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Star · K9V

TOI-2453

TOI-2453 is a main-sequence star of spectral type K9V in the constellation Orion, 267.8 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationOrion
Distance267.8 light-years (82.1 pc)
Apparent magnitudemagnitude 14.39
Absolute magnitudemagnitude 9.82
Spectral typeK9V
Surface temperature3,720 K
Luminosity0.0386 L☉
Radius0.502 R☉
Mass0.501 M☉
Right ascension (J2000)4h 59m 21.0s
Declination (J2000)+12° 56′ 11″
Space velocity (relative to the Sun)19.9 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 14.39. Visible from the whole Northern Hemisphere and south to latitude 77° S. North of latitude 77° N it never sets. It stands highest at midnight in December, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1758. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.7 million years.

The Sun seen from there

From a planet around TOI-2453, the Sun would look like a star of magnitude 9.40, in the direction where our sky has the constellation Ophiuchus. It would be invisible to the naked eye.

Planets

Neighbours

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

  • HIP 23492 6.24 light-years
  • HIP 23710 7.59 light-years
  • HIP 23085 9.51 light-years
  • HIP 22708 17.5 light-years
  • HIP 22712 17.6 light-years
  • HIP 22773 17.9 light-years
  • HIP 22021 19.0 light-years

Open in the simulation

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