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CONFIRMED EXOPLANET · Sub-Neptune

TOI-6080 b

Orbits Host Star: TOI-6080 · Distance: 613.800 Light-Years (188.183 pc)
Planetary Radius
3.324 R⊕
Planetary Mass
11.000 M⊕
Surface Gravity
1 g / g⊕
Equilibrium Temp
919K (+646°C / +1195°F)
Orbital Period
8.056 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.24 / 1.00
Insolation Flux
168.81 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-6080 b is a confirmed sub-neptune exoplanet orbiting the star TOI-6080, located approximately 613.8 light-years (188.18 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 0.0823% across the stellar disk), this world measures 3.324 Earth radii (0.3 Jupiter radii) and has a measured mass of 11 Earth masses. Combining its mass and radius yields a mean bulk density of 1.65 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 1 g⊕ (9.81 m/s²), and an escape velocity of 20.3 km/s.

In its orbital architecture around TOI-6080, TOI-6080 b completes one full revolution every 8.056 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 919 K (+646°C / +1195°F) and receiving 168.81 S⊕ (~229,753 W/m²), TOI-6080 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-6080 is classified as a stellar host with an effective photospheric temperature of 5,775 K, a radius of 1.0622 R☉, a mass of 1.01 M☉, an estimated bolometric luminosity of 1.126 L☉. From Earth, TOI-6080 shines at apparent V-band magnitude 11.178 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.24 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-6080
Spectral Type Unclassified
Effective Temp (Teff) 5,775 K
Stellar Radius 1.0622 R☉
Stellar Mass 1.0100 M☉
Bolometric Luminosity 1.126 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 11.178 · G: 11.049
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 8.056 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.0835°
Mean Bulk Density 1.65 g/cm³ (20.3 km/s vesc)
Insolation Flux 168.8120 S⊕ (~229,753 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 613.800 LY (188.183 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 17h46m25.06s · DEC: +38d04m43.35s (J2000: 266.60442°, 38.07871°)
Target Field: TOI-6080 (J2000 266.60442°, 38.07871°)
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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