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Star · F2V

HIP 8588

HIP 8588 is a main-sequence star of spectral type F2V in the constellation Aries, 135.7 light-years from the Sun.

ConstellationAries
Distance135.7 light-years (41.6 pc)
Apparent magnitudemagnitude 5.92
Absolute magnitudemagnitude 2.82
Spectral typeF2V
Surface temperature7,450 K
Luminosity6.42 L☉
Radius1.52 R☉
Mass1.59 M☉ (estimated)
Right ascension (J2000)1h 50m 52.0s
Declination (J2000)+11° 02′ 36″
Space velocity (relative to the Sun)18.7 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.92). Visible from the whole Northern Hemisphere and south to latitude 79° S. North of latitude 79° N 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 1890. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.4 million years.

The Sun seen from there

From a planet around HIP 8588, the Sun would look like a star of magnitude 7.93, 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.