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CONFIRMED EXOPLANET · Sub-Neptune

TOI-205 b

Orbits Host Star: TOI-205 · Distance: 579.800 Light-Years (177.759 pc)
Planetary Radius
2.501 R⊕
Planetary Mass
6.810 M⊕
Surface Gravity
1.09 g / g⊕
Equilibrium Temp
1800K (+1527°C / +2781°F)
Orbital Period
4.253 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.13 / 1.00
Insolation Flux
1,740.92 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-205 b is a confirmed sub-neptune exoplanet orbiting the star TOI-205, located approximately 579.8 light-years (177.76 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 0.0249% across the stellar disk), this world measures 2.501 Earth radii and has a measured mass of 6.81 Earth masses. Combining its mass and radius yields a mean bulk density of 2.4 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.09 g⊕ (10.69 m/s²), and an escape velocity of 18.5 km/s.

In its orbital architecture around TOI-205, TOI-205 b completes one full revolution every 4.253 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1800 K (+1527°C / +2781°F) and receiving 1,740.92 S⊕ (~2,369,395 W/m²), TOI-205 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-205 is classified as a stellar host with an effective photospheric temperature of 6,303 K, a radius of 1.4538 R☉, a mass of 1.2 M☉, an estimated bolometric luminosity of 2.993 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = 0.13 dex (metal-rich relative to the Sun). From Earth, TOI-205 shines at apparent V-band magnitude 9.921 (accessible to binoculars and small amateur telescopes) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.13 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-205
Spectral Type Unclassified
Effective Temp (Teff) 6,303 K
Stellar Radius 1.4538 R☉
Stellar Mass 1.2000 M☉
Bolometric Luminosity 2.993 L☉
Metallicity [Fe/H] 0.130 dex
Stellar Age —
Apparent Magnitude V: 9.921 · G: 9.794
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 4.253 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 86.6259°
Mean Bulk Density 2.4 g/cm³ (18.5 km/s vesc)
Insolation Flux 1740.9224 S⊕ (~2,369,395 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 579.800 LY (177.759 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 00h31m54.11s · DEC: -56d57m54.29s (J2000: 7.97546°, -56.96508°)
Target Field: TOI-205 (J2000 7.97546°, -56.96508°)
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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