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CONFIRMED EXOPLANET · Sub-Neptune

TOI-1291 b

Orbits Host Star: TOI-1291 · Distance: 1396.300 Light-Years (428.123 pc)
Planetary Radius
5.638 R⊕
Planetary Mass
27.100 M⊕
Surface Gravity
0.85 g / g⊕
Equilibrium Temp
1649K (+1376°C / +2509°F)
Orbital Period
7.162 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.10 / 1.00
Insolation Flux
1,230.42 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-1291 b is a confirmed sub-neptune exoplanet orbiting the star TOI-1291, located approximately 1396.3 light-years (428.12 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 0.0815% across the stellar disk), this world measures 5.638 Earth radii (0.5 Jupiter radii) and has a measured mass of 27.1 Earth masses. Combining its mass and radius yields a mean bulk density of 0.83 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.85 g⊕ (8.34 m/s²), and an escape velocity of 24.5 km/s.

In its orbital architecture around TOI-1291, TOI-1291 b completes one full revolution every 7.162 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1649 K (+1376°C / +2509°F) and receiving 1,230.42 S⊕ (~1,674,602 W/m²), TOI-1291 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-1291 is classified as a stellar host with an effective photospheric temperature of 6,140 K, a radius of 1.8109 R☉, a mass of 1.2 M☉, an estimated bolometric luminosity of 4.182 L☉. From Earth, TOI-1291 shines at apparent V-band magnitude 11.516 (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-1291
Spectral Type Unclassified
Effective Temp (Teff) 6,140 K
Stellar Radius 1.8109 R☉
Stellar Mass 1.2000 M☉
Bolometric Luminosity 4.182 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 11.516 · G: 11.244
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 7.162 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 88.3839°
Mean Bulk Density 0.83 g/cm³ (24.5 km/s vesc)
Insolation Flux 1230.4200 S⊕ (~1,674,602 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 1396.300 LY (428.123 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 16h23m16.32s · DEC: +62d55m30.44s (J2000: 245.81801°, 62.92512°)
Target Field: TOI-1291 (J2000 245.81801°, 62.92512°)
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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