TOI-1450 A b
Astrophysical Synthesis & Habitability Characterization
TOI-1450 A b is a confirmed terrestrial exoplanet orbiting the star TOI-1450 A, located approximately 73.2 light-years (22.45 parsecs) from the Solar System. First announced in 2024 by Transiting Exoplanet Survey Satellite (TESS) using the Transit detection technique (producing an estimated primary transit depth of 0.046% across the stellar disk), this world measures 1.13 Earth radii and has a measured mass of 1.258 Earth masses. Combining its mass and radius yields a mean bulk density of 4.81 g/cm³ (a terrestrial silicate-iron composition comparable to Earth (5.51 g/cm³)), a surface gravity of 0.99 g⊕ (9.71 m/s²), and an escape velocity of 11.8 km/s.
In its orbital architecture around TOI-1450 A, TOI-1450 A b completes one full revolution every 2.044 Earth days.
⚠️ Thermal Regime (Irradiated / Hot Zone): At an equilibrium temperature of 722 K (+449°C / +840°F) and receiving 44.95 S⊕ (~61,176 W/m²), TOI-1450 A b orbits interior to the runaway greenhouse boundary where surface liquid water cannot persist.
The host star TOI-1450 A is classified as a low-mass red dwarf of spectral type M3.0 V with an effective photospheric temperature of 3,437 K, a radius of 0.483 R☉, a mass of 0.48 M☉, an estimated bolometric luminosity of 0.029 L☉. Stellar evolution modeling indicates a metallicity of [Fe/H] = -0.12 dex (metal-poor relative to the Sun). From Earth, TOI-1450 A shines at apparent V-band magnitude 12.28 (faint and requiring research-grade or CCD telescopic photometry) in the Northern celestial hemisphere. The TOI-1450 A system is a multi-planet architecture hosting 2 confirmed worlds, with TOI-1450 A b sharing its stellar neighborhood alongside TOI-1450 A c.
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-1450 A |
| Spectral Type | M3.0 V |
| Effective Temp (Teff) | 3,437 K |
| Stellar Radius | 0.4830 R☉ |
| Stellar Mass | 0.4800 M☉ |
| Bolometric Luminosity | 0.029 L☉ |
| Metallicity [Fe/H] | -0.120 dex |
| Stellar Age | — |
| Apparent Magnitude | V: 12.280 · G: 11.239 |
| System Architecture | 2 Stars, 2 Planets |
🪐 Orbital & Physical Dynamics
| Semi-Major Axis (a) | — |
| Orbital Period | 2.044 days |
| Orbital Eccentricity (e) | Circular (0.00) |
| Orbital Inclination (i) | 86.2450° |
| Mean Bulk Density | 4.81 g/cm³ (11.8 km/s vesc) |
| Insolation Flux | 44.9493 S⊕ (~61,176 W/m²) |
| Habitable Zone Status | Exterior / Non-HZ |
| Celestial Distance | 73.200 LY (22.447 pc) |