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Star · F6IV

HIP 102011

HIP 102011 is a subgiant star of spectral type F6IV in the constellation Cepheus, 108.5 light-years from the Sun.

ConstellationCepheus
Distance108.5 light-years (33.3 pc)
Apparent magnitudemagnitude 6.02
Absolute magnitudemagnitude 3.41
Spectral typeF6IV
Surface temperature6,660 K
Luminosity3.68 L☉
Radius1.44 R☉
Mass1.39 M☉ (estimated)
Right ascension (J2000)20h 40m 17.9s
Declination (J2000)+60° 30′ 19″
Space velocity (relative to the Sun)32.5 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.02). Visible from the whole Northern Hemisphere and south to latitude 29° S. North of latitude 29° N it never sets. It stands highest at midnight in July, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1917. 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 102011, the Sun would look like a star of magnitude 7.44, in the direction where our sky has the constellation Carina. It would be invisible to the naked eye.

Neighbours

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

  • HIP 101593 8.56 light-years
  • WISEA J201204.11+672608.0 14.3 light-years
  • HIP 106286 15.2 light-years
  • HIP 99355 16.6 light-years
  • GJ 9706 16.8 light-years
  • HIP 107191 17.6 light-years
  • HIP 104225 18.1 light-years
  • GJ 4150 18.2 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.