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Star · M 4.5V

GJ 1151

GJ 1151 is a main-sequence star of spectral type M 4.5V in the constellation Ursa Major, 26.2 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationUrsa Major
Distance26.2 light-years (8.04 pc)
Apparent magnitudemagnitude 13.25
Absolute magnitudemagnitude 13.72
Spectral typeM 4.5V
Surface temperature3,280 K
Luminosity0.00331 L☉
Radius0.178 R☉
Mass0.164 M☉
Metallicity [Fe/H]-0.12
Right ascension (J2000)11h 51m 01.4s
Declination (J2000)+48° 22′ 37″
Space velocity (relative to the Sun)77.3 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 13.25. Visible from the whole Northern Hemisphere and south to latitude 42° S. North of latitude 42° N it never sets. It stands highest at midnight in March, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 2000. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 465 thousand years.

The Sun seen from there

From a planet around GJ 1151, the Sun would look like a star of magnitude 4.36, in the direction where our sky has the constellation Phoenix. It would be visible to the naked eye.

Planets

Neighbours

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

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