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CONFIRMED EXOPLANET · Super-Earth

TOI-4363 b

Orbits Host Star: TOI-4363 · Distance: 253.700 Light-Years (77.775 pc)
Planetary Radius
1.767 R⊕
Planetary Mass
3.770 M⊕
Surface Gravity
1.21 g / g⊕
Equilibrium Temp
885K (+612°C / +1134°F)
Orbital Period
2.119 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.32 / 1.00
Insolation Flux
144.79 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-4363 b is a confirmed super-earth exoplanet orbiting the star TOI-4363, located approximately 253.7 light-years (77.78 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 0.0549% across the stellar disk), this world measures 1.767 Earth radii and has a measured mass of 3.77 Earth masses. Combining its mass and radius yields a mean bulk density of 3.77 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.21 g⊕ (11.87 m/s²), and an escape velocity of 16.3 km/s.

In its orbital architecture around TOI-4363, TOI-4363 b completes one full revolution every 2.119 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 885 K (+612°C / +1134°F) and receiving 144.79 S⊕ (~197,053 W/m²), TOI-4363 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-4363 is classified as a stellar host with an effective photospheric temperature of 4,278 K, a radius of 0.6913 R☉, a mass of 0.62 M☉, an estimated bolometric luminosity of 0.144 L☉. From Earth, TOI-4363 shines at apparent V-band magnitude 12.678 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.32 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-4363
Spectral Type Unclassified
Effective Temp (Teff) 4,278 K
Stellar Radius 0.6913 R☉
Stellar Mass 0.6200 M☉
Bolometric Luminosity 0.144 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 12.678 · G: 12.083
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 2.119 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 86.4349°
Mean Bulk Density 3.77 g/cm³ (16.3 km/s vesc)
Insolation Flux 144.7854 S⊕ (~197,053 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 253.700 LY (77.775 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 02h28m26.53s · DEC: -12d32m57.71s (J2000: 37.11056°, -12.54936°)
Target Field: TOI-4363 (J2000 37.11056°, -12.54936°)
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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