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Star · K1IV

HIP 100852

HIP 100852 is a subgiant star of spectral type K1IV in the constellation Sagittarius, 128.1 light-years from the Sun.

ConstellationSagittarius
Distance128.1 light-years (39.3 pc)
Apparent magnitudemagnitude 6.24
Absolute magnitudemagnitude 3.27
Spectral typeK1IV
Surface temperature4,840 K
Luminosity6.26 L☉
Radius3.56 R☉
Mass1.58 M☉ (estimated)
Right ascension (J2000)20h 26m 53.0s
Declination (J2000)−37° 24′ 11″
Space velocity (relative to the Sun)57.2 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.24). Visible from the whole Southern Hemisphere and north to latitude 53° N. South of latitude 53° 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 1898. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.3 million years.

The Sun seen from there

From a planet around HIP 100852, the Sun would look like a star of magnitude 7.80, in the direction where our sky has the constellation Lynx. It would be invisible to the naked eye.

Neighbours

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

  • 2MASS J20414283-3506442 8.46 light-years
  • HIP 101432 10.6 light-years
  • HIP 101292 11.3 light-years
  • HIP 102580 12.5 light-years
  • HIP 101274 12.7 light-years
  • HIP 99926 17.1 light-years
  • HIP 103646 17.2 light-years
  • HIP 99966 17.3 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.