TOI-1450 A

Planetary system · 73.2 light-years away

TOI-1450 A is 73.2 light-years from the Sun. The NASA Exoplanet Archive lists 2 planets around this M3.0 V star; the first was found in 2024 by transit (Transiting Exoplanet Survey Satellite (TESS)).

Fly there in 3D

Worth knowing

TOI-1450 A b goes round its star every 2.04 days, 43 times as often as Mercury goes round the Sun.

TOI-1450 A is one of 2 stars in its system: the other is drawn where the Washington Double Star Catalog measures it on the sky.

Where the archive gives only a period or only an orbit size, the other is worked out from Kepler’s third law with the star’s mass.

The star

Spectral typeM3.0 V
Surface temperature3,437 K
Mass0.48 solar masses
Radius0.483 solar radii
Luminosity0.02723 times the Sun
Apparent magnitude12.28
Distance from the Sun73.2 light-years (22.4 parsecs)
Position (J2000)RA 286.8541°, Dec 59.0866°
ConstellationDraco

The other star

TOI-1450 B has no spectral type listed of magnitude 16.53, moving through space with it. In 2021 it was 3.2″ from TOI-1450 A, at position angle 325° (Washington Double Star Catalog, 19074+5905 KPP3335 AB): 71.8 AU on the sky at this distance. The true distance can only be larger. Its colour is estimated from its brightness.

Planets (2)

PlanetYearOrbitRadiusMassFound
TOI-1450 A b2.04 days0.0247 AU from Kepler’s law1.13 R⊕1.258 M⊕Transit, 2024
TOI-1450 A c5.07 days0.0452 AU from Kepler’s law1.13 R⊕ estimated1.527 M⊕ minimumTransit, 2024

Values are the NASA Exoplanet Archive’s composite parameters. A radius marked estimated comes from a mass–radius relation; a mass marked minimum is M sin i. Planet sizes and colours in the 3D view are renderings: none of these worlds has been photographed as more than a point of light.

The planets, compared

For a star of 3,437 K, 0.027 times as bright as the Sun, the habitable zone, where starlight could keep water liquid on a rocky surface, runs from about 0.17 to 0.33 AU. None of its known planets orbits inside it. The zone says how much starlight arrives, not whether a planet has water or air. The edges follow Kopparapu et al. (2014), as the 3D view draws them.

The light you see left 73 years ago, within living memory.

Nearest systems to it

Also found by Transiting Exoplanet Survey Satellite (TESS)

Sources

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