMT-2022-BLG-1818L · Distance: 17286.300 Light-Years (5300.000 pc)
Planetary Radius
13.200 R⊕
Planetary Mass
114.418 M⊕
Surface Gravity
0.66 g / g⊕
Equilibrium Temp
—
Orbital Period
—
Discovery Year
2026 (Microlensing)
Earth Similarity (ESI)
0.25 / 1.00

Astrophysical Synthesis & Habitability Characterization

KMT-2022-BLG-1818L c is a confirmed gas giant exoplanet orbiting the star KMT-2022-BLG-1818L, located approximately 17286.3 light-years (5300 parsecs) from the Solar System. First announced in 2026 by KMTNet using the Microlensing detection technique (detected via relativistic gravitational lensing of a background source star), this world measures 13.2 Earth radii (1.18 Jupiter radii) and has a measured mass of 114.418 Earth masses (0.36 Jupiter masses). Combining its mass and radius yields a mean bulk density of 0.27 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.66 g⊕ (6.47 m/s²), and an escape velocity of 32.9 km/s.

☁️ Atmospheric Regime (Volatile / Gas Envelope): With a radius of 13.200 R⊕, KMT-2022-BLG-1818L c exceeds the empirical ~1.8–2.2 R⊕ Fulton radius valley threshold, indicating a substantial hydrogen-helium or supercritical volatile envelope without a conventional solid terrestrial surface.

The host star KMT-2022-BLG-1818L is classified as a stellar host with a mass of 0.79 M☉. The KMT-2022-BLG-1818L system is a multi-planet architecture hosting 2 confirmed worlds, with KMT-2022-BLG-1818L c sharing its stellar neighborhood alongside KMT-2022-BLG-1818L b.

Earth Similarity Index (ESI): 0.25 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: KMTNet · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name KMT-2022-BLG-1818L
Spectral Type Unclassified
Effective Temp (Teff) —
Stellar Radius —
Stellar Mass 0.7900 M☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude —
System Architecture 1 Star, 2 Planets

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 12.600000 AU
Orbital Period —
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 0.27 g/cm³ (32.9 km/s vesc)
Insolation Flux —
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 17286.300 LY (5300.000 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 18h03m11.67s · DEC: -27d28m52.00s (J2000: 270.79863°, -27.48111°)
Target Field: KMT-2022-BLG-1818L (J2000 270.79863°, -27.48111°)
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 ↗

Other Worlds in the KMT-2022-BLG-1818L System (1)

NASA EXOPLANET ARCHIVE COMPOSITE PARAMETERS
Inspect Raw NASA Archive Record ↗