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Star · F3V

HIP 97515

HIP 97515 is a main-sequence star of spectral type F3V in the constellation Sagittarius, 152.2 light-years from the Sun.

ConstellationSagittarius
Distance152.2 light-years (46.7 pc)
Apparent magnitudemagnitude 6.04
Absolute magnitudemagnitude 2.69
Spectral typeF3V
Surface temperature6,860 K
Luminosity7.1 L☉
Radius1.88 R☉
Mass1.63 M☉ (estimated)
Right ascension (J2000)19h 49m 11.6s
Declination (J2000)−28° 47′ 20″
Space velocity (relative to the Sun)49.7 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.04). Visible from the whole Southern Hemisphere and north to latitude 61° N. South of latitude 61° S it never sets. It stands highest at midnight in July, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1874. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.7 million years.

The Sun seen from there

From a planet around HIP 97515, the Sun would look like a star of magnitude 8.18, 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 98839 11.4 light-years
  • HIP 97531 11.5 light-years
  • HIP 97557 11.7 light-years
  • HIP 96854 12.7 light-years
  • HIP 98049 14.2 light-years
  • WISE J195113.62-331116.7 14.5 light-years
  • HIP 97512 15.7 light-years
  • HIP 95203 16.1 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.