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CONFIRMED EXOPLANET · Sub-Neptune

TOI-128.01

Orbits Host Star: TOI-128 · Distance: 223.300 Light-Years (68.473 pc)
Planetary Radius
2.219 R⊕
Planetary Mass
5.560 M⊕
Surface Gravity
1.13 g / g⊕
Equilibrium Temp
1345K (+1072°C / +1962°F)
Orbital Period
4.94 days
Discovery Year
2024 (Transit)
Earth Similarity (ESI)
0.19 / 1.00
Insolation Flux
182.41 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-128.01 is a confirmed sub-neptune exoplanet orbiting the star TOI-128, located approximately 223.3 light-years (68.47 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 0.0324% across the stellar disk), this world measures 2.219 Earth radii and has a measured mass of 5.56 Earth masses. Combining its mass and radius yields a mean bulk density of 2.81 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.13 g⊕ (11.08 m/s²), and an escape velocity of 17.7 km/s.

In its orbital architecture around TOI-128, TOI-128.01 completes one full revolution every 4.94 Earth days at a semi-major axis of 0.05381 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 118.5 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1345 K (+1072°C / +1962°F) and receiving 182.41 S⊕ (~248,255 W/m²), TOI-128.01 orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-128 is classified as a stellar host with an effective photospheric temperature of 6,086 K, a radius of 1.13 R☉, a mass of 0.852 M☉, an estimated bolometric luminosity of 1.572 L☉. From Earth, TOI-128 shines at apparent V-band magnitude 8.44 (accessible to binoculars and small amateur telescopes) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.19 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-128
Spectral Type Unclassified
Effective Temp (Teff) 6,086 K
Stellar Radius 1.1300 R☉
Stellar Mass 0.8520 M☉
Bolometric Luminosity 1.572 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 8.440 · G: 8.372
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.053810 AU
Orbital Period 4.94 days
Mean Orbital Velocity 118.5 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 2.81 g/cm³ (17.7 km/s vesc)
Insolation Flux 182.4060 S⊕ (~248,255 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 223.300 LY (68.473 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 05h18m05.03s · DEC: -80d57m51.78s (J2000: 79.52094°, -80.96438°)
Target Field: TOI-128 (J2000 79.52094°, -80.96438°)
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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