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Star · M0V

TOI-1442

TOI-1442 is a main-sequence star of spectral type M0V in the constellation Draco, 135.0 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationDraco
Distance135.0 light-years (41.4 pc)
Apparent magnitudemagnitude 15.02
Absolute magnitudemagnitude 11.94
Spectral typeM0V
Surface temperature3,330 K
Luminosity0.0105 L☉
Radius0.31 R☉
Mass0.29 M☉
Right ascension (J2000)19h 09m 10.1s
Declination (J2000)+74° 10′ 28″
Space velocity (relative to the Sun)92.2 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 15.02. Visible from the whole Northern Hemisphere and south to latitude 16° S. North of latitude 16° N it never sets. It stands highest at midnight in July, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1891. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.4 million years.

The Sun seen from there

From a planet around TOI-1442, the Sun would look like a star of magnitude 7.91, in the direction where our sky has the constellation Volans. It would be invisible to the naked eye.

Planets

Neighbours

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

  • TOI-2095 3.57 light-years
  • HIP 93119 4.54 light-years
  • HIP 91906 7.45 light-years
  • HIP 87079 13.6 light-years
  • HIP 94802 14.2 light-years
  • τ Dra 15.7 light-years
  • HIP 93007 15.7 light-years
  • HIP 85887 15.8 light-years

Open in the simulation

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