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CONFIRMED EXOPLANET · Sub-Neptune

TOI-4640 b

Orbits Host Star: TOI-4640 · Distance: 799.400 Light-Years (245.089 pc)
Planetary Radius
2.843 R⊕
Planetary Mass
8.460 M⊕
Surface Gravity
1.05 g / g⊕
Equilibrium Temp
1379K (+1106°C / +2023°F)
Orbital Period
2.686 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.17 / 1.00
Insolation Flux
854.27 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-4640 b is a confirmed sub-neptune exoplanet orbiting the star TOI-4640, located approximately 799.4 light-years (245.09 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 0.0596% across the stellar disk), this world measures 2.843 Earth radii and has a measured mass of 8.46 Earth masses. Combining its mass and radius yields a mean bulk density of 2.03 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.05 g⊕ (10.3 m/s²), and an escape velocity of 19.3 km/s.

In its orbital architecture around TOI-4640, TOI-4640 b completes one full revolution every 2.686 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1379 K (+1106°C / +2023°F) and receiving 854.27 S⊕ (~1,162,667 W/m²), TOI-4640 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-4640 is classified as a stellar host with an effective photospheric temperature of 5,743 K, a radius of 1.0672 R☉, a mass of 1.1 M☉, an estimated bolometric luminosity of 1.112 L☉. From Earth, TOI-4640 shines at apparent V-band magnitude 11.63 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.17 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-4640
Spectral Type Unclassified
Effective Temp (Teff) 5,743 K
Stellar Radius 1.0672 R☉
Stellar Mass 1.1000 M☉
Bolometric Luminosity 1.112 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 11.630 · G: 11.526
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 2.686 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 87.1739°
Mean Bulk Density 2.03 g/cm³ (19.3 km/s vesc)
Insolation Flux 854.2741 S⊕ (~1,162,667 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 799.400 LY (245.089 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 02h32m49.28s · DEC: +10d04m20.88s (J2000: 38.20532°, 10.07247°)
Target Field: TOI-4640 (J2000 38.20532°, 10.07247°)
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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