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CONFIRMED EXOPLANET · Gas Giant

TOI-5599 b

Orbits Host Star: TOI-5599 · Distance: 1787.200 Light-Years (547.948 pc)
Planetary Radius
7.189 R⊕
Planetary Mass
40.900 M⊕
Surface Gravity
0.79 g / g⊕
Equilibrium Temp
1496K (+1223°C / +2233°F)
Orbital Period
5.437 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.10 / 1.00
Insolation Flux
833.22 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-5599 b is a confirmed gas giant exoplanet orbiting the star TOI-5599, located approximately 1787.2 light-years (547.95 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 0.1187% across the stellar disk), this world measures 7.189 Earth radii (0.64 Jupiter radii) and has a measured mass of 40.9 Earth masses (0.13 Jupiter masses). Combining its mass and radius yields a mean bulk density of 0.61 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.79 g⊕ (7.75 m/s²), and an escape velocity of 26.7 km/s.

In its orbital architecture around TOI-5599, TOI-5599 b completes one full revolution every 5.437 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1496 K (+1223°C / +2233°F) and receiving 833.22 S⊕ (~1,134,010 W/m²), TOI-5599 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-5599 is classified as a stellar host with an effective photospheric temperature of 6,137 K, a radius of 1.9133 R☉, a mass of 1.21 M☉, an estimated bolometric luminosity of 4.659 L☉. From Earth, TOI-5599 shines at apparent V-band magnitude 11.779 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.10 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-5599
Spectral Type Unclassified
Effective Temp (Teff) 6,137 K
Stellar Radius 1.9133 R☉
Stellar Mass 1.2100 M☉
Bolometric Luminosity 4.659 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 11.779 · G: 11.648
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 5.437 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 87.2305°
Mean Bulk Density 0.61 g/cm³ (26.7 km/s vesc)
Insolation Flux 833.2180 S⊕ (~1,134,010 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1787.200 LY (547.948 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 13h17m18.30s · DEC: +55d40m53.54s (J2000: 199.32624°, 55.68154°)
Target Field: TOI-5599 (J2000 199.32624°, 55.68154°)
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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