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Star · F2IV

HIP 66257

HIP 66257 is a subgiant star of spectral type F2IV in the constellation Canes Venatici, 152.9 light-years from the Sun.

ConstellationCanes Venatici
Distance152.9 light-years (46.9 pc)
Apparent magnitudemagnitude 4.91
Absolute magnitudemagnitude 1.55
Spectral typeF2IV
Surface temperature6,860 K
Luminosity20.3 L☉
Radius3.19 R☉
Mass2.15 M☉ (estimated)
Right ascension (J2000)13h 34m 47.8s
Declination (J2000)+37° 10′ 57″
Space velocity (relative to the Sun)22.5 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 4.91). Visible from the whole Northern Hemisphere and south to latitude 53° S. North of latitude 53° N it never sets. It stands highest at midnight in April, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1873. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.7 million years.

The Sun seen from there

From a planet around HIP 66257, the Sun would look like a star of magnitude 8.19, in the direction where our sky has the constellation Sculptor. It would be invisible to the naked eye.

Neighbours

Its nearest neighbours in the catalogue (within 20 light-years):

  • HIP 65937 4.57 light-years
  • HIP 66514 6.97 light-years
  • HIP 65049 10.5 light-years
  • HIP 64747 10.6 light-years
  • HIP 66865 11.8 light-years
  • HIP 66712 12.1 light-years
  • HIP 66593 14.3 light-years
  • 2MASS J13120707+3937445 15.5 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.