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CONFIRMED EXOPLANET · Super-Earth

TOI-4529 b

Orbits Host Star: TOI-4529 (Type M1.5 V) · Distance: 92.600 Light-Years (28.384 pc)
Planetary Radius
1.770 R⊕
Planetary Mass
4.900 M⊕
Surface Gravity
1.56 g / g⊕
Equilibrium Temp
511K (+238°C / +460°F)
Orbital Period
5.88 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.57 / 1.00
Insolation Flux
14.61 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-4529 b is a confirmed super-earth exoplanet orbiting the star TOI-4529, located approximately 92.6 light-years (28.38 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 0.1143% across the stellar disk), this world measures 1.77 Earth radii and has a measured mass of 4.9 Earth masses. Combining its mass and radius yields a mean bulk density of 4.87 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.56 g⊕ (15.3 m/s²), and an escape velocity of 18.6 km/s.

In its orbital architecture around TOI-4529, TOI-4529 b completes one full revolution every 5.88 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 511 K (+238°C / +460°F) and receiving 14.61 S⊕ (~19,883 W/m²), TOI-4529 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-4529 is classified as a low-mass red dwarf of spectral type M1.5 V with an effective photospheric temperature of 3,697 K, a radius of 0.48 R☉, a mass of 0.482 M☉, an estimated bolometric luminosity of 0.039 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.24 dex (metal-poor relative to the Sun). From Earth, TOI-4529 shines at apparent V-band magnitude 12.214 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.57 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-4529
Spectral Type M1.5 V
Effective Temp (Teff) 3,697 K
Stellar Radius 0.4800 R☉
Stellar Mass 0.4820 M☉
Bolometric Luminosity 0.039 L☉
Metallicity [Fe/H] -0.240 dex
Stellar Age —
Apparent Magnitude V: 12.214 · G: 11.216
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 5.88 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.7000°
Mean Bulk Density 4.87 g/cm³ (18.6 km/s vesc)
Insolation Flux 14.6089 S⊕ (~19,883 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 92.600 LY (28.384 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 01h07m52.52s · DEC: +12d52m51.44s (J2000: 16.96885°, 12.88095°)
Target Field: TOI-4529 (J2000 16.96885°, 12.88095°)
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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