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Star · K0IV

Gl 57.1A

Gl 57.1A is a subgiant star of spectral type K0IV in the constellation Cetus, 98.0 light-years from the Sun.

Other namesHIP 6456
ConstellationCetus
Distance98.0 light-years (30.1 pc)
Apparent magnitudemagnitude 7.85
Absolute magnitudemagnitude 5.46
Spectral typeK0IV
Surface temperature5,000 K
Luminosity0.771 L☉
Radius1.17 R☉
Mass0.937 M☉ (estimated)
Right ascension (J2000)1h 23m 02.6s
Declination (J2000)−12° 57′ 58″
Space velocity (relative to the Sun)74.4 km/s

In the sky

Too faint for the naked eye (magnitude 7.85); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 77° N. South of latitude 77° S it never sets. It stands highest at midnight in October, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1928. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.7 million years.

The Sun seen from there

From a planet around Gl 57.1A, the Sun would look like a star of magnitude 7.22, in the direction where our sky has the constellation Virgo. It would be invisible 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.