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Star · M4.5 V

TOI-2136

TOI-2136 is a main-sequence star of spectral type M4.5 V in the constellation Lyra, 108.8 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationLyra
Distance108.8 light-years (33.4 pc)
Apparent magnitudemagnitude 14.13
Absolute magnitudemagnitude 11.51
Spectral typeM4.5 V
Surface temperature3,340 K
Luminosity0.013 L☉
Radius0.34 R☉
Mass0.34 M☉
Age4.6 billion years
Metallicity [Fe/H]0.03
Right ascension (J2000)18h 44m 42.3s
Declination (J2000)+36° 33′ 47″
Space velocity (relative to the Sun)28.5 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 14.13. Visible from the whole Northern Hemisphere and south to latitude 53° S. North of latitude 53° N it never sets. It stands highest at midnight in June, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1917. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.9 million years.

The Sun seen from there

From a planet around TOI-2136, the Sun would look like a star of magnitude 7.45, in the direction where our sky has the constellation Puppis. It would be invisible to the naked eye.

Planets

Neighbours

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

  • HIP 91326 6.16 light-years
  • HIP 92122 8.17 light-years
  • PSO J284.7214+39.3189 9.32 light-years
  • HIP 92532 11.3 light-years
  • HIP 90061 11.3 light-years
  • HIP 93350 13.0 light-years
  • HIP 89282 15.8 light-years
  • PSO J274.0908+30.5470 16.3 light-years

Open in the simulation

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