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CONFIRMED EXOPLANET · Sub-Neptune

TIC 219893931 b

Orbits Host Star: TIC 219893931 · Distance: 1338.700 Light-Years (410.453 pc)
Planetary Radius
2.920 R⊕
Planetary Mass
8.850 M⊕
Surface Gravity
1.04 g / g⊕
Equilibrium Temp
—
Orbital Period
6.41 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.65 / 1.00

Astrophysical Synthesis & Habitability Characterization

TIC 219893931 b is a confirmed sub-neptune exoplanet orbiting the star TIC 219893931, located approximately 1338.7 light-years (410.45 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 0.0435% across the stellar disk), this world measures 2.92 Earth radii and has a measured mass of 8.85 Earth masses. Combining its mass and radius yields a mean bulk density of 1.96 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 1.04 g⊕ (10.2 m/s²), and an escape velocity of 19.5 km/s.

In its orbital architecture around TIC 219893931, TIC 219893931 b completes one full revolution every 6.41 Earth days.

☁️ Atmospheric Regime (Volatile / Gas Envelope): With a radius of 2.920 R⊕, TIC 219893931 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 219893931 is classified as a stellar host with an effective photospheric temperature of 5,956 K, a radius of 1.284 R☉, a mass of 1.14 M☉, an estimated bolometric luminosity of 1.861 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -2.83 dex (metal-poor relative to the Sun). From Earth, TIC 219893931 shines at apparent V-band magnitude 12.161 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.65 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 219893931
Spectral Type Unclassified
Effective Temp (Teff) 5,956 K
Stellar Radius 1.2840 R☉
Stellar Mass 1.1400 M☉
Bolometric Luminosity 1.861 L☉
Metallicity [Fe/H] -2.830 dex
Stellar Age —
Apparent Magnitude V: 12.161 · G: 12.053
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 6.41 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 1.96 g/cm³ (19.5 km/s vesc)
Insolation Flux —
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1338.700 LY (410.453 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 17h30m14.91s · DEC: +71d50m34.61s (J2000: 262.56212°, 71.84295°)
Target Field: TIC 219893931 (J2000 262.56212°, 71.84295°)
Surveys available: Digitized Sky Survey (DSS2 Optical), 2MASS (Near-Infrared), AllWISE (Mid-Infrared) · Field of View: 0.18° (10.8 arcmin)
Aladin Lite v3 · Centre de Données astronomiques de Strasbourg (CDS)
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