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CONFIRMED EXOPLANET · Sub-Neptune

TOI-4747 b

Orbits Host Star: TOI-4747 · Distance: 993.500 Light-Years (304.615 pc)
Planetary Radius
3.958 R⊕
Planetary Mass
14.800 M⊕
Surface Gravity
0.94 g / g⊕
Equilibrium Temp
1035K (+762°C / +1404°F)
Orbital Period
5.219 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.20 / 1.00
Insolation Flux
190.80 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-4747 b is a confirmed sub-neptune exoplanet orbiting the star TOI-4747, located approximately 993.5 light-years (304.62 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 0.1347% across the stellar disk), this world measures 3.958 Earth radii (0.35 Jupiter radii) and has a measured mass of 14.8 Earth masses. Combining its mass and radius yields a mean bulk density of 1.32 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.94 g⊕ (9.22 m/s²), and an escape velocity of 21.6 km/s.

In its orbital architecture around TOI-4747, TOI-4747 b completes one full revolution every 5.219 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1035 K (+762°C / +1404°F) and receiving 190.80 S⊕ (~259,672 W/m²), TOI-4747 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-4747 is classified as a stellar host with an effective photospheric temperature of 5,595 K, a radius of 0.9888 R☉, a mass of 1.01 M☉, an estimated bolometric luminosity of 0.86 L☉. From Earth, TOI-4747 shines at apparent V-band magnitude 12.442 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.20 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-4747
Spectral Type Unclassified
Effective Temp (Teff) 5,595 K
Stellar Radius 0.9888 R☉
Stellar Mass 1.0100 M☉
Bolometric Luminosity 0.86 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 12.442 · G: 12.278
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 5.219 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.4203°
Mean Bulk Density 1.32 g/cm³ (21.6 km/s vesc)
Insolation Flux 190.7950 S⊕ (~259,672 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 993.500 LY (304.615 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 05h45m42.64s · DEC: -45d01m45.22s (J2000: 86.42767°, -45.02923°)
Target Field: TOI-4747 (J2000 86.42767°, -45.02923°)
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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