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CONFIRMED EXOPLANET · Sub-Neptune

TOI-808 b

Orbits Host Star: TOI-808 · Distance: 320.200 Light-Years (98.185 pc)
Planetary Radius
2.203 R⊕
Planetary Mass
5.490 M⊕
Surface Gravity
1.13 g / g⊕
Equilibrium Temp
711K (+438°C / +820°F)
Orbital Period
9.739 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.37 / 1.00
Insolation Flux
60.39 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-808 b is a confirmed sub-neptune exoplanet orbiting the star TOI-808, located approximately 320.2 light-years (98.19 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 0.0588% across the stellar disk), this world measures 2.203 Earth radii and has a measured mass of 5.49 Earth masses. Combining its mass and radius yields a mean bulk density of 2.83 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.13 g⊕ (11.08 m/s²), and an escape velocity of 17.7 km/s.

In its orbital architecture around TOI-808, TOI-808 b completes one full revolution every 9.739 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 711 K (+438°C / +820°F) and receiving 60.39 S⊕ (~82,188 W/m²), TOI-808 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-808 is classified as a stellar host with an effective photospheric temperature of 5,078 K, a radius of 0.8332 R☉, a mass of 0.87 M☉, an estimated bolometric luminosity of 0.414 L☉. From Earth, TOI-808 shines at apparent V-band magnitude 10.729 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.37 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-808
Spectral Type Unclassified
Effective Temp (Teff) 5,078 K
Stellar Radius 0.8332 R☉
Stellar Mass 0.8700 M☉
Bolometric Luminosity 0.414 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 10.729 · G: 10.603
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 9.739 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.4232°
Mean Bulk Density 2.83 g/cm³ (17.7 km/s vesc)
Insolation Flux 60.3881 S⊕ (~82,188 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 320.200 LY (98.185 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 08h54m59.65s · DEC: -44d17m19.07s (J2000: 133.74855°, -44.28863°)
Target Field: TOI-808 (J2000 133.74855°, -44.28863°)
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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