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CONFIRMED EXOPLANET · Sub-Neptune

TOI-1814 b

Orbits Host Star: TOI-1814 · Distance: 1182.400 Light-Years (362.522 pc)
Planetary Radius
5.185 R⊕
Planetary Mass
23.500 M⊕
Surface Gravity
0.87 g / g⊕
Equilibrium Temp
978K (+705°C / +1301°F)
Orbital Period
6.369 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.19 / 1.00
Insolation Flux
216.06 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-1814 b is a confirmed sub-neptune exoplanet orbiting the star TOI-1814, located approximately 1182.4 light-years (362.52 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 0.0396% across the stellar disk), this world measures 5.185 Earth radii (0.46 Jupiter radii) and has a measured mass of 23.5 Earth masses. Combining its mass and radius yields a mean bulk density of 0.93 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.87 g⊕ (8.53 m/s²), and an escape velocity of 23.8 km/s.

In its orbital architecture around TOI-1814, TOI-1814 b completes one full revolution every 6.369 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 978 K (+705°C / +1301°F) and receiving 216.06 S⊕ (~294,060 W/m²), TOI-1814 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-1814 is classified as a stellar host with an effective photospheric temperature of 4,873 K, a radius of 2.3895 R☉, an estimated bolometric luminosity of 2.889 L☉. From Earth, TOI-1814 shines at apparent V-band magnitude 11.182 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.19 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-1814
Spectral Type Unclassified
Effective Temp (Teff) 4,873 K
Stellar Radius 2.3895 R☉
Stellar Mass —
Bolometric Luminosity 2.889 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 11.182 · G: 11.414
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 6.369 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 87.4551°
Mean Bulk Density 0.93 g/cm³ (23.8 km/s vesc)
Insolation Flux 216.0619 S⊕ (~294,060 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1182.400 LY (362.522 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 15h47m16.05s · DEC: +77d13m57.51s (J2000: 236.81688°, 77.23264°)
Target Field: TOI-1814 (J2000 236.81688°, 77.23264°)
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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