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CONFIRMED EXOPLANET · Sub-Neptune

TOI-1054.01

Orbits Host Star: TOI-1054 · Distance: 288.400 Light-Years (88.434 pc)
Planetary Radius
2.434 R⊕
Planetary Mass
6.500 M⊕
Surface Gravity
1.1 g / g⊕
Equilibrium Temp
853K (+580°C / +1076°F)
Orbital Period
15.508 days
Discovery Year
2021 (Transit)
Earth Similarity (ESI)
0.30 / 1.00
Insolation Flux
88.07 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-1054.01 is a confirmed sub-neptune exoplanet orbiting the star TOI-1054, located approximately 288.4 light-years (88.43 parsecs) from the Solar System. First announced in 2021 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.0364% across the stellar disk), this world measures 2.434 Earth radii and has a measured mass of 6.5 Earth masses. Combining its mass and radius yields a mean bulk density of 2.49 g/cm³ (an intermediate density indicative of a deep water-ice mantle or dense volatile envelope), a surface gravity of 1.1 g⊕ (10.79 m/s²), and an escape velocity of 18.3 km/s.

In its orbital architecture around TOI-1054, TOI-1054.01 completes one full revolution every 15.508 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 853 K (+580°C / +1076°F) and receiving 88.07 S⊕ (~119,866 W/m²), TOI-1054.01 orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-1054 is classified as a stellar host with an effective photospheric temperature of 6,122 K, a radius of 1.17 R☉, a mass of 1.14 M☉, an estimated bolometric luminosity of 1.725 L☉. From Earth, TOI-1054 shines at apparent V-band magnitude 8.95 (accessible to binoculars and small amateur telescopes) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.30 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-1054
Spectral Type Unclassified
Effective Temp (Teff) 6,122 K
Stellar Radius 1.1700 R☉
Stellar Mass 1.1400 M☉
Bolometric Luminosity 1.725 L☉
Metallicity [Fe/H] —
Stellar Age —
Apparent Magnitude V: 8.950 · G: 8.817
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 15.508 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) —
Mean Bulk Density 2.49 g/cm³ (18.3 km/s vesc)
Insolation Flux 88.0718 S⊕ (~119,866 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 288.400 LY (88.434 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 20h08m27.40s · DEC: -54d19m03.01s (J2000: 302.11417°, -54.3175°)
Target Field: TOI-1054 (J2000 302.11417°, -54.3175°)
Surveys available: Digitized Sky Survey (DSS2 Optical), 2MASS (Near-Infrared), AllWISE (Mid-Infrared) · Field of View: 0.18° (10.8 arcmin)
Aladin Lite v3 · Centre de Données astronomiques de Strasbourg (CDS)
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