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CONFIRMED EXOPLANET · Sub-Neptune

TOI-5174 b

Orbits Host Star: TOI-5174 · Distance: 643.300 Light-Years (197.243 pc)
Planetary Radius
5.351 R⊕
Planetary Mass
24.800 M⊕
Surface Gravity
0.87 g / g⊕
Equilibrium Temp
808K (+535°C / +995°F)
Orbital Period
12.214 days
Discovery Year
2022 (Transit)
Earth Similarity (ESI)
0.23 / 1.00
Insolation Flux
100.91 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-5174 b is a confirmed sub-neptune exoplanet orbiting the star TOI-5174, located approximately 643.3 light-years (197.24 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 0.2009% across the stellar disk), this world measures 5.351 Earth radii (0.48 Jupiter radii) and has a measured mass of 24.8 Earth masses. Combining its mass and radius yields a mean bulk density of 0.89 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.87 g⊕ (8.53 m/s²), and an escape velocity of 24.1 km/s.

In its orbital architecture around TOI-5174, TOI-5174 b completes one full revolution every 12.214 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 808 K (+535°C / +995°F) and receiving 100.91 S⊕ (~137,340 W/m²), TOI-5174 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-5174 is classified as a stellar host with an effective photospheric temperature of 5,644 K, a radius of 1.0946 R☉, a mass of 1 M☉, an estimated bolometric luminosity of 1.091 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = 0.415 dex (metal-rich relative to the Sun). From Earth, TOI-5174 shines at apparent V-band magnitude 11.583 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.23 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-5174
Spectral Type Unclassified
Effective Temp (Teff) 5,644 K
Stellar Radius 1.0946 R☉
Stellar Mass 1.0000 M☉
Bolometric Luminosity 1.091 L☉
Metallicity [Fe/H] 0.415 dex
Stellar Age —
Apparent Magnitude V: 11.583 · G: 11.103
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 12.214 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 0.89 g/cm³ (24.1 km/s vesc)
Insolation Flux 100.9112 S⊕ (~137,340 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 643.300 LY (197.243 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 11h36m26.28s · DEC: -02d01m24.06s (J2000: 174.1095°, -2.02335°)
Target Field: TOI-5174 (J2000 174.1095°, -2.02335°)
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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