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CONFIRMED EXOPLANET · Gas Giant

TOI-2200 b

Orbits Host Star: TOI-2200 · Distance: 819.500 Light-Years (251.245 pc)
Planetary Radius
6.963 R⊕
Planetary Mass
38.700 M⊕
Surface Gravity
0.8 g / g⊕
Equilibrium Temp
1147K (+874°C / +1605°F)
Orbital Period
2.936 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.14 / 1.00
Insolation Flux
288.09 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-2200 b is a confirmed gas giant exoplanet orbiting the star TOI-2200, located approximately 819.5 light-years (251.25 parsecs) from the Solar System. First announced in 2026 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.597% across the stellar disk), this world measures 6.963 Earth radii (0.62 Jupiter radii) and has a measured mass of 38.7 Earth masses (0.12 Jupiter masses). Combining its mass and radius yields a mean bulk density of 0.63 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.8 g⊕ (7.85 m/s²), and an escape velocity of 26.4 km/s.

In its orbital architecture around TOI-2200, TOI-2200 b completes one full revolution every 2.936 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1147 K (+874°C / +1605°F) and receiving 288.09 S⊕ (~392,086 W/m²), TOI-2200 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-2200 is classified as a stellar host with an effective photospheric temperature of 5,036 K, a radius of 0.8262 R☉, a mass of 0.85 M☉, an estimated bolometric luminosity of 0.394 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = 0.273 dex (metal-rich relative to the Sun). From Earth, TOI-2200 shines at apparent V-band magnitude 13.085 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.14 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-2200
Spectral Type Unclassified
Effective Temp (Teff) 5,036 K
Stellar Radius 0.8262 R☉
Stellar Mass 0.8500 M☉
Bolometric Luminosity 0.394 L☉
Metallicity [Fe/H] 0.273 dex
Stellar Age —
Apparent Magnitude V: 13.085 · G: 12.904
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 2.936 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.6445°
Mean Bulk Density 0.63 g/cm³ (26.4 km/s vesc)
Insolation Flux 288.0870 S⊕ (~392,086 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 819.500 LY (251.245 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 06h35m08.04s · DEC: -72d27m24.40s (J2000: 98.78351°, -72.45678°)
Target Field: TOI-2200 (J2000 98.78351°, -72.45678°)
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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