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CONFIRMED EXOPLANET · Sub-Neptune

TOI-2459 b

Orbits Host Star: TOI-2459 · Distance: 119.400 Light-Years (36.611 pc)
Planetary Radius
2.953 R⊕
Planetary Mass
9.030 M⊕
Surface Gravity
1.04 g / g⊕
Equilibrium Temp
445K (+172°C / +342°F)
Orbital Period
19.105 days
Discovery Year
2023 (Transit)
Earth Similarity (ESI)
0.51 / 1.00
Insolation Flux
8.52 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-2459 b is a confirmed sub-neptune exoplanet orbiting the star TOI-2459, located approximately 119.4 light-years (36.61 parsecs) from the Solar System. First announced in 2023 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.1608% across the stellar disk), this world measures 2.953 Earth radii and has a measured mass of 9.03 Earth masses. Combining its mass and radius yields a mean bulk density of 1.93 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 1.04 g⊕ (10.2 m/s²), and an escape velocity of 19.6 km/s.

In its orbital architecture around TOI-2459, TOI-2459 b completes one full revolution every 19.105 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 445 K (+172°C / +342°F) and receiving 8.52 S⊕ (~11,594 W/m²), TOI-2459 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-2459 is classified as a stellar host with an effective photospheric temperature of 4,195 K, a radius of 0.6751 R☉, a mass of 0.66 M☉, an estimated bolometric luminosity of 0.127 L☉. From Earth, TOI-2459 shines at apparent V-band magnitude 10.772 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.51 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-2459
Spectral Type Unclassified
Effective Temp (Teff) 4,195 K
Stellar Radius 0.6751 R☉
Stellar Mass 0.6600 M☉
Bolometric Luminosity 0.127 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 10.772 · G: 10.165
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 19.105 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 89.5900°
Mean Bulk Density 1.93 g/cm³ (19.6 km/s vesc)
Insolation Flux 8.5187 S⊕ (~11,594 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 119.400 LY (36.611 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 05h28m34.40s · DEC: -39d22m22.96s (J2000: 82.14333°, -39.37305°)
Target Field: TOI-2459 (J2000 82.14333°, -39.37305°)
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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