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CONFIRMED EXOPLANET · Sub-Neptune

TOI-938 b

Orbits Host Star: TOI-938 · Distance: 701.300 Light-Years (215.034 pc)
Planetary Radius
4.824 R⊕
Planetary Mass
20.800 M⊕
Surface Gravity
0.89 g / g⊕
Equilibrium Temp
1073K (+800°C / +1472°F)
Orbital Period
8.807 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.18 / 1.00
Insolation Flux
220.74 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-938 b is a confirmed sub-neptune exoplanet orbiting the star TOI-938, located approximately 701.3 light-years (215.03 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 0.2016% across the stellar disk), this world measures 4.824 Earth radii (0.43 Jupiter radii) and has a measured mass of 20.8 Earth masses. Combining its mass and radius yields a mean bulk density of 1.02 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.89 g⊕ (8.73 m/s²), and an escape velocity of 23.2 km/s.

In its orbital architecture around TOI-938, TOI-938 b completes one full revolution every 8.807 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1073 K (+800°C / +1472°F) and receiving 220.74 S⊕ (~300,420 W/m²), TOI-938 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-938 is classified as a stellar host with an effective photospheric temperature of 5,829 K, a radius of 0.9851 R☉, a mass of 1.1 M☉, an estimated bolometric luminosity of 1.005 L☉. From Earth, TOI-938 shines at apparent V-band magnitude 11.389 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.18 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-938
Spectral Type Unclassified
Effective Temp (Teff) 5,829 K
Stellar Radius 0.9851 R☉
Stellar Mass 1.1000 M☉
Bolometric Luminosity 1.005 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 11.389 · G: 11.259
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 8.807 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.7833°
Mean Bulk Density 1.02 g/cm³ (23.2 km/s vesc)
Insolation Flux 220.7350 S⊕ (~300,420 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 701.300 LY (215.034 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 04h12m07.76s · DEC: -12d07m07.81s (J2000: 63.03234°, -12.11884°)
Target Field: TOI-938 (J2000 63.03234°, -12.11884°)
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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