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Star · M

TOI-2274

TOI-2274 is a giant star of spectral type M in the constellation Lyra, 159.4 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationLyra
Distance159.4 light-years (48.9 pc)
Apparent magnitudemagnitude 11.95
Absolute magnitudemagnitude 8.50
Spectral typeM
Surface temperature3,940 K
Luminosity0.0866 L☉
Radius0.631 R☉
Mass0.612 M☉
Right ascension (J2000)18h 29m 50.3s
Declination (J2000)+40° 32′ 26″
Space velocity (relative to the Sun)28.8 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 11.95. Visible from the whole Northern Hemisphere and south to latitude 49° S. North of latitude 49° 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 1867. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.8 million years.

The Sun seen from there

From a planet around TOI-2274, the Sun would look like a star of magnitude 8.28, in the direction where our sky has the constellation Columba. It would be invisible to the naked eye.

Planets

Neighbours

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

  • HIP 91120 7.06 light-years
  • ε¹ Lyr 8.09 light-years
  • ε² Lyr 8.24 light-years
  • HIP 90415 8.25 light-years
  • ζ¹ Lyr 11.5 light-years
  • ζ² Lyr 11.5 light-years
  • HIP 91507 13.0 light-years
  • HIP 91058 17.4 light-years

Open in the simulation

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