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CONFIRMED EXOPLANET · Sub-Neptune

TIC 237254473 b

Orbits Host Star: TIC 237254473 · Distance: 1326.300 Light-Years (406.633 pc)
Planetary Radius
3.300 R⊕
Planetary Mass
10.900 M⊕
Surface Gravity
1 g / g⊕
Equilibrium Temp
—
Orbital Period
10.118 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.61 / 1.00

Astrophysical Synthesis & Habitability Characterization

TIC 237254473 b is a confirmed sub-neptune exoplanet orbiting the star TIC 237254473, located approximately 1326.3 light-years (406.63 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 0.0493% across the stellar disk), this world measures 3.3 Earth radii (0.29 Jupiter radii) and has a measured mass of 10.9 Earth masses. Combining its mass and radius yields a mean bulk density of 1.67 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 1 g⊕ (9.81 m/s²), and an escape velocity of 20.3 km/s.

In its orbital architecture around TIC 237254473, TIC 237254473 b completes one full revolution every 10.118 Earth days.

☁️ Atmospheric Regime (Volatile / Gas Envelope): With a radius of 3.300 R⊕, TIC 237254473 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 237254473 is classified as a stellar host with an effective photospheric temperature of 5,700 K, a radius of 1.362 R☉, a mass of 1.12 M☉, an estimated bolometric luminosity of 1.757 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.006 dex (near-solar heavy-element abundance). From Earth, TIC 237254473 shines at apparent V-band magnitude 12.241 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.61 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 237254473
Spectral Type Unclassified
Effective Temp (Teff) 5,700 K
Stellar Radius 1.3620 R☉
Stellar Mass 1.1200 M☉
Bolometric Luminosity 1.757 L☉
Metallicity [Fe/H] -0.006 dex
Stellar Age —
Apparent Magnitude V: 12.241 · G: 12.159
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 10.118 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 1.67 g/cm³ (20.3 km/s vesc)
Insolation Flux —
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1326.300 LY (406.633 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h55m59.13s · DEC: +72d55m11.86s (J2000: 298.99638°, 72.91996°)
Target Field: TIC 237254473 (J2000 298.99638°, 72.91996°)
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)
SIMBAD Astronomical Query ↗ NASA ADS Research Papers ↗
NASA EXOPLANET ARCHIVE COMPOSITE PARAMETERS
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