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CONFIRMED EXOPLANET · Sub-Neptune

TIC 18942729 b

Orbits Host Star: TIC 18942729 · Distance: 375.600 Light-Years (115.169 pc)
Planetary Radius
2.000 R⊕
Planetary Mass
4.660 M⊕
Surface Gravity
1.17 g / g⊕
Equilibrium Temp
—
Orbital Period
0.998 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.79 / 1.00 Moderate

Astrophysical Synthesis & Habitability Characterization

TIC 18942729 b is a confirmed sub-neptune exoplanet orbiting the star TIC 18942729, located approximately 375.6 light-years (115.17 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 0.0494% across the stellar disk), this world measures 2 Earth radii and has a measured mass of 4.66 Earth masses. Combining its mass and radius yields a mean bulk density of 3.21 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.17 g⊕ (11.47 m/s²), and an escape velocity of 17.1 km/s.

In its orbital architecture around TIC 18942729, TIC 18942729 b completes one full revolution every 0.998 Earth days.

ℹ️ Thermal & Atmospheric Regime: Current photometric and spectroscopic constraints for TIC 18942729 b place it outside the conservative habitable zone definition pending further atmospheric characterization.

The host star TIC 18942729 is classified as a stellar host with an effective photospheric temperature of 4,360 K, a radius of 0.8253 R☉, a mass of 0.652 M☉, an estimated bolometric luminosity of 0.221 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = 0.012 dex (near-solar heavy-element abundance). From Earth, TIC 18942729 shines at apparent V-band magnitude 12.545 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.79 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 18942729
Spectral Type Unclassified
Effective Temp (Teff) 4,360 K
Stellar Radius 0.8253 R☉
Stellar Mass 0.6520 M☉
Bolometric Luminosity 0.221 L☉
Metallicity [Fe/H] 0.012 dex
Stellar Age —
Apparent Magnitude V: 12.545 · G: 12.278
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 0.998 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 85.2341°
Mean Bulk Density 3.21 g/cm³ (17.1 km/s vesc)
Insolation Flux —
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 375.600 LY (115.169 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 07h56m51.62s · DEC: +16d40m38.04s (J2000: 119.21507°, 16.67723°)
Target Field: TIC 18942729 (J2000 119.21507°, 16.67723°)
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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