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Star · M1V

TOI-6894

TOI-6894 is a main-sequence star of spectral type M1V in the constellation Leo, 238.4 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationLeo
Distance238.4 light-years (73.1 pc)
Apparent magnitudemagnitude 17.94
Absolute magnitudemagnitude 13.62
Spectral typeM1V
Surface temperature3,010 K
Luminosity0.00375 L☉
Radius0.228 R☉
Mass0.207 M☉
Metallicity [Fe/H]0.14
Right ascension (J2000)11h 33m 52.6s
Declination (J2000)+12° 27′ 04″
Space velocity (relative to the Sun)51.4 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 17.94. Visible from the whole Northern Hemisphere and south to latitude 78° S. North of latitude 78° N it never sets. It stands highest at midnight in March, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1788. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.2 million years.

The Sun seen from there

From a planet around TOI-6894, the Sun would look like a star of magnitude 9.15, in the direction where our sky has the constellation Aquarius. It would be invisible to the naked eye.

Planets

Neighbours

Its nearest neighbours in the catalogue (within 20 light-years):

  • ULAS J114105.18+091647.6 16.4 light-years
  • HIP 55488 18.4 light-years
  • HIP 55661 19.8 light-years
  • HIP 55033 19.8 light-years
  • HIP 55674 20.0 light-years

Open in the simulation

Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.