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Star · F1IV

HIP 105652

HIP 105652 is a subgiant star of spectral type F1IV in the constellation Vulpecula, 169.3 light-years from the Sun.

ConstellationVulpecula
Distance169.3 light-years (51.9 pc)
Apparent magnitudemagnitude 5.70
Absolute magnitudemagnitude 2.12
Spectral typeF1IV
Surface temperature7,370 K
Luminosity12.2 L☉
Radius2.14 R☉
Mass1.87 M☉ (estimated)
Right ascension (J2000)21h 23m 58.8s
Declination (J2000)+24° 16′ 27″
Space velocity (relative to the Sun)36.2 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 5.70). Visible from the whole Northern Hemisphere and south to latitude 66° S. North of latitude 66° N it never sets. 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 1857. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.0 million years.

The Sun seen from there

From a planet around HIP 105652, the Sun would look like a star of magnitude 8.41, 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):

  • HIP 106296 8.54 light-years
  • HIP 106581 14.4 light-years
  • HIP 104124 16.4 light-years
  • HIP 106949 17.0 light-years
  • HIP 103784 18.0 light-years
  • HIP 103833 18.1 light-years
  • 1 Peg 18.1 light-years
  • HIP 106040 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.