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Star · M

TOI-5319

TOI-5319 is a main-sequence star of spectral type M in the constellation Aries, 198.3 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationAries
Distance198.3 light-years (60.8 pc)
Apparent magnitudemagnitude 14.17
Absolute magnitudemagnitude 10.25
Spectral typeM
Surface temperature3,580 K
Luminosity0.0347 L☉
Radius0.485 R☉
Mass0.5 M☉
Right ascension (J2000)2h 20m 51.3s
Declination (J2000)+23° 31′ 14″
Space velocity (relative to the Sun)27.7 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 14.17. Visible from the whole Northern Hemisphere and south to latitude 66° S. North of latitude 66° N 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 1828. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.5 million years.

The Sun seen from there

From a planet around TOI-5319, the Sun would look like a star of magnitude 8.75, in the direction where our sky has the constellation Hydra. It would be invisible to the naked eye.

Planets

Neighbours

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

  • HIP 10652 9.86 light-years
  • HIP 11329 13.8 light-years
  • HIP 10668 16.0 light-years
  • 2MASSI J0224367+253704 17.4 light-years
  • HIP 10351 17.7 light-years
  • HIP 11157 18.4 light-years
  • HIP 12820 19.6 light-years

Open in the simulation

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