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CONFIRMED EXOPLANET · Gas Giant

OGLE-2019-BLG-0468L c

Orbits Host Star: OGLE-2019-BLG-0468L (Type G) · Distance: 14350.900 Light-Years (4400.000 pc)
Planetary Radius
12.500 R⊕
Planetary Mass
3248.206 M⊕
Surface Gravity
20.79 g / g⊕
Equilibrium Temp
—
Orbital Period
—
Discovery Year
2022 (Microlensing)
Earth Similarity (ESI)
0.38 / 1.00

Astrophysical Synthesis & Habitability Characterization

OGLE-2019-BLG-0468L c is a confirmed gas giant exoplanet orbiting the star OGLE-2019-BLG-0468L, located approximately 14350.9 light-years (4400 parsecs) from the Solar System. First announced in 2022 by OGLE using the Microlensing detection technique (detected via relativistic gravitational lensing of a background source star), this world measures 12.5 Earth radii (1.12 Jupiter radii) and has a measured mass of 3248.206 Earth masses (10.22 Jupiter masses). Combining its mass and radius yields a mean bulk density of 9.17 g/cm³ (an iron-enriched, high-compression rocky core), a surface gravity of 20.79 g⊕ (203.88 m/s²), and an escape velocity of 180.3 km/s.

☁️ Atmospheric Regime (Volatile / Gas Envelope): With a radius of 12.500 R⊕, OGLE-2019-BLG-0468L 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 OGLE-2019-BLG-0468L is classified as a solar-type yellow star of spectral type G with a mass of 0.92 M☉. The OGLE-2019-BLG-0468L system is a multi-planet architecture hosting 2 confirmed worlds, with OGLE-2019-BLG-0468L c sharing its stellar neighborhood alongside OGLE-2019-BLG-0468L b.

Earth Similarity Index (ESI): 0.38 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: OGLE · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name OGLE-2019-BLG-0468L
Spectral Type G
Effective Temp (Teff) —
Stellar Radius —
Stellar Mass 0.9200 M☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude —
System Architecture 1 Star, 2 Planets

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 2.770000 AU
Orbital Period —
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 9.17 g/cm³ (180.3 km/s vesc)
Insolation Flux —
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 14350.900 LY (4400.000 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 17h45m37.44s · DEC: -24d26m50.2s (J2000: 266.406°, -24.44728°)
Target Field: OGLE-2019-BLG-0468L (J2000 266.406°, -24.44728°)
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 OGLE-2019-BLG-0468L System (1)

NASA EXOPLANET ARCHIVE COMPOSITE PARAMETERS
Inspect Raw NASA Archive Record ↗