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Star · M3

Gl 257B

Gl 257B is a supergiant star of spectral type M3 in the constellation Puppis, 26.2 light-years from the Sun.

ConstellationPuppis
Distance26.2 light-years (8.04 pc)
Apparent magnitudemagnitude 11.70
Absolute magnitudemagnitude 12.17
Spectral typeM3
Surface temperature2,980 K
Luminosity0.0212 L☉
Radius0.548 R☉
Mass1.2 M☉ (estimated)
Right ascension (J2000)6h 57m 47.4s
Declination (J2000)−44° 17′ 27″
Space velocity (relative to the Sun)44.9 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 11.70. Visible from the whole Southern Hemisphere and north to latitude 46° N. South of latitude 46° S it never sets. It stands highest at midnight in January, 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 Gl 257B, the Sun would look like a star of magnitude 4.36, in the direction where our sky has the constellation Lyra. 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.