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CONFIRMED EXOPLANET · Sub-Neptune

TOI-921 b

Orbits Host Star: TOI-921 · Distance: 958.900 Light-Years (294.015 pc)
Planetary Radius
3.534 R⊕
Planetary Mass
12.200 M⊕
Surface Gravity
0.98 g / g⊕
Equilibrium Temp
951K (+678°C / +1252°F)
Orbital Period
5.129 days
Discovery Year
2026 (Transit)
Earth Similarity (ESI)
0.23 / 1.00
Insolation Flux
426.77 S⊕

Astrophysical Synthesis & Habitability Characterization

TOI-921 b is a confirmed sub-neptune exoplanet orbiting the star TOI-921, located approximately 958.9 light-years (294.02 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 0.0805% across the stellar disk), this world measures 3.534 Earth radii (0.32 Jupiter radii) and has a measured mass of 12.2 Earth masses. Combining its mass and radius yields a mean bulk density of 1.52 g/cm³ (a low bulk density dominated by an extended hydrogen-helium gaseous envelope), a surface gravity of 0.98 g⊕ (9.61 m/s²), and an escape velocity of 20.8 km/s.

In its orbital architecture around TOI-921, TOI-921 b completes one full revolution every 5.129 Earth days.

⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 951 K (+678°C / +1252°F) and receiving 426.77 S⊕ (~580,832 W/m²), TOI-921 b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.

The host star TOI-921 is classified as a stellar host with an effective photospheric temperature of 6,012 K, a radius of 1.1417 R☉, a mass of 1.13 M☉, an estimated bolometric luminosity of 1.528 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.058 dex (near-solar heavy-element abundance). From Earth, TOI-921 shines at apparent V-band magnitude 11.813 (faint and requiring research-grade or CCD telescopic photometry) in the Southern celestial hemisphere.

Earth Similarity Index (ESI): 0.23 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-921
Spectral Type Unclassified
Effective Temp (Teff) 6,012 K
Stellar Radius 1.1417 R☉
Stellar Mass 1.1300 M☉
Bolometric Luminosity 1.528 L☉
Metallicity [Fe/H] -0.058 dex
Stellar Age —
Apparent Magnitude V: 11.813 · G: 11.634
System Architecture 1 Star, 1 Planet

🪐 Orbital & Physical Dynamics

Semi-Major Axis (a) —
Orbital Period 5.129 days
Orbital Eccentricity (e) Circular (0.00)
Orbital Inclination (i) 86.5756°
Mean Bulk Density 1.52 g/cm³ (20.8 km/s vesc)
Insolation Flux 426.7683 S⊕ (~580,832 W/m²)
Habitable Zone Status Exterior / Non-HZ
Celestial Distance 958.900 LY (294.015 pc)

🔭 Deep Space Viewport // Host Star Field

RA: 06h38m41.81s · DEC: -56d13m13.94s (J2000: 99.6742°, -56.22054°)
Target Field: TOI-921 (J2000 99.6742°, -56.22054°)
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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