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Star · M2 V

TOI-5799

TOI-5799 is a main-sequence star of spectral type M2 V in the constellation Aquila, 90.9 light-years from the Sun. It is orbited by 2 confirmed exoplanet(s).

ConstellationAquila
Distance90.9 light-years (27.9 pc)
Apparent magnitudemagnitude 13.30
Absolute magnitudemagnitude 11.08
Spectral typeM2 V
Surface temperature3,450 K
Luminosity0.0148 L☉
Radius0.321 R☉
Mass0.325 M☉
Age9.6 billion years
Metallicity [Fe/H]0.01
Right ascension (J2000)20h 06m 31.2s
Declination (J2000)+15° 59′ 21″
Space velocity (relative to the Sun)45.3 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 13.30. Visible from the whole Northern Hemisphere and south to latitude 74° S. North of latitude 74° 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 1935. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.6 million years.

The Sun seen from there

From a planet around TOI-5799, the Sun would look like a star of magnitude 7.05, 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 100511 8.75 light-years
  • GJ 4126 9.15 light-years
  • HIP 120148 9.89 light-years
  • HIP 99316 10.1 light-years
  • GJ 9689 10.6 light-years
  • HIP 100963 12.8 light-years
  • HIP 97051 13.8 light-years
  • HIP 99205 15.4 light-years

Open in the simulation

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