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CONFIRMED EXOPLANET · Super-Earth

TOI-512 b

Orbits Host Star: TOI-512 · Distance: 219.800 Light-Years (67.398 pc)
Planetary Radius
1.540 R⊕
Planetary Mass
3.570 M⊕
Surface Gravity
1.51 g / g⊕
Equilibrium Temp
1009K (+736°C / +1357°F)
Orbital Period
7.189 days
Discovery Year
2025 (Transit)
Earth Similarity (ESI)
0.30 / 1.00
Insolation Flux
127.00 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-512 b is a confirmed super-earth exoplanet orbiting the star TOI-512, located approximately 219.8 light-years (67.4 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 0.0252% across the stellar disk), this world measures 1.54 Earth radii and has a measured mass of 3.57 Earth masses. Combining its mass and radius yields a mean bulk density of 5.39 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.51 g⊕ (14.81 m/s²), and an escape velocity of 17 km/s.

In its orbital architecture around TOI-512, TOI-512 b completes one full revolution every 7.189 Earth days. With a near-circular eccentricity of e = 0.02, the planet experiences minimal orbital distance variation.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1009 K (+736°C / +1357°F) and receiving 127.00 S⊕ (~172,847 W/m²), TOI-512 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-512 is classified as a stellar host with an effective photospheric temperature of 5,277 K, a radius of 0.89 R☉, a mass of 0.74 M☉, an estimated bolometric luminosity of 0.551 L☉. Stellar evolution modeling indicates an estimated stellar age of 8.235 Gyr and a metallicity of [Fe/H] = -0.11 dex (metal-poor relative to the Sun). From Earth, TOI-512 shines at apparent V-band magnitude 9.735 (accessible to binoculars and small amateur telescopes) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.30 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-512
Spectral Type Unclassified
Effective Temp (Teff) 5,277 K
Stellar Radius 0.8900 R☉
Stellar Mass 0.7400 M☉
Bolometric Luminosity 0.551 L☉
Metallicity [Fe/H] -0.110 dex
Stellar Age 8.235 Gyr
Apparent Magnitude V: 9.735 · G: 9.480
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 7.189 days
Orbital Eccentricity (e) 0.02000
Orbital Inclination (i) 88.9200°
Mean Bulk Density 5.39 g/cm³ (17 km/s vesc)
Insolation Flux 127.0000 S⊕ (~172,847 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 219.800 LY (67.398 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 06h26m35.21s · DEC: -38d36m25.95s (J2000: 96.6467°, -38.60721°)
Target Field: TOI-512 (J2000 96.6467°, -38.60721°)
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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