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CONFIRMED EXOPLANET · Sub-Neptune

TOI-3082 b

Orbits Host Star: TOI-3082 · Distance: 368.700 Light-Years (113.048 pc)
Planetary Radius
3.662 R⊕
Planetary Mass
13.000 M⊕
Surface Gravity
0.97 g / g⊕
Equilibrium Temp
1033K (+760°C / +1400°F)
Orbital Period
1.927 days
Discovery Year
2023 (Transit)
Earth Similarity (ESI)
0.21 / 1.00
Insolation Flux
131.65 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-3082 b is a confirmed sub-neptune exoplanet orbiting the star TOI-3082, located approximately 368.7 light-years (113.05 parsecs) from the Solar System. First announced in 2023 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.2404% across the stellar disk), this world measures 3.662 Earth radii (0.33 Jupiter radii) and has a measured mass of 13 Earth masses. Combining its mass and radius yields a mean bulk density of 1.46 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.97 g⊕ (9.51 m/s²), and an escape velocity of 21.1 km/s.

In its orbital architecture around TOI-3082, TOI-3082 b completes one full revolution every 1.927 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1033 K (+760°C / +1400°F) and receiving 131.65 S⊕ (~179,173 W/m²), TOI-3082 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-3082 is classified as a stellar host with an effective photospheric temperature of 4,263 K, a radius of 0.6847 R☉, a mass of 0.664 M☉, an estimated bolometric luminosity of 0.139 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = 0.17 dex (metal-rich relative to the Sun). From Earth, TOI-3082 shines at apparent V-band magnitude 12.934 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.21 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-3082
Spectral Type Unclassified
Effective Temp (Teff) 4,263 K
Stellar Radius 0.6847 R☉
Stellar Mass 0.6640 M☉
Bolometric Luminosity 0.139 L☉
Metallicity [Fe/H] 0.170 dex
Stellar Age —
Apparent Magnitude V: 12.934 · G: 12.531
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 1.927 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 87.6300°
Mean Bulk Density 1.46 g/cm³ (21.1 km/s vesc)
Insolation Flux 131.6480 S⊕ (~179,173 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 368.700 LY (113.048 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 13h03m37.94s · DEC: -19d13m08.34s (J2000: 195.90807°, -19.21898°)
Target Field: TOI-3082 (J2000 195.90807°, -19.21898°)
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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