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CONFIRMED EXOPLANET · Sub-Neptune

TIC 117642575 b

Orbits Host Star: TIC 117642575 · Distance: 615.600 Light-Years (188.758 pc)
Planetary Radius
2.827 R⊕
Planetary Mass
8.380 M⊕
Surface Gravity
1.05 g / g⊕
Equilibrium Temp
—
Orbital Period
4.945 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.66 / 1.00

Astrophysical Synthesis & Habitability Characterization

TIC 117642575 b is a confirmed sub-neptune exoplanet orbiting the star TIC 117642575, located approximately 615.6 light-years (188.76 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 0.0575% across the stellar disk), this world measures 2.827 Earth radii and has a measured mass of 8.38 Earth masses. Combining its mass and radius yields a mean bulk density of 2.05 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.05 g⊕ (10.3 m/s²), and an escape velocity of 19.3 km/s.

In its orbital architecture around TIC 117642575, TIC 117642575 b completes one full revolution every 4.945 Earth days.

☁️ Atmospheric Regime (Volatile / Gas Envelope): With a radius of 2.827 R⊕, TIC 117642575 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 117642575 is classified as a stellar host with an effective photospheric temperature of 5,720 K, a radius of 1.081 R☉, a mass of 1.06 M☉, an estimated bolometric luminosity of 1.122 L☉. From Earth, TIC 117642575 shines at apparent V-band magnitude 11.029 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.66 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 117642575
Spectral Type Unclassified
Effective Temp (Teff) 5,720 K
Stellar Radius 1.0810 R☉
Stellar Mass 1.0600 M☉
Bolometric Luminosity 1.122 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 11.029 · G: 10.841
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 4.945 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 86.9056°
Mean Bulk Density 2.05 g/cm³ (19.3 km/s vesc)
Insolation Flux —
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 615.600 LY (188.758 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 00h37m55.22s · DEC: -37d03m58.65s (J2000: 9.48007°, -37.06629°)
Target Field: TIC 117642575 (J2000 9.48007°, -37.06629°)
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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