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CONFIRMED EXOPLANET · Sub-Neptune

TOI-1744.01

Orbits Host Star: TOI-1744 · Distance: 373.100 Light-Years (114.390 pc)
Planetary Radius
2.680 R⊕
Planetary Mass
7.650 M⊕
Surface Gravity
1.07 g / g⊕
Equilibrium Temp
598K (+325°C / +617°F)
Orbital Period
22.342 days
Discovery Year
2024 (Transit)
Earth Similarity (ESI)
0.41 / 1.00
Insolation Flux
63.31 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-1744.01 is a confirmed sub-neptune exoplanet orbiting the star TOI-1744, located approximately 373.1 light-years (114.39 parsecs) from the Solar System. First announced in 2024 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.0465% across the stellar disk), this world measures 2.68 Earth radii and has a measured mass of 7.65 Earth masses. Combining its mass and radius yields a mean bulk density of 2.19 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.07 g⊕ (10.49 m/s²), and an escape velocity of 18.9 km/s.

In its orbital architecture around TOI-1744, TOI-1744.01 completes one full revolution every 22.342 Earth days at a semi-major axis of 0.164086 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 79.9 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 598 K (+325°C / +617°F) and receiving 63.31 S⊕ (~86,165 W/m²), TOI-1744.01 orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-1744 is classified as a stellar host with an effective photospheric temperature of 6,179 K, a radius of 1.14 R☉, a mass of 1.18 M☉, an estimated bolometric luminosity of 1.7 L☉. From Earth, TOI-1744 shines at apparent V-band magnitude 9.543 (accessible to binoculars and small amateur telescopes) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.41 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-1744
Spectral Type Unclassified
Effective Temp (Teff) 6,179 K
Stellar Radius 1.1400 R☉
Stellar Mass 1.1800 M☉
Bolometric Luminosity 1.7 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 9.543 · G: 9.392
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.164086 AU
Orbital Period 22.342 days
Mean Orbital Velocity 79.9 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 2.19 g/cm³ (18.9 km/s vesc)
Insolation Flux 63.3100 S⊕ (~86,165 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 373.100 LY (114.390 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 19h37m09.86s · DEC: +60d52m52.69s (J2000: 294.29107°, 60.8813°)
Target Field: TOI-1744 (J2000 294.29107°, 60.8813°)
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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