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Star · M2.0 V

TOI-1201

TOI-1201 is a main-sequence star of spectral type M2.0 V in the constellation Eridanus, 122.8 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationEridanus
Distance122.8 light-years (37.6 pc)
Apparent magnitudemagnitude 13.10
Absolute magnitudemagnitude 10.22
Spectral typeM2.0 V
Surface temperature3,480 K
Luminosity0.034 L☉
Radius0.508 R☉
Mass0.512 M☉
Metallicity [Fe/H]0.05
Right ascension (J2000)2h 48m 59.5s
Declination (J2000)−14° 32′ 14″
Space velocity (relative to the Sun)44.8 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 13.10. Visible from the whole Southern Hemisphere and north to latitude 75° N. South of latitude 75° S it never sets. It stands highest at midnight in October, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1903. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.2 million years.

The Sun seen from there

From a planet around TOI-1201, the Sun would look like a star of magnitude 7.71, in the direction where our sky has the constellation Boötes. It would be invisible to the naked eye.

Planets

Neighbours

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

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