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Star · G0IV

HIP 39271

HIP 39271 is a subgiant star of spectral type G0IV in the constellation Canis Minor, 208.8 light-years from the Sun.

ConstellationCanis Minor
Distance208.8 light-years (64.0 pc)
Apparent magnitudemagnitude 6.22
Absolute magnitudemagnitude 2.19
Spectral typeG0IV
Surface temperature6,090 K
Luminosity11.8 L☉
Radius3.09 R☉
Mass1.85 M☉ (estimated)
Right ascension (J2000)8h 01m 50.7s
Declination (J2000)+8° 54′ 50″
Space velocity (relative to the Sun)13.7 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.22). Visible from the whole Northern Hemisphere and south to latitude 81° S. 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 1817. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.7 million years.

The Sun seen from there

From a planet around HIP 39271, the Sun would look like a star of magnitude 8.86, in the direction where our sky has the constellation Aquila. 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.