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CONFIRMED EXOPLANET · Gas Giant

TOI-2184 b

Orbits Host Star: TOI-2184 · Distance: 2571.100 Light-Years (788.317 pc)
Planetary Radius
11.400 R⊕
Planetary Mass
206.588 M⊕
Surface Gravity
1.59 g / g⊕
Equilibrium Temp
1676K (+1403°C / +2557°F)
Orbital Period
6.907 days
Discovery Year
2022 (Transit)
Earth Similarity (ESI)
0.08 / 1.00
Insolation Flux
1,429.00 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-2184 b is a confirmed gas giant exoplanet orbiting the star TOI-2184, located approximately 2571.1 light-years (788.32 parsecs) from the Solar System. First announced in 2022 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.1299% across the stellar disk), this world measures 11.4 Earth radii (1.02 Jupiter radii) and has a measured mass of 206.588 Earth masses (0.65 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 1.59 g⊕ (15.59 m/s²), and an escape velocity of 47.6 km/s.

In its orbital architecture around TOI-2184, TOI-2184 b completes one full revolution every 6.907 Earth days. Its moderate orbital eccentricity of e = 0.08 driving measurable seasonal insolation cycles.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1676 K (+1403°C / +2557°F) and receiving 1,429.00 S⊕ (~1,944,869 W/m²), TOI-2184 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-2184 is classified as a stellar host with an effective photospheric temperature of 5,966 K, a radius of 2.9 R☉, a mass of 1.53 M☉, an estimated bolometric luminosity of 9.559 L☉. Stellar evolution modeling indicates an estimated stellar age of 2.3 Gyr and a metallicity of [Fe/H] = 0.14 dex (metal-rich relative to the Sun). From Earth, TOI-2184 shines at apparent V-band magnitude 12.254 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.08 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: Transiting Exoplanet Survey Satellite (TESS) · Catalogue Source: NASA Exoplanet Archive (IPAC / Caltech).

☀️ Host Star Telemetry

Host Star Name TOI-2184
Spectral Type Unclassified
Effective Temp (Teff) 5,966 K
Stellar Radius 2.9000 R☉
Stellar Mass 1.5300 M☉
Bolometric Luminosity 9.559 L☉
Metallicity [Fe/H] 0.140 dex
Stellar Age 2.300 Gyr
Apparent Magnitude V: 12.254 · G: 11.848
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 6.907 days
Orbital Eccentricity (e) 0.08000
Orbital Inclination (i) —
Mean Bulk Density 0.77 g/cm³ (47.6 km/s vesc)
Insolation Flux 1429.0000 S⊕ (~1,944,869 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 2571.100 LY (788.317 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 06h43m19.95s · DEC: -66d56m51.56s (J2000: 100.83312°, -66.94766°)
Target Field: TOI-2184 (J2000 100.83312°, -66.94766°)
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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