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CONFIRMED EXOPLANET · Sub-Neptune

TIC 139702105 b

Orbits Host Star: TIC 139702105 · Distance: 299.400 Light-Years (91.788 pc)
Planetary Radius
2.453 R⊕
Planetary Mass
6.590 M⊕
Surface Gravity
1.1 g / g⊕
Equilibrium Temp
—
Orbital Period
6.836 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.71 / 1.00 Moderate

Astrophysical Synthesis & Habitability Characterization

TIC 139702105 b is a confirmed sub-neptune exoplanet orbiting the star TIC 139702105, located approximately 299.4 light-years (91.79 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 0.0322% across the stellar disk), this world measures 2.453 Earth radii and has a measured mass of 6.59 Earth masses. Combining its mass and radius yields a mean bulk density of 2.46 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.1 g⊕ (10.79 m/s²), and an escape velocity of 18.3 km/s.

In its orbital architecture around TIC 139702105, TIC 139702105 b completes one full revolution every 6.836 Earth days.

☁️ Atmospheric Regime (Volatile / Gas Envelope): With a radius of 2.453 R⊕, TIC 139702105 b exceeds the empirical ~1.8–2.2 R⊕ Fulton radius valley threshold, indicating a substantial hydrogen-helium or supercritical volatile envelope without a conventional solid terrestrial surface.

The host star TIC 139702105 is classified as a stellar host with an effective photospheric temperature of 5,742 K, a radius of 1.2542 R☉, a mass of 0.9 M☉, an estimated bolometric luminosity of 1.534 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.28 dex (metal-poor relative to the Sun). From Earth, TIC 139702105 shines at apparent V-band magnitude 9.651 (accessible to binoculars and small amateur telescopes) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.71 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 TIC 139702105
Spectral Type Unclassified
Effective Temp (Teff) 5,742 K
Stellar Radius 1.2542 R☉
Stellar Mass 0.9000 M☉
Bolometric Luminosity 1.534 L☉
Metallicity [Fe/H] -0.280 dex
Stellar Age —
Apparent Magnitude V: 9.651 · G: 9.456
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 6.836 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.8402°
Mean Bulk Density 2.46 g/cm³ (18.3 km/s vesc)
Insolation Flux —
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 299.400 LY (91.788 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 04h25m59.53s · DEC: -18d12m52.36s (J2000: 66.49803°, -18.21455°)
Target Field: TIC 139702105 (J2000 66.49803°, -18.21455°)
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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