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Star · K9V

K2-321

K2-321 is a main-sequence star of spectral type K9V in the constellation Sextans, 251.1 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationSextans
Distance251.1 light-years (77.0 pc)
Apparent magnitudemagnitude 13.65
Absolute magnitudemagnitude 9.22
Spectral typeK9V
Surface temperature3,750 K
Luminosity0.063 L☉
Radius0.595 R☉
Mass0.578 M☉
Metallicity [Fe/H]0.15
Right ascension (J2000)10h 25m 37.3s
Declination (J2000)+2° 30′ 50″
Space velocity (relative to the Sun)62.2 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 13.65. Visible from the whole Northern Hemisphere and south to latitude 87° S. It stands highest at midnight in February, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1775. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.5 million years.

The Sun seen from there

From a planet around K2-321, the Sun would look like a star of magnitude 9.26, in the direction where our sky has the constellation Aquarius. It would be invisible to the naked eye.

Planets

Neighbours

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

Open in the simulation

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