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Star · A0V

HIP 29997

HIP 29997 is a main-sequence star of spectral type A0V in the constellation Camelopardalis, 177.8 light-years from the Sun.

ConstellationCamelopardalis
Distance177.8 light-years (54.5 pc)
Apparent magnitudemagnitude 4.76
Absolute magnitudemagnitude 1.08
Spectral typeA0V
Surface temperature9,820 K
Luminosity42.5 L☉
Radius2.25 R☉
Mass2.65 M☉ (estimated)
Right ascension (J2000)6h 18m 50.8s
Declination (J2000)+69° 19′ 11″
Space velocity (relative to the Sun)31.4 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 4.76). Visible from the whole Northern Hemisphere and south to latitude 21° S. North of latitude 21° N it never sets. It stands highest at midnight in December, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1848. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.2 million years.

The Sun seen from there

From a planet around HIP 29997, the Sun would look like a star of magnitude 8.51, in the direction where our sky has the constellation Pavo. It would be invisible to the naked eye.

Neighbours

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

  • HIP 29421 7.92 light-years
  • HIP 31575 10.2 light-years
  • HIP 32945 11.6 light-years
  • HIP 28304 14.3 light-years
  • HIP 31528 16.7 light-years
  • HIP 30130 19.8 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.