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CONFIRMED EXOPLANET · Sub-Neptune

TOI-7155 b

Orbits Host Star: TOI-7155 · Distance: 472.100 Light-Years (144.751 pc)
Planetary Radius
2.408 R⊕
Planetary Mass
6.380 M⊕
Surface Gravity
1.1 g / g⊕
Equilibrium Temp
914K (+641°C / +1186°F)
Orbital Period
3.895 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.28 / 1.00
Insolation Flux
116.25 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-7155 b is a confirmed sub-neptune exoplanet orbiting the star TOI-7155, located approximately 472.1 light-years (144.75 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 0.1083% across the stellar disk), this world measures 2.408 Earth radii and has a measured mass of 6.38 Earth masses. Combining its mass and radius yields a mean bulk density of 2.52 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-7155, TOI-7155 b completes one full revolution every 3.895 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 914 K (+641°C / +1186°F) and receiving 116.25 S⊕ (~158,220 W/m²), TOI-7155 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-7155 is classified as a stellar host with an effective photospheric temperature of 4,673 K, a radius of 0.6707 R☉, a mass of 0.755 M☉, an estimated bolometric luminosity of 0.192 L☉. From Earth, TOI-7155 shines at apparent V-band magnitude 12.758 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.28 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-7155
Spectral Type Unclassified
Effective Temp (Teff) 4,673 K
Stellar Radius 0.6707 R☉
Stellar Mass 0.7550 M☉
Bolometric Luminosity 0.192 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 12.758 · G: 12.484
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 3.895 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 86.8712°
Mean Bulk Density 2.52 g/cm³ (18.2 km/s vesc)
Insolation Flux 116.2530 S⊕ (~158,220 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 472.100 LY (144.751 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 00h49m46.91s · DEC: +79d17m16.28s (J2000: 12.44545°, 79.28786°)
Target Field: TOI-7155 (J2000 12.44545°, 79.28786°)
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)
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