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Star · A9IV

HIP 36807

HIP 36807 is a subgiant star of spectral type A9IV in the constellation Puppis, 269.0 light-years from the Sun.

ConstellationPuppis
Distance269.0 light-years (82.5 pc)
Apparent magnitudemagnitude 6.11
Absolute magnitudemagnitude 1.53
Spectral typeA9IV
Surface temperature7,480 K
Luminosity21.2 L☉
Radius2.74 R☉
Mass2.17 M☉ (estimated)
Right ascension (J2000)7h 34m 12.8s
Declination (J2000)−33° 27′ 48″
Space velocity (relative to the Sun)41.4 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.11). Visible from the whole Southern Hemisphere and north to latitude 57° N. South of latitude 57° S it never sets. It stands highest at midnight in January, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1757. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.8 million years.

The Sun seen from there

From a planet around HIP 36807, the Sun would look like a star of magnitude 9.41, in the direction where our sky has the constellation Cygnus. It would be invisible to the naked eye.

Neighbours

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

  • HIP 35877 11.5 light-years
  • HIP 35691 14.1 light-years
  • HIP 36897 16.1 light-years
  • HIP 38401 17.6 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.