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CONFIRMED EXOPLANET · Super-Earth

TOI-5728 b

Orbits Host Star: TOI-5728 · Distance: 178.400 Light-Years (54.705 pc)
Planetary Radius
1.310 R⊕
Planetary Mass
2.270 M⊕
Surface Gravity
1.32 g / g⊕
Equilibrium Temp
382K (+109°C / +228°F)
Orbital Period
11.498 days
Discovery Year
2025 (Transit)
Earth Similarity (ESI)
0.77 / 1.00 Moderate
Insolation Flux
3.51 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-5728 b is a confirmed super-earth exoplanet orbiting the star TOI-5728, located approximately 178.4 light-years (54.71 parsecs) from the Solar System. First announced in 2025 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.1054% across the stellar disk), this world measures 1.31 Earth radii and has a measured mass of 2.27 Earth masses. Combining its mass and radius yields a mean bulk density of 5.57 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.32 g⊕ (12.94 m/s²), and an escape velocity of 14.7 km/s.

In its orbital architecture around TOI-5728, TOI-5728 b completes one full revolution every 11.498 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 382 K (+109°C / +228°F) and receiving 3.51 S⊕ (~4,780 W/m²), TOI-5728 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-5728 is classified as a stellar host with an effective photospheric temperature of 3,419 K, a radius of 0.37 R☉, a mass of 0.36 M☉, an estimated bolometric luminosity of 0.017 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.12 dex (metal-poor relative to the Sun). From Earth, TOI-5728 shines at apparent V-band magnitude 15.02 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.77 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-5728
Spectral Type Unclassified
Effective Temp (Teff) 3,419 K
Stellar Radius 0.3700 R☉
Stellar Mass 0.3600 M☉
Bolometric Luminosity 0.017 L☉
Metallicity [Fe/H] -0.120 dex
Stellar Age —
Apparent Magnitude V: 15.020 · G: 13.685
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 11.498 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 89.8300°
Mean Bulk Density 5.57 g/cm³ (14.7 km/s vesc)
Insolation Flux 3.5120 S⊕ (~4,780 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 178.400 LY (54.705 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 17h21m24.22s · DEC: +67d33m01.52s (J2000: 260.35094°, 67.55042°)
Target Field: TOI-5728 (J2000 260.35094°, 67.55042°)
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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