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Star · G2V

Gl 225.2B

Gl 225.2B is a main-sequence star of spectral type G2V in the constellation Columba, 60.4 light-years from the Sun.

ConstellationColumba
Distance60.4 light-years (18.5 pc)
Apparent magnitudemagnitude 9.10
Absolute magnitudemagnitude 7.76
Spectral typeG2V
Surface temperature5,780 K
Luminosity0.0728 L☉
Radius0.269 R☉
Mass0.519 M☉ (estimated)
Right ascension (J2000)6h 00m 20.1s
Declination (J2000)−31° 01′ 46″
Space velocity (relative to the Sun)50.6 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 9.10. Visible from the whole Southern Hemisphere and north to latitude 59° N. South of latitude 59° S it never sets. It stands highest at midnight in December, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1966. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.1 million years.

The Sun seen from there

From a planet around Gl 225.2B, the Sun would look like a star of magnitude 6.17, in the direction where our sky has the constellation Hercules. 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.