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CONFIRMED EXOPLANET · Terrestrial

TOI-6324 b

Orbits Host Star: TOI-6324 · Distance: 67.000 Light-Years (20.549 pc)
Planetary Radius
1.059 R⊕
Planetary Mass
1.170 M⊕
Surface Gravity
1.04 g / g⊕
Equilibrium Temp
1216K (+943°C / +1729°F)
Orbital Period
0.279 days
Discovery Year
2025 (Transit)
Earth Similarity (ESI)
0.26 / 1.00
Insolation Flux
284.21 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-6324 b is a confirmed terrestrial exoplanet orbiting the star TOI-6324, located approximately 67 light-years (20.55 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 0.1098% across the stellar disk), this world measures 1.059 Earth radii and has a measured mass of 1.17 Earth masses. Combining its mass and radius yields a mean bulk density of 5.43 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 1.04 g⊕ (10.2 m/s²), and an escape velocity of 11.8 km/s.

In its orbital architecture around TOI-6324, TOI-6324 b completes one full revolution every 0.279 Earth days. The orbit is modeled as circular (e = 0.00), maintaining a constant stellar distance throughout its year.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1216 K (+943°C / +1729°F) and receiving 284.21 S⊕ (~386,811 W/m²), TOI-6324 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-6324 is classified as a stellar host with an effective photospheric temperature of 3,247 K, a radius of 0.293 R☉, a mass of 0.269 M☉, an estimated bolometric luminosity of 0.00856 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.32 dex (metal-poor relative to the Sun). From Earth, TOI-6324 shines at apparent V-band magnitude 13.386 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.26 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-6324
Spectral Type Unclassified
Effective Temp (Teff) 3,247 K
Stellar Radius 0.2930 R☉
Stellar Mass 0.2690 M☉
Bolometric Luminosity 0.00856 L☉
Metallicity [Fe/H] -0.320 dex
Stellar Age —
Apparent Magnitude V: 13.386 · G: 12.214
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 0.279 days
Orbital Eccentricity (e) 0.00000
Orbital Inclination (i) 74.6000°
Mean Bulk Density 5.43 g/cm³ (11.8 km/s vesc)
Insolation Flux 284.2110 S⊕ (~386,811 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 67.000 LY (20.549 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 22h03m22.69s · DEC: +67d29m55.24s (J2000: 330.84454°, 67.49868°)
Target Field: TOI-6324 (J2000 330.84454°, 67.49868°)
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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