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CONFIRMED EXOPLANET · Sub-Neptune

TOI-1768.01

Orbits Host Star: TOI-1768 · Distance: 514.000 Light-Years (157.597 pc)
Planetary Radius
3.453 R⊕
Planetary Mass
11.800 M⊕
Surface Gravity
0.99 g / g⊕
Equilibrium Temp
1566K (+1293°C / +2359°F)
Orbital Period
7.338 days
Discovery Year
2024 (Transit)
Earth Similarity (ESI)
0.13 / 1.00
Insolation Flux
240.87 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-1768.01 is a confirmed sub-neptune exoplanet orbiting the star TOI-1768, located approximately 514 light-years (157.6 parsecs) from the Solar System. First announced in 2024 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.0828% across the stellar disk), this world measures 3.453 Earth radii (0.31 Jupiter radii) and has a measured mass of 11.8 Earth masses. Combining its mass and radius yields a mean bulk density of 1.58 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.99 g⊕ (9.71 m/s²), and an escape velocity of 20.7 km/s.

In its orbital architecture around TOI-1768, TOI-1768.01 completes one full revolution every 7.338 Earth days at a semi-major axis of 0.076381 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 113.2 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1566 K (+1293°C / +2359°F) and receiving 240.87 S⊕ (~327,824 W/m²), TOI-1768.01 orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-1768 is classified as a stellar host with an effective photospheric temperature of 5,994 K, a radius of 1.1 R☉, a mass of 1.1 M☉, an estimated bolometric luminosity of 1.401 L☉. From Earth, TOI-1768 shines at apparent V-band magnitude 10.419 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.13 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-1768
Spectral Type Unclassified
Effective Temp (Teff) 5,994 K
Stellar Radius 1.1000 R☉
Stellar Mass 1.1000 M☉
Bolometric Luminosity 1.401 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 10.419 · G: 10.311
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.076381 AU
Orbital Period 7.338 days
Mean Orbital Velocity 113.2 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 1.58 g/cm³ (20.7 km/s vesc)
Insolation Flux 240.8700 S⊕ (~327,824 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 514.000 LY (157.597 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 10h08m24.67s · DEC: +55d32m23.86s (J2000: 152.10278°, 55.53996°)
Target Field: TOI-1768 (J2000 152.10278°, 55.53996°)
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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