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Star · A7V

HIP 90478

HIP 90478 is a main-sequence star of spectral type A7V in the constellation Sagittarius, 254.8 light-years from the Sun.

ConstellationSagittarius
Distance254.8 light-years (78.1 pc)
Apparent magnitudemagnitude 6.31
Absolute magnitudemagnitude 1.85
Spectral typeA7V
Surface temperature7,710 K
Luminosity16.1 L☉
Radius2.25 R☉
Mass2.01 M☉ (estimated)
Right ascension (J2000)18h 27m 43.8s
Declination (J2000)−26° 38′ 05″
Space velocity (relative to the Sun)32.1 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.31). Visible from the whole Southern Hemisphere and north to latitude 63° N. South of latitude 63° S it never sets. It stands highest at midnight in June, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1771. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 4.5 million years.

The Sun seen from there

From a planet around HIP 90478, the Sun would look like a star of magnitude 9.29, in the direction where our sky has the constellation Gemini. It would be invisible to the naked eye.

Neighbours

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

  • HIP 90510 5.43 light-years
  • HIP 90154 6.78 light-years
  • HIP 90504 9.24 light-years
  • HIP 90861 11.9 light-years
  • HIP 89829 16.2 light-years
  • HIP 91095 19.9 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.