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Star · F2

HIP 41282

HIP 41282 is a main-sequence star of spectral type F2 in the constellation Puppis, 112.5 light-years from the Sun.

ConstellationPuppis
Distance112.5 light-years (34.5 pc)
Apparent magnitudemagnitude 6.01
Absolute magnitudemagnitude 3.32
Spectral typeF2
Surface temperature6,870 K
Luminosity3.98 L☉
Radius1.41 R☉
Mass1.41 M☉ (estimated)
Right ascension (J2000)8h 25m 19.0s
Declination (J2000)−21° 02′ 46″
Space velocity (relative to the Sun)11.6 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.01). Visible from the whole Southern Hemisphere and north to latitude 69° N. South of latitude 69° 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 1914. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.0 million years.

The Sun seen from there

From a planet around HIP 41282, the Sun would look like a star of magnitude 7.52, in the direction where our sky has the constellation Vulpecula. It would be invisible to the naked eye.

Neighbours

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

  • GJ 9269 9.00 light-years
  • HIP 42281 10.6 light-years
  • HIP 42108 10.7 light-years
  • HIP 42910 11.0 light-years
  • HIP 41609 11.7 light-years
  • GJ 3493 11.9 light-years
  • COCONUTS-3B 13.1 light-years
  • HIP 41134 13.3 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.