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Star · G0V

HIP 103571

HIP 103571 is a main-sequence star of spectral type G0V in the constellation Equuleus, 179.5 light-years from the Sun.

ConstellationEquuleus
Distance179.5 light-years (55.0 pc)
Apparent magnitudemagnitude 5.24
Absolute magnitudemagnitude 1.54
Spectral typeG0V
Surface temperature6,590 K
Luminosity20.7 L☉
Radius3.49 R☉
Mass2.16 M☉ (estimated)
Right ascension (J2000)20h 59m 05.1s
Declination (J2000)+4° 17′ 41″
Space velocity (relative to the Sun)48.8 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.24). Visible from the whole Northern Hemisphere and south to latitude 86° S. It stands highest at midnight in August, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1846. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.2 million years.

The Sun seen from there

From a planet around HIP 103571, the Sun would look like a star of magnitude 8.53, in the direction where our sky has the constellation Hydra. 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.