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CONFIRMED EXOPLANET · Sub-Neptune

TOI-2453 b

Orbits Host Star: TOI-2453 · Distance: 267.100 Light-Years (81.904 pc)
Planetary Radius
3.244 R⊕
Planetary Mass
10.600 M⊕
Surface Gravity
1.01 g / g⊕
Equilibrium Temp
551K (+278°C / +532°F)
Orbital Period
4.441 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.41 / 1.00
Insolation Flux
21.75 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-2453 b is a confirmed sub-neptune exoplanet orbiting the star TOI-2453, located approximately 267.1 light-years (81.9 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 0.3503% across the stellar disk), this world measures 3.244 Earth radii (0.29 Jupiter radii) and has a measured mass of 10.6 Earth masses. Combining its mass and radius yields a mean bulk density of 1.71 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 1.01 g⊕ (9.9 m/s²), and an escape velocity of 20.2 km/s.

In its orbital architecture around TOI-2453, TOI-2453 b completes one full revolution every 4.441 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 551 K (+278°C / +532°F) and receiving 21.75 S⊕ (~29,600 W/m²), TOI-2453 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-2453 is classified as a stellar host with an effective photospheric temperature of 3,720 K, a radius of 0.5025 R☉, a mass of 0.5005 M☉, an estimated bolometric luminosity of 0.043 L☉. From Earth, TOI-2453 shines at apparent V-band magnitude 14.415 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.41 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-2453
Spectral Type Unclassified
Effective Temp (Teff) 3,720 K
Stellar Radius 0.5025 R☉
Stellar Mass 0.5005 M☉
Bolometric Luminosity 0.043 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 14.415 · G: 13.510
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 4.441 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 87.9509°
Mean Bulk Density 1.71 g/cm³ (20.2 km/s vesc)
Insolation Flux 21.7490 S⊕ (~29,600 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 267.100 LY (81.904 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 04h59m21.00s · DEC: +12d56m10.87s (J2000: 74.83748°, 12.93635°)
Target Field: TOI-2453 (J2000 74.83748°, 12.93635°)
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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