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CONFIRMED EXOPLANET · Sub-Neptune

TOI-7008 b

Orbits Host Star: TOI-7008 · Distance: 1338.800 Light-Years (410.467 pc)
Planetary Radius
4.947 R⊕
Planetary Mass
21.700 M⊕
Surface Gravity
0.89 g / g⊕
Equilibrium Temp
1783K (+1510°C / +2750°F)
Orbital Period
0.841 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.10 / 1.00
Insolation Flux
1,679.35 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-7008 b is a confirmed sub-neptune exoplanet orbiting the star TOI-7008, located approximately 1338.8 light-years (410.47 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 0.2267% across the stellar disk), this world measures 4.947 Earth radii (0.44 Jupiter radii) and has a measured mass of 21.7 Earth masses. Combining its mass and radius yields a mean bulk density of 0.99 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.89 g⊕ (8.73 m/s²), and an escape velocity of 23.4 km/s.

In its orbital architecture around TOI-7008, TOI-7008 b completes one full revolution every 0.841 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1783 K (+1510°C / +2750°F) and receiving 1,679.35 S⊕ (~2,285,595 W/m²), TOI-7008 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-7008 is classified as a stellar host with an effective photospheric temperature of 5,116 K, a radius of 0.9526 R☉, a mass of 0.88 M☉, an estimated bolometric luminosity of 0.558 L☉. From Earth, TOI-7008 shines at apparent V-band magnitude 13.6 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.10 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 TOI-7008
Spectral Type Unclassified
Effective Temp (Teff) 5,116 K
Stellar Radius 0.9526 R☉
Stellar Mass 0.8800 M☉
Bolometric Luminosity 0.558 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 13.600 · G: 13.452
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 0.841 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 81.4173°
Mean Bulk Density 0.99 g/cm³ (23.4 km/s vesc)
Insolation Flux 1679.3500 S⊕ (~2,285,595 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1338.800 LY (410.467 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 14h27m57.18s · DEC: +79d27m01.43s (J2000: 216.98825°, 79.4504°)
Target Field: TOI-7008 (J2000 216.98825°, 79.4504°)
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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