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CONFIRMED EXOPLANET · Sub-Neptune

TOI-682.01

Orbits Host Star: TOI-682 · Distance: 271.200 Light-Years (83.155 pc)
Planetary Radius
3.742 R⊕
Planetary Mass
13.500 M⊕
Surface Gravity
0.96 g / g⊕
Equilibrium Temp
1090K (+817°C / +1503°F)
Orbital Period
6.839 days
Discovery Year
2021 (Transit)
Earth Similarity (ESI)
0.19 / 1.00
Insolation Flux
234.46 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-682.01 is a confirmed sub-neptune exoplanet orbiting the star TOI-682, located approximately 271.2 light-years (83.16 parsecs) from the Solar System. First announced in 2021 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.1009% across the stellar disk), this world measures 3.742 Earth radii (0.33 Jupiter radii) and has a measured mass of 13.5 Earth masses. Combining its mass and radius yields a mean bulk density of 1.42 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.96 g⊕ (9.41 m/s²), and an escape velocity of 21.2 km/s.

In its orbital architecture around TOI-682, TOI-682.01 completes one full revolution every 6.839 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1090 K (+817°C / +1503°F) and receiving 234.46 S⊕ (~319,100 W/m²), TOI-682.01 orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-682 is classified as a stellar host with an effective photospheric temperature of 5,085 K, a radius of 1.08 R☉, a mass of 0.85 M☉, an estimated bolometric luminosity of 0.7 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = 0.27 dex (metal-rich relative to the Sun). From Earth, TOI-682 shines at apparent V-band magnitude 9.969 (accessible to binoculars and small amateur telescopes) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.19 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-682
Spectral Type Unclassified
Effective Temp (Teff) 5,085 K
Stellar Radius 1.0800 R☉
Stellar Mass 0.8500 M☉
Bolometric Luminosity 0.7 L☉
Metallicity [Fe/H] 0.270 dex
Stellar Age —
Apparent Magnitude V: 9.969 · G: 9.742
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 6.839 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 1.42 g/cm³ (21.2 km/s vesc)
Insolation Flux 234.4600 S⊕ (~319,100 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 271.200 LY (83.155 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 11h11m32.50s · DEC: -22d04m22.01s (J2000: 167.88543°, -22.07278°)
Target Field: TOI-682 (J2000 167.88543°, -22.07278°)
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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