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CONFIRMED EXOPLANET · Sub-Neptune

TOI-5502 b

Orbits Host Star: TOI-5502 · Distance: 811.000 Light-Years (248.654 pc)
Planetary Radius
4.129 R⊕
Planetary Mass
15.900 M⊕
Surface Gravity
0.93 g / g⊕
Equilibrium Temp
870K (+597°C / +1107°F)
Orbital Period
11.626 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.24 / 1.00
Insolation Flux
95.20 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-5502 b is a confirmed sub-neptune exoplanet orbiting the star TOI-5502, located approximately 811 light-years (248.65 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 0.0818% across the stellar disk), this world measures 4.129 Earth radii (0.37 Jupiter radii) and has a measured mass of 15.9 Earth masses. Combining its mass and radius yields a mean bulk density of 1.25 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.93 g⊕ (9.12 m/s²), and an escape velocity of 22 km/s.

In its orbital architecture around TOI-5502, TOI-5502 b completes one full revolution every 11.626 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 870 K (+597°C / +1107°F) and receiving 95.20 S⊕ (~129,561 W/m²), TOI-5502 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-5502 is classified as a stellar host with an effective photospheric temperature of 6,089 K, a radius of 1.3238 R☉, a mass of 1.244 M☉, an estimated bolometric luminosity of 2.161 L☉. From Earth, TOI-5502 shines at apparent V-band magnitude 10.881 (faint and requiring research-grade or CCD telescopic photometry) in the Northern 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-5502
Spectral Type Unclassified
Effective Temp (Teff) 6,089 K
Stellar Radius 1.3238 R☉
Stellar Mass 1.2440 M☉
Bolometric Luminosity 2.161 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 10.881 · G: 10.704
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 11.626 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.9351°
Mean Bulk Density 1.25 g/cm³ (22 km/s vesc)
Insolation Flux 95.1955 S⊕ (~129,561 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 811.000 LY (248.654 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 09h00m48.97s · DEC: +27d59m54.00s (J2000: 135.20406°, 27.99833°)
Target Field: TOI-5502 (J2000 135.20406°, 27.99833°)
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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