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CONFIRMED EXOPLANET · Sub-Neptune

TOI-1777.01

Orbits Host Star: TOI-1777 · Distance: 260.200 Light-Years (79.767 pc)
Planetary Radius
2.246 R⊕
Planetary Mass
5.670 M⊕
Surface Gravity
1.12 g / g⊕
Equilibrium Temp
580K (+307°C / +585°F)
Orbital Period
14.65 days
Discovery Year
2024 (Transit)
Earth Similarity (ESI)
0.45 / 1.00
Insolation Flux
71.34 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-1777.01 is a confirmed sub-neptune exoplanet orbiting the star TOI-1777, located approximately 260.2 light-years (79.77 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 0.0441% across the stellar disk), this world measures 2.246 Earth radii and has a measured mass of 5.67 Earth masses. Combining its mass and radius yields a mean bulk density of 2.76 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.12 g⊕ (10.98 m/s²), and an escape velocity of 17.8 km/s.

In its orbital architecture around TOI-1777, TOI-1777.01 completes one full revolution every 14.65 Earth days at a semi-major axis of 0.119466 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 88.7 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 580 K (+307°C / +585°F) and receiving 71.34 S⊕ (~97,094 W/m²), TOI-1777.01 orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-1777 is classified as a stellar host with an effective photospheric temperature of 5,859 K, a radius of 0.98 R☉, a mass of 1.06 M☉, an estimated bolometric luminosity of 1.015 L☉. From Earth, TOI-1777 shines at apparent V-band magnitude 9.31 (accessible to binoculars and small amateur telescopes) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.45 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-1777
Spectral Type Unclassified
Effective Temp (Teff) 5,859 K
Stellar Radius 0.9800 R☉
Stellar Mass 1.0600 M☉
Bolometric Luminosity 1.015 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 9.310 · G: 9.154
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.119466 AU
Orbital Period 14.65 days
Mean Orbital Velocity 88.7 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 2.76 g/cm³ (17.8 km/s vesc)
Insolation Flux 71.3400 S⊕ (~97,094 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 260.200 LY (79.767 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 10h07m13.69s · DEC: +46d06m53.57s (J2000: 151.80703°, 46.11488°)
Target Field: TOI-1777 (J2000 151.80703°, 46.11488°)
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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