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Star · G5

HIP 109384

HIP 109384 is a main-sequence star of spectral type G5 in the constellation Cepheus, 192.9 light-years from the Sun. It is orbited by 1 confirmed exoplanet(s).

ConstellationCepheus
Distance192.9 light-years (59.1 pc)
Apparent magnitudemagnitude 9.61
Absolute magnitudemagnitude 5.75
Spectral typeG5
Surface temperature5,180 K
Luminosity0.48 L☉
Radius0.831 R☉
Mass0.78 M☉
Metallicity [Fe/H]-0.26
Right ascension (J2000)22h 09m 37.4s
Declination (J2000)+71° 18′ 52″
Space velocity (relative to the Sun)94.7 km/s

In the sky

A telescope is needed to see it: its apparent magnitude is 9.61. Visible from the whole Northern Hemisphere and south to latitude 19° S. North of latitude 19° N 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 1833. At the speed of Voyager 1, the fastest craft leaving the Solar System (16.9 km per second), the trip would take 3.4 million years.

The Sun seen from there

From a planet around HIP 109384, the Sun would look like a star of magnitude 8.69, in the direction where our sky has the constellation Carina. It would be invisible to the naked eye.

Planets

Neighbours

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

  • 31 Cep 11.2 light-years
  • HIP 113517 14.9 light-years
  • 11 Cep 15.3 light-years
  • HIP 106914 16.5 light-years
  • HIP 112670 16.8 light-years
  • HIP 112946 19.4 light-years

Open in the simulation

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