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Star · M0 V

GJ 338 B

GJ 338 B is a main-sequence star of spectral type M0 V in the constellation Ursa Major, 20.7 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

Other namesGl 338B · HIP 120005
ConstellationUrsa Major
Distance20.7 light-years (6.33 pc)
Apparent magnitudemagnitude 7.70
Absolute magnitudemagnitude 8.69
Spectral typeM0 V
Surface temperature4,010 K
Luminosity0.0792 L☉
Radius0.58 R☉
Mass0.64 M☉
Age4.0 billion years
Metallicity [Fe/H]-0.03
Right ascension (J2000)9h 14m 24.7s
Declination (J2000)+52° 41′ 12″
Space velocity (relative to the Sun)52.6 km/s

In the sky

Too faint for the naked eye (magnitude 7.70); binoculars will find it. Visible from the whole Northern Hemisphere and south to latitude 37° S. North of latitude 37° N it never sets. 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 2005. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 366 thousand years.

The Sun seen from there

From a planet around GJ 338 B, the Sun would look like a star of magnitude 3.84, in the direction where our sky has the constellation Indus. It would be visible 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.