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CONFIRMED EXOPLANET · Sub-Neptune

TOI-5532 b

Orbits Host Star: TOI-5532 · Distance: 296.800 Light-Years (90.999 pc)
Planetary Radius
2.528 R⊕
Planetary Mass
6.930 M⊕
Surface Gravity
1.08 g / g⊕
Equilibrium Temp
617K (+344°C / +651°F)
Orbital Period
5.654 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.41 / 1.00
Insolation Flux
34.32 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-5532 b is a confirmed sub-neptune exoplanet orbiting the star TOI-5532, located approximately 296.8 light-years (91 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 0.1225% across the stellar disk), this world measures 2.528 Earth radii and has a measured mass of 6.93 Earth masses. Combining its mass and radius yields a mean bulk density of 2.37 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.08 g⊕ (10.59 m/s²), and an escape velocity of 18.5 km/s.

In its orbital architecture around TOI-5532, TOI-5532 b completes one full revolution every 5.654 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 617 K (+344°C / +651°F) and receiving 34.32 S⊕ (~46,713 W/m²), TOI-5532 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-5532 is classified as a stellar host with an effective photospheric temperature of 4,208 K, a radius of 0.6621 R☉, a mass of 0.6361 M☉, an estimated bolometric luminosity of 0.123 L☉. From Earth, TOI-5532 shines at apparent V-band magnitude 13.072 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.41 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-5532
Spectral Type Unclassified
Effective Temp (Teff) 4,208 K
Stellar Radius 0.6621 R☉
Stellar Mass 0.6361 M☉
Bolometric Luminosity 0.123 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 13.072 · G: 12.435
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 5.654 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 85.1576°
Mean Bulk Density 2.37 g/cm³ (18.5 km/s vesc)
Insolation Flux 34.3229 S⊕ (~46,713 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 296.800 LY (90.999 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 02h45m31.30s · DEC: +05d09m02.64s (J2000: 41.3804°, 5.15073°)
Target Field: TOI-5532 (J2000 41.3804°, 5.15073°)
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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