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CONFIRMED EXOPLANET · Sub-Neptune

TOI-5595 b

Orbits Host Star: TOI-5595 · Distance: 446.700 Light-Years (136.955 pc)
Planetary Radius
4.737 R⊕
Planetary Mass
20.100 M⊕
Surface Gravity
0.9 g / g⊕
Equilibrium Temp
621K (+348°C / +658°F)
Orbital Period
5.99 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.31 / 1.00
Insolation Flux
24.76 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-5595 b is a confirmed sub-neptune exoplanet orbiting the star TOI-5595, located approximately 446.7 light-years (136.96 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 0.3414% across the stellar disk), this world measures 4.737 Earth radii (0.42 Jupiter radii) and has a measured mass of 20.1 Earth masses. Combining its mass and radius yields a mean bulk density of 1.04 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.9 g⊕ (8.83 m/s²), and an escape velocity of 23 km/s.

In its orbital architecture around TOI-5595, TOI-5595 b completes one full revolution every 5.99 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 621 K (+348°C / +658°F) and receiving 24.76 S⊕ (~33,702 W/m²), TOI-5595 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-5595 is classified as a stellar host with an effective photospheric temperature of 4,417 K, a radius of 0.7433 R☉, a mass of 0.645 M☉, an estimated bolometric luminosity of 0.189 L☉. From Earth, TOI-5595 shines at apparent V-band magnitude 13.316 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere.

Earth Similarity Index (ESI): 0.31 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-5595
Spectral Type Unclassified
Effective Temp (Teff) 4,417 K
Stellar Radius 0.7433 R☉
Stellar Mass 0.6450 M☉
Bolometric Luminosity 0.189 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 13.316 · G: 12.972
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 5.99 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 89.0797°
Mean Bulk Density 1.04 g/cm³ (23 km/s vesc)
Insolation Flux 24.7628 S⊕ (~33,702 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 446.700 LY (136.955 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 07h21m50.44s · DEC: +35d13m19.14s (J2000: 110.46016°, 35.22198°)
Target Field: TOI-5595 (J2000 110.46016°, 35.22198°)
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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