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CONFIRMED EXOPLANET · Sub-Neptune

TOI-3493 b

Orbits Host Star: TOI-3493 (Type G1/2 V) · Distance: 315.500 Light-Years (96.722 pc)
Planetary Radius
3.220 R⊕
Planetary Mass
8.970 M⊕
Surface Gravity
0.87 g / g⊕
Equilibrium Temp
1102K (+829°C / +1524°F)
Orbital Period
8.159 days
Discovery Year
2025 (Transit)
Earth Similarity (ESI)
0.20 / 1.00
Insolation Flux
245.00 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-3493 b is a confirmed sub-neptune exoplanet orbiting the star TOI-3493, located approximately 315.5 light-years (96.72 parsecs) from the Solar System. First announced in 2025 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.0578% across the stellar disk), this world measures 3.22 Earth radii (0.29 Jupiter radii) and has a measured mass of 8.97 Earth masses. Combining its mass and radius yields a mean bulk density of 1.48 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 18.7 km/s.

In its orbital architecture around TOI-3493, TOI-3493 b completes one full revolution every 8.159 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1102 K (+829°C / +1524°F) and receiving 245.00 S⊕ (~333,445 W/m²), TOI-3493 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-3493 is classified as a solar-type yellow star of spectral type G1/2 V with an effective photospheric temperature of 5,844 K, a radius of 1.228 R☉, a mass of 1.023 M☉, an estimated bolometric luminosity of 1.578 L☉. Stellar evolution modeling indicates an estimated stellar age of 7.3 Gyr and a metallicity of [Fe/H] = 0.03 dex (near-solar heavy-element abundance). From Earth, TOI-3493 shines at apparent V-band magnitude 9.317 (accessible to binoculars and small amateur telescopes) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.20 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-3493
Spectral Type G1/2 V
Effective Temp (Teff) 5,844 K
Stellar Radius 1.2280 R☉
Stellar Mass 1.0230 M☉
Bolometric Luminosity 1.578 L☉
Metallicity [Fe/H] 0.030 dex
Stellar Age 7.300 Gyr
Apparent Magnitude V: 9.317 · G: 9.120
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 8.159 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 89.2500°
Mean Bulk Density 1.48 g/cm³ (18.7 km/s vesc)
Insolation Flux 245.0000 S⊕ (~333,445 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 315.500 LY (96.722 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 13h43m11.77s · DEC: -22d35m07.60s (J2000: 205.79903°, -22.58544°)
Target Field: TOI-3493 (J2000 205.79903°, -22.58544°)
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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