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CONFIRMED EXOPLANET · Sub-Neptune

TOI-1659.01

Orbits Host Star: TOI-1659 · Distance: 399.500 Light-Years (122.494 pc)
Planetary Radius
2.255 R⊕
Planetary Mass
5.710 M⊕
Surface Gravity
1.12 g / g⊕
Equilibrium Temp
1031K (+758°C / +1396°F)
Orbital Period
5.878 days
Discovery Year
2024 (Transit)
Earth Similarity (ESI)
0.25 / 1.00
Insolation Flux
268.44 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-1659.01 is a confirmed sub-neptune exoplanet orbiting the star TOI-1659, located approximately 399.5 light-years (122.49 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 0.0422% across the stellar disk), this world measures 2.255 Earth radii and has a measured mass of 5.71 Earth masses. Combining its mass and radius yields a mean bulk density of 2.75 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-1659, TOI-1659.01 completes one full revolution every 5.878 Earth days at a semi-major axis of 0.065757 AU (orbiting interior to Mercury's 0.387 AU benchmark in the Solar System). Its mean orbital velocity is approximately 121.7 km/s (compared to Earth's 29.8 km/s).

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1031 K (+758°C / +1396°F) and receiving 268.44 S⊕ (~365,347 W/m²), TOI-1659.01 orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-1659 is classified as a stellar host with an effective photospheric temperature of 5,977 K, a radius of 1.006 R☉, a mass of 1.1 M☉, an estimated bolometric luminosity of 1.159 L☉. From Earth, TOI-1659 shines at apparent V-band magnitude 10.078 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.25 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-1659
Spectral Type Unclassified
Effective Temp (Teff) 5,977 K
Stellar Radius 1.0060 R☉
Stellar Mass 1.1000 M☉
Bolometric Luminosity 1.159 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 10.078 · G: 9.976
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) 0.065757 AU
Orbital Period 5.878 days
Mean Orbital Velocity 121.7 km/s
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 2.75 g/cm³ (17.8 km/s vesc)
Insolation Flux 268.4400 S⊕ (~365,347 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 399.500 LY (122.494 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 18h31m42.05s · DEC: +82d18m21.42s (J2000: 277.92519°, 82.30595°)
Target Field: TOI-1659 (J2000 277.92519°, 82.30595°)
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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