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CONFIRMED EXOPLANET · Sub-Neptune

TOI-1346 b

Orbits Host Star: TOI-1346 · Distance: 376.500 Light-Years (115.450 pc)
Planetary Radius
2.390 R⊕
Planetary Mass
6.300 M⊕
Surface Gravity
1.1 g / g⊕
Equilibrium Temp
1324K (+1051°C / +1924°F)
Orbital Period
1.762 days
Discovery Year
2025 (Transit)
Earth Similarity (ESI)
0.19 / 1.00
Insolation Flux
468.54 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-1346 b is a confirmed sub-neptune exoplanet orbiting the star TOI-1346, located approximately 376.5 light-years (115.45 parsecs) from the Solar System. First announced in 2025 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.0789% across the stellar disk), this world measures 2.39 Earth radii and has a measured mass of 6.3 Earth masses. Combining its mass and radius yields a mean bulk density of 2.54 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.1 g⊕ (10.79 m/s²), and an escape velocity of 18.2 km/s.

In its orbital architecture around TOI-1346, TOI-1346 b completes one full revolution every 1.762 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1324 K (+1051°C / +1924°F) and receiving 468.54 S⊕ (~637,685 W/m²), TOI-1346 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-1346 is classified as a stellar host with an effective photospheric temperature of 5,099 K, a radius of 0.78 R☉, a mass of 0.82 M☉, an estimated bolometric luminosity of 0.369 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.01 dex (near-solar heavy-element abundance). From Earth, TOI-1346 shines at apparent V-band magnitude 11.693 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The TOI-1346 system is a multi-planet architecture hosting 2 confirmed worlds, with TOI-1346 b sharing its stellar neighborhood alongside TOI-1346 c.

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-1346
Spectral Type Unclassified
Effective Temp (Teff) 5,099 K
Stellar Radius 0.7800 R☉
Stellar Mass 0.8200 M☉
Bolometric Luminosity 0.369 L☉
Metallicity [Fe/H] -0.010 dex
Stellar Age —
Apparent Magnitude V: 11.693 · G: 11.304
System Architecture 1 Star, 2 Planets

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 1.762 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 82.8300°
Mean Bulk Density 2.54 g/cm³ (18.2 km/s vesc)
Insolation Flux 468.5415 S⊕ (~637,685 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 376.500 LY (115.450 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 17h06m29.44s · DEC: +68d50m35.89s (J2000: 256.62268°, 68.8433°)
Target Field: TOI-1346 (J2000 256.62268°, 68.8433°)
Surveys available: Digitized Sky Survey (DSS2 Optical), 2MASS (Near-Infrared), AllWISE (Mid-Infrared) · Field of View: 0.18° (10.8 arcmin)
Aladin Lite v3 · Centre de Données astronomiques de Strasbourg (CDS)
SIMBAD Astronomical Query ↗ NASA ADS Research Papers ↗

Other Worlds in the TOI-1346 System (1)

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