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Star · G3V

HIP 2237

HIP 2237 is a main-sequence star of spectral type G3V in the constellation Cetus, 105.0 light-years from the Sun.

ConstellationCetus
Distance105.0 light-years (32.2 pc)
Apparent magnitudemagnitude 6.44
Absolute magnitudemagnitude 3.90
Spectral typeG3V
Surface temperature5,990 K
Luminosity2.47 L☉
Radius1.46 R☉
Mass1.25 M☉ (estimated)
Right ascension (J2000)0h 28m 21.1s
Declination (J2000)−20° 20′ 06″
Space velocity (relative to the Sun)25.9 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.44). Visible from the whole Southern Hemisphere and north to latitude 70° N. South of latitude 70° S 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 1921. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 1.9 million years.

The Sun seen from there

From a planet around HIP 2237, the Sun would look like a star of magnitude 7.37, in the direction where our sky has the constellation Coma Berenices. 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.