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CONFIRMED EXOPLANET · Sub-Neptune

TOI-2545 b

Orbits Host Star: TOI-2545 · Distance: 349.400 Light-Years (107.118 pc)
Planetary Radius
2.750 R⊕
Planetary Mass
8.000 M⊕
Surface Gravity
1.06 g / g⊕
Equilibrium Temp
1023K (+750°C / +1382°F)
Orbital Period
7.994 days
Discovery Year
2022 (Transit)
Earth Similarity (ESI)
0.24 / 1.00
Insolation Flux
258.82 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-2545 b is a confirmed sub-neptune exoplanet orbiting the star TOI-2545, located approximately 349.4 light-years (107.12 parsecs) from the Solar System. First announced in 2022 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.0405% across the stellar disk), this world measures 2.75 Earth radii and has a measured mass of 8 Earth masses. Combining its mass and radius yields a mean bulk density of 2.12 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.06 g⊕ (10.4 m/s²), and an escape velocity of 19.1 km/s.

In its orbital architecture around TOI-2545, TOI-2545 b completes one full revolution every 7.994 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 1023 K (+750°C / +1382°F) and receiving 258.82 S⊕ (~352,256 W/m²), TOI-2545 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-2545 is classified as a stellar host with an effective photospheric temperature of 5,846 K, a radius of 1.2532 R☉, a mass of 1.055 M☉, an estimated bolometric luminosity of 1.646 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.273 dex (metal-poor relative to the Sun). From Earth, TOI-2545 shines at apparent V-band magnitude 9.521 (accessible to binoculars and small amateur telescopes) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.24 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-2545
Spectral Type Unclassified
Effective Temp (Teff) 5,846 K
Stellar Radius 1.2532 R☉
Stellar Mass 1.0550 M☉
Bolometric Luminosity 1.646 L☉
Metallicity [Fe/H] -0.273 dex
Stellar Age —
Apparent Magnitude V: 9.521 · G: 9.295
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 7.994 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 2.12 g/cm³ (19.1 km/s vesc)
Insolation Flux 258.8217 S⊕ (~352,256 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 349.400 LY (107.118 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 09h02m10.99s · DEC: -03d25m14.95s (J2000: 135.5458°, -3.42082°)
Target Field: TOI-2545 (J2000 135.5458°, -3.42082°)
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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