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Star · M3V

Gl 875.1

Gl 875.1 is a main-sequence star of spectral type M3V in the constellation Pegasus, 49.3 light-years from the Sun.

Other namesHIP 112909
ConstellationPegasus
Distance49.3 light-years (15.1 pc)
Apparent magnitudemagnitude 11.66
Absolute magnitudemagnitude 10.76
Spectral typeM3V
Surface temperature3,790 K
Luminosity0.0156 L☉
Radius0.289 R☉
Mass0.31 M☉ (estimated)
Right ascension (J2000)22h 51m 53.5s
Declination (J2000)+31° 45′ 16″
Space velocity (relative to the Sun)37.8 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 11.66. Visible from the whole Northern Hemisphere and south to latitude 58° S. North of latitude 58° N it never sets. It stands highest at midnight in September, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1977. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 874 thousand years.

The Sun seen from there

From a planet around Gl 875.1, the Sun would look like a star of magnitude 5.73, in the direction where our sky has the constellation Hydra. It would be visible to the naked eye.

Neighbours

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

Open in the simulation

Position, brightness and colour from the HYG / AT-HYG catalogue; temperature, luminosity, radius and mass are approximate values computed from these observations.