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Star · K1 III

HIP 90988

HIP 90988 is a giant star of spectral type K1 III in the constellation Telescopium, 303.9 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationTelescopium
Distance303.9 light-years (93.2 pc)
Apparent magnitudemagnitude 7.75
Absolute magnitudemagnitude 2.90
Spectral typeK1 III
Surface temperature4,880 K
Luminosity7.76 L☉
Radius3.94 R☉
Mass1.61 M☉
Age4.6 billion years
Metallicity [Fe/H]0.17
Right ascension (J2000)18h 33m 33.4s
Declination (J2000)−50° 12′ 42″
Space velocity (relative to the Sun)38.5 km/s

In the sky

Too faint for the naked eye (magnitude 7.75); binoculars will find it. Visible from the whole Southern Hemisphere and north to latitude 40° N. South of latitude 40° 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 1722. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 5.4 million years.

The Sun seen from there

From a planet around HIP 90988, the Sun would look like a star of magnitude 9.68, in the direction where our sky has the constellation Auriga. It would be invisible to the naked eye.

Planets

Neighbours

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

  • HIP 90899 11.1 light-years
  • HIP 92165 15.6 light-years
  • HIP 91461 15.9 light-years
  • HIP 89460 18.9 light-years

Open in the simulation

Stellar parameters from the NASA Exoplanet Archive; position and brightness from the HYG / AT-HYG catalogue.