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CONFIRMED EXOPLANET · Terrestrial

TOI-5716 b

Orbits Host Star: TOI-5716 · Distance: 128.500 Light-Years (39.412 pc)
Planetary Radius
0.960 R⊕
Planetary Mass
0.840 M⊕
Surface Gravity
0.91 g / g⊕
Equilibrium Temp
400K (+127°C / +261°F)
Orbital Period
6.766 days
Discovery Year
2025 (Transit)
Earth Similarity (ESI)
0.77 / 1.00 Moderate
Insolation Flux
3.41 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-5716 b is a confirmed terrestrial exoplanet orbiting the star TOI-5716, located approximately 128.5 light-years (39.41 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 0.16% across the stellar disk), this world measures 0.96 Earth radii and has a measured mass of 0.84 Earth masses. Combining its mass and radius yields a mean bulk density of 5.24 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 0.91 g⊕ (8.92 m/s²), and an escape velocity of 10.5 km/s.

In its orbital architecture around TOI-5716, TOI-5716 b completes one full revolution every 6.766 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 400 K (+127°C / +261°F) and receiving 3.41 S⊕ (~4,640 W/m²), TOI-5716 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-5716 is classified as a stellar host with an effective photospheric temperature of 3,436 K, a radius of 0.22 R☉, a mass of 0.19 M☉, an estimated bolometric luminosity of 0.00605 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.54 dex (metal-poor relative to the Sun). From Earth, TOI-5716 shines at apparent V-band magnitude 15.83 (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-5716
Spectral Type Unclassified
Effective Temp (Teff) 3,436 K
Stellar Radius 0.2200 R☉
Stellar Mass 0.1900 M☉
Bolometric Luminosity 0.00605 L☉
Metallicity [Fe/H] -0.540 dex
Stellar Age —
Apparent Magnitude V: 15.830 · G: 14.374
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 6.766 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 89.4000°
Mean Bulk Density 5.24 g/cm³ (10.5 km/s vesc)
Insolation Flux 3.4093 S⊕ (~4,640 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 128.500 LY (39.412 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 13h27m36.19s · DEC: +73d10m38.76s (J2000: 201.9008°, 73.17743°)
Target Field: TOI-5716 (J2000 201.9008°, 73.17743°)
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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