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CONFIRMED EXOPLANET · Sub-Neptune

TOI-4638.01

Orbits Host Star: TOI-4638 · Distance: 548.800 Light-Years (168.248 pc)
Planetary Radius
2.933 R⊕
Planetary Mass
8.920 M⊕
Surface Gravity
1.04 g / g⊕
Equilibrium Temp
780K (+507°C / +945°F)
Orbital Period
10.284 days
Discovery Year
2024 (Transit)
Earth Similarity (ESI)
0.31 / 1.00
Insolation Flux
87.81 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-4638.01 is a confirmed sub-neptune exoplanet orbiting the star TOI-4638, located approximately 548.8 light-years (168.25 parsecs) from the Solar System. First announced in 2024 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.0903% across the stellar disk), this world measures 2.933 Earth radii and has a measured mass of 8.92 Earth masses. Combining its mass and radius yields a mean bulk density of 1.95 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 1.04 g⊕ (10.2 m/s²), and an escape velocity of 19.5 km/s.

In its orbital architecture around TOI-4638, TOI-4638.01 completes one full revolution every 10.284 Earth days at a semi-major axis of 0.093013 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 98.4 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 780 K (+507°C / +945°F) and receiving 87.81 S⊕ (~119,509 W/m²), TOI-4638.01 orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-4638 is classified as a stellar host with an effective photospheric temperature of 5,700 K, a radius of 0.895 R☉, a mass of 1.02 M☉, an estimated bolometric luminosity of 0.759 L☉. From Earth, TOI-4638 shines at apparent V-band magnitude 11.657 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.31 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-4638
Spectral Type Unclassified
Effective Temp (Teff) 5,700 K
Stellar Radius 0.8950 R☉
Stellar Mass 1.0200 M☉
Bolometric Luminosity 0.759 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 11.657 · G: 11.210
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.093013 AU
Orbital Period 10.284 days
Mean Orbital Velocity 98.4 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 1.95 g/cm³ (19.5 km/s vesc)
Insolation Flux 87.8100 S⊕ (~119,509 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 548.800 LY (168.248 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 00h51m16.96s · DEC: +12d47m16.75s (J2000: 12.82066°, 12.78799°)
Target Field: TOI-4638 (J2000 12.82066°, 12.78799°)
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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