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Star · G1V

HIP 103077

HIP 103077 is a main-sequence star of spectral type G1V in the constellation Aquarius, 144.1 light-years from the Sun.

ConstellationAquarius
Distance144.1 light-years (44.2 pc)
Apparent magnitudemagnitude 6.38
Absolute magnitudemagnitude 3.15
Spectral typeG1V
Surface temperature5,740 K
Luminosity5.12 L☉
Radius2.29 R☉
Mass1.5 M☉ (estimated)
Right ascension (J2000)20h 53m 05.6s
Declination (J2000)−11° 34′ 25″
Space velocity (relative to the Sun)13.3 km/s

In the sky

Visible to the naked eye under a dark sky (apparent magnitude 6.38). Visible from the whole Southern Hemisphere and north to latitude 78° N. South of latitude 78° S it never sets. It stands highest at midnight in August, the best time to observe it.

Through a telescope from Earth

Light's journey

The light you see tonight set out around the year 1882. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 2.6 million years.

The Sun seen from there

From a planet around HIP 103077, the Sun would look like a star of magnitude 8.06, in the direction where our sky has the constellation Cancer. It would be invisible to the naked eye.

Neighbours

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

  • μ Aqr 6.53 light-years
  • HIP 102664 9.07 light-years
  • HIP 104331 11.4 light-years
  • HIP 103349 12.5 light-years
  • SDSS J204317.69-155103.4 12.7 light-years
  • HIP 103311 15.4 light-years
  • HIP 104687 16.8 light-years
  • θ Cap 17.2 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.