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CONFIRMED EXOPLANET · Sub-Neptune

TIC 423703298 b

Orbits Host Star: TIC 423703298 · Distance: 444.200 Light-Years (136.191 pc)
Planetary Radius
2.772 R⊕
Planetary Mass
8.110 M⊕
Surface Gravity
1.06 g / g⊕
Equilibrium Temp
—
Orbital Period
4.037 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.67 / 1.00

Astrophysical Synthesis & Habitability Characterization

TIC 423703298 b is a confirmed sub-neptune exoplanet orbiting the star TIC 423703298, located approximately 444.2 light-years (136.19 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 0.1213% across the stellar disk), this world measures 2.772 Earth radii and has a measured mass of 8.11 Earth masses. Combining its mass and radius yields a mean bulk density of 2.1 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.06 g⊕ (10.4 m/s²), and an escape velocity of 19.1 km/s.

In its orbital architecture around TIC 423703298, TIC 423703298 b completes one full revolution every 4.037 Earth days.

☁️ Atmospheric Regime (Volatile / Gas Envelope): With a radius of 2.772 R⊕, TIC 423703298 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 423703298 is classified as a stellar host with an effective photospheric temperature of 4,540 K, a radius of 0.7298 R☉, a mass of 0.691 M☉, an estimated bolometric luminosity of 0.203 L☉. From Earth, TIC 423703298 shines at apparent V-band magnitude 12.923 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.67 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 423703298
Spectral Type Unclassified
Effective Temp (Teff) 4,540 K
Stellar Radius 0.7298 R☉
Stellar Mass 0.6910 M☉
Bolometric Luminosity 0.203 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 12.923 · G: 12.537
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 4.037 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.3796°
Mean Bulk Density 2.1 g/cm³ (19.1 km/s vesc)
Insolation Flux —
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 444.200 LY (136.191 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 01h31m44.65s · DEC: -17d00m48.84s (J2000: 22.93605°, -17.01357°)
Target Field: TIC 423703298 (J2000 22.93605°, -17.01357°)
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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