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CONFIRMED EXOPLANET · Super-Earth

TOI-1756 b

Orbits Host Star: TOI-1756 · Distance: 282.800 Light-Years (86.716 pc)
Planetary Radius
1.942 R⊕
Planetary Mass
4.430 M⊕
Surface Gravity
1.17 g / g⊕
Equilibrium Temp
696K (+423°C / +793°F)
Orbital Period
2.783 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.40 / 1.00
Insolation Flux
55.58 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-1756 b is a confirmed super-earth exoplanet orbiting the star TOI-1756, located approximately 282.8 light-years (86.72 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 0.1001% across the stellar disk), this world measures 1.942 Earth radii and has a measured mass of 4.43 Earth masses. Combining its mass and radius yields a mean bulk density of 3.34 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.17 g⊕ (11.47 m/s²), and an escape velocity of 16.9 km/s.

In its orbital architecture around TOI-1756, TOI-1756 b completes one full revolution every 2.783 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 696 K (+423°C / +793°F) and receiving 55.58 S⊕ (~75,648 W/m²), TOI-1756 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-1756 is classified as a stellar host with an effective photospheric temperature of 3,892 K, a radius of 0.5626 R☉, a mass of 0.5565 M☉, an estimated bolometric luminosity of 0.065 L☉. From Earth, TOI-1756 shines at apparent V-band magnitude 13.88 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.40 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-1756
Spectral Type Unclassified
Effective Temp (Teff) 3,892 K
Stellar Radius 0.5626 R☉
Stellar Mass 0.5565 M☉
Bolometric Luminosity 0.065 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 13.880 · G: 13.110
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 2.783 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 87.4364°
Mean Bulk Density 3.34 g/cm³ (16.9 km/s vesc)
Insolation Flux 55.5824 S⊕ (~75,648 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 282.800 LY (86.716 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 20h25m18.91s · DEC: +77d38m11.08s (J2000: 306.32877°, 77.63641°)
Target Field: TOI-1756 (J2000 306.32877°, 77.63641°)
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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