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CONFIRMED EXOPLANET · Sub-Neptune

TOI-4662 b

Orbits Host Star: TOI-4662 · Distance: 362.200 Light-Years (111.047 pc)
Planetary Radius
2.880 R⊕
Planetary Mass
8.650 M⊕
Surface Gravity
1.04 g / g⊕
Equilibrium Temp
741K (+468°C / +874°F)
Orbital Period
4.703 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.32 / 1.00
Insolation Flux
50.10 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-4662 b is a confirmed sub-neptune exoplanet orbiting the star TOI-4662, located approximately 362.2 light-years (111.05 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 0.1448% across the stellar disk), this world measures 2.88 Earth radii and has a measured mass of 8.65 Earth masses. Combining its mass and radius yields a mean bulk density of 2 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.04 g⊕ (10.2 m/s²), and an escape velocity of 19.4 km/s.

In its orbital architecture around TOI-4662, TOI-4662 b completes one full revolution every 4.703 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 741 K (+468°C / +874°F) and receiving 50.10 S⊕ (~68,192 W/m²), TOI-4662 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-4662 is classified as a stellar host with an effective photospheric temperature of 4,520 K, a radius of 0.6938 R☉, a mass of 0.703 M☉, an estimated bolometric luminosity of 0.18 L☉. From Earth, TOI-4662 shines at apparent V-band magnitude 12.437 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.32 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-4662
Spectral Type Unclassified
Effective Temp (Teff) 4,520 K
Stellar Radius 0.6938 R☉
Stellar Mass 0.7030 M☉
Bolometric Luminosity 0.18 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 12.437 · G: 12.098
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 4.703 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 87.4650°
Mean Bulk Density 2 g/cm³ (19.4 km/s vesc)
Insolation Flux 50.1040 S⊕ (~68,192 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 362.200 LY (111.047 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 03h50m03.85s · DEC: -31d05m38.49s (J2000: 57.51603°, -31.09402°)
Target Field: TOI-4662 (J2000 57.51603°, -31.09402°)
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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