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CONFIRMED EXOPLANET · Sub-Neptune

TOI-799 b

Orbits Host Star: TOI-799 · Distance: 517.000 Light-Years (158.526 pc)
Planetary Radius
2.066 R⊕
Planetary Mass
4.920 M⊕
Surface Gravity
1.15 g / g⊕
Equilibrium Temp
959K (+686°C / +1267°F)
Orbital Period
5.545 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.28 / 1.00
Insolation Flux
199.63 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-799 b is a confirmed sub-neptune exoplanet orbiting the star TOI-799, located approximately 517 light-years (158.53 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 0.0428% across the stellar disk), this world measures 2.066 Earth radii and has a measured mass of 4.92 Earth masses. Combining its mass and radius yields a mean bulk density of 3.08 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.15 g⊕ (11.28 m/s²), and an escape velocity of 17.3 km/s.

In its orbital architecture around TOI-799, TOI-799 b completes one full revolution every 5.545 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 959 K (+686°C / +1267°F) and receiving 199.63 S⊕ (~271,700 W/m²), TOI-799 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-799 is classified as a stellar host with an effective photospheric temperature of 5,663 K, a radius of 0.9155 R☉, a mass of 1 M☉, an estimated bolometric luminosity of 0.773 L☉. From Earth, TOI-799 shines at apparent V-band magnitude 11.195 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.28 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-799
Spectral Type Unclassified
Effective Temp (Teff) 5,663 K
Stellar Radius 0.9155 R☉
Stellar Mass 1.0000 M☉
Bolometric Luminosity 0.773 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 11.195 · G: 11.056
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 5.545 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 87.7697°
Mean Bulk Density 3.08 g/cm³ (17.3 km/s vesc)
Insolation Flux 199.6326 S⊕ (~271,700 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 517.000 LY (158.526 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 06h33m52.59s · DEC: -52d27m37.06s (J2000: 98.46912°, -52.4603°)
Target Field: TOI-799 (J2000 98.46912°, -52.4603°)
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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