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CONFIRMED EXOPLANET · Sub-Neptune

TOI-2518 b

Orbits Host Star: TOI-2518 · Distance: 524.500 Light-Years (160.825 pc)
Planetary Radius
2.268 R⊕
Planetary Mass
5.770 M⊕
Surface Gravity
1.12 g / g⊕
Equilibrium Temp
1095K (+822°C / +1512°F)
Orbital Period
6.898 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.24 / 1.00
Insolation Flux
239.13 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-2518 b is a confirmed sub-neptune exoplanet orbiting the star TOI-2518, located approximately 524.5 light-years (160.83 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 0.0438% across the stellar disk), this world measures 2.268 Earth radii and has a measured mass of 5.77 Earth masses. Combining its mass and radius yields a mean bulk density of 2.73 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.12 g⊕ (10.98 m/s²), and an escape velocity of 17.8 km/s.

In its orbital architecture around TOI-2518, TOI-2518 b completes one full revolution every 6.898 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1095 K (+822°C / +1512°F) and receiving 239.13 S⊕ (~325,460 W/m²), TOI-2518 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-2518 is classified as a stellar host with an effective photospheric temperature of 5,751 K, a radius of 0.9934 R☉, a mass of 1.11 M☉, an estimated bolometric luminosity of 0.969 L☉. From Earth, TOI-2518 shines at apparent V-band magnitude 10.954 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.24 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-2518
Spectral Type Unclassified
Effective Temp (Teff) 5,751 K
Stellar Radius 0.9934 R☉
Stellar Mass 1.1100 M☉
Bolometric Luminosity 0.969 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 10.954 · G: 10.650
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 6.898 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 87.9575°
Mean Bulk Density 2.73 g/cm³ (17.8 km/s vesc)
Insolation Flux 239.1330 S⊕ (~325,460 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 524.500 LY (160.825 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 07h01m46.76s · DEC: -34d55m10.87s (J2000: 105.44485°, -34.91969°)
Target Field: TOI-2518 (J2000 105.44485°, -34.91969°)
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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